PLACE IN RETURN BOX to remove this checkout from your record. TO AVOID FINES return on or betore dete due. “- DATE DUE DATE DUE DATE DUE MSU In An AMrmdive AotlonlEquel Opportunity Institution Hlfll RESOLUTION INFRARED SPECTROSCOPY 0F Cfléf, CD31, AND CD Dr AND 3 INFRARED—RADIOFREQUENCY DOUBLE RESONANCE SPECTROSCOPY 0F CD31 AND CD3Br By Han—Gook Cho A DISSERTATION Submitted to Michigan State University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Department of Chemistry 1989 moonw- ABSTRACT HIGH RESOLUTION INFRARED SPECTROSCOPY OF CR3F, CD31, AND CDBBr AND INFRARED-RADIOFREOUENCY DOUBLE RESONANCE SPECTROSCOPY 0? CD31 AND CD3Br BY Han-Cook Cho The v3+v6-v6 band of CH3F and the v2 bands of CD31 and CD3Br have been recorded by means of an infrared microwave sideband laser (IMSL) spectrometer and analyzed by vibration-rotation theory including coupling with nearby vibrational states. The frequency measurement and analysis were performed in order to obtain frequency information for subsequent double resonance studies as well as to investigate the effect of various energy couplings. It has been possible to record the lineshapes of high J and K transitions at Doppler-limited resolution and to use the measured frequencies to determine molecular constants including high order centrifugal distortion constants for the ground and excited vibrational states. In the infrared spectrum of CHBF the high resolution allowed, in addition to the measurement of conventional transitions, the observation of 14 l-type doublets between two degenerate vibrational states. As a result, the infrared frequencies in the 03+96-v6 band can be reproduced with the molecular constants to within a few MHz, which is accurate enough for most double resonance studies. In CD31 and CDBBr analysis of the v2 vibration-rotation ii structure also led to molecular constants that can predict the frequencies to within a few MHz. These frequencies were used for double resonance experiments in this work. Infrared-radiofrequency double resonance, which has already been recognized as a very sensitive and precise method for the observation of various hyperfine energy structures, was used to record pure quadrupole transitions of CD31 and C038r for the ground and the v2 vibrational states. The data were analyzed by means of exact diagonalization of the total Hamiltonian matrix composed of the rotational and quadrupole interaction parts. The IMBL spectrometer employed as the infrared pumping source had sufficient tunability to make it possible to select for study an appropriate set of transitions without having to depend on accidental coincidences with laser lines. Consequently, it was possible to make precise measurements of a large number of transitions and to determine the spin-rotation constants as well as the centrifugal distortion constants for the quadrupole coupling in these molecules. During the fitting of the frequencies of the pure quadrupole spectra, it became evident that some effect was causing an apparent shift of the transitions, especially at low RF-frequencies. The shift has been traced to a double—resonance effect that appears in calculations when four interacting levels are taken into account, but is not evident in calculations based on the usual three-level system employed for double-resonance theory. An appropriate linear equation was set up in the density matrix fbrmalism for the four-interacting- level system, and solved at each RF-frequency for a sequence of values of the molecular velocity and for a fixed value of the laser frequency. The agreement between the experimental and the calculated spectra iii obtained for both the frequency shift and the distorted lineshape strongly confirms the four-interacting-level double-resonance effect. iv To the Memory of Bo-Kyoung ACKNOWLEDGMENTS I would like to thank Dr. R. H. Schwendeman for his guidance and encouragement throughout the course of this study and the preparation of this thesis. I wish to thank the other members of our group for their cooperation in the laboratory. The partial support from the National Science Foundation is gratefully acknowledged. vi TABLE OF CONTENTS LIST OF TABLES . . . . . . . . . . . . . . . . . . . . . . . . x LIST OF FIGURES . . . . . . . . . . . . . . . . . . . . . . . xii CHAPTER I INTRODUCTION . . . . . . . . . . . . . . . . . . . 1 CHAPTER II HIGH RESOLUTION INFRARED STUDY OF THE D +v -v 12 3 6 6 BAND OF CH3F . . . . . . . . . . . . . . . . . . 6 11-1 Introduction . . . . . . . . . . . . . . . . . . . . 6 11-2 Theory . . . . . . . . . . . . . . . . . . . . . . . 10 II-2-l Hamiltonian for Harmonic Oscillator-Rigid Rotor Approximation . . . . . . . . . . . . . . . . . ll II-2-l-l Harmonic Oscillator . . . . . . . . . . . . 12 II-2-l-2 Rigid Rotor . . . . . . . . . . . . . . . . 16 II-2-2 Selection Rules . . . . . . . . . . . . . . . . 22 11-2-3 Nonrigid Symmetric Top Molecules . . . . . . . . 27 II-2-3-l Centrifugal Distortion . . . . . . . . . . 27 II-2-3-2 Coriolis Interaction . . . . . . . . . . . 3O II-2-3-3 Rotational l-type Resonance Interaction . . 35 11-3 Experimental . . . . . . . . . . . . . . . . . . . . 40 II-3-l White-Type Long Path Cell . . . . . . . . . . . 40 II-3-2 Infrared-Microwave Sideband Laser Spectrometer . 43 11-4 Results . . . . . . . . . . . . . . . . . . . . . . . 49 II-4-l Term Values and Selection Rules . . . . . . . . 49 11-4-2 Analysis . . . . . . . . . . . . . . . . . . . . 52 11-5 Discussion . . . . . . . . . . . . . . . . . . . . . 65 11-6 Appendix . . . . . . . . . . . . . . . . . . . . . . 69 11-? References . . . . . . . . . . . . . . . . . . . . . 71 CHAPTER III HIGH RESOLUTION INFRARED SPECTROSCOPY OF THE v2 BANDS 0? CD31 AND CD3Br . . . . . . . . . . . . . 73 III-l Introduction . . . . . . . . . . . . . . . . . . . . 73 III-2 Theory . . . . . . . . . . . . . . . . . . . . . . . 79 III-2-l Term Values . . . . . . . . . . . . . . . . . . 79 vii III-2-2 Coriolis Interaction III-2-2-l CD31 III-2-2-2 CD38r . . . . . . . . . . . . . III-2—3 Effect of Nuclear Quadrupole Coupling . III-2-4 Hypothetical Unsplit Frequencies III-2-4-1 CD31 . III-2-4—2 CD33r III-3 Experimental . III-4 Results III-4-l CD I 3 III-4-2 CD3Br . III-5 Discussion . III-5-1 CD31 III-5-2 CDBBr . III-6 References . CHAPTER IV INFRARED-RADIOFREQUENCY DOUBLE RESONANCE OF CDBI AND CD3Br IV-l Introduction IV-l-l CD31 . IV-l-2 CD3Br IV-2 Theory IV-2—l IR-RF Double Resonance . IV-2-2 Nuclear Quadrupole Coupling IV-2—3 Irreducible Tensor Method IV-2-4 Quadrupole Interaction Energy IV-2-5 Quadrupole Coupling of CD31 and CD38r IV-3 Experimental IV~4 Results and Discussion IV-4-l CD I . 3 IV-4-2 CD3Br IV-4-3 Other Aspects IV-5 Appendix IV—6 References viii 79 80 82 EEEEB 91 91 97 121 121 124 125 127 127 131 132 135 135 137 141 142 145 148 155 155 163 173 177 178 CHAPTER V FOUR-INTERACTING-LEVEL DOUBLE RESONANCE . . . . . . 181 V-l Introduction . . . . . . . . . . . . . . . . . . . . . 181 V-2 Theory . . . . . . . . . . . . . . . . . . . . . . . . 185 V-3 Results and Discussion . . . . . . . . . . . . . . . . 192 V-4 References . . . . . . . . . . . . . . . . . . . . . . 198 ix LIST OF TABLES Table 2-1 Observed Transition Frequencies from R-type Doublets of 12 the v3+v6 ”6 Band of CH3F 2-2 Comparison of Observed and Calculated Frequencies in 12 the v3+v6 v6 Band of CH3F 1 State of 12CH3F 2-3 Molecular Constants of the v6 2-4 Molecular Constants of the v3 4 State of lzcngr 1, v6 = 1 Vibrational 2-5 Coincidences between Calculated Frequencies for the 12 v3+06-v6 Band of CH3F and Laser Frequenc1es 3-1 Comparison of Observed and Calculated Frequencies in the v2 Band of CD31 3-2 Comparison of Ground State Rotational Constants of CD31 . . . . 3-3 Molecular Constants of the v2 1 State of CD31 without Coriolis Correction 3-4 Molecular Constants of the v2 1 State of CD31 with Coriolis Correction 3-5 Coincidences between Calculated Frequencies for the v2 Band of CD31 and Laser Frequencies . 3-6 Comparison of Observed and Calculated Frequencies in the v Band of CD 79Br . . . . . . . . . . . . . 2 3 Page 55 58 63 64 67 92 98 99 100 101 104 3-8 3-9 3-10 3-11 4-6 4-7 4-8 4-9 Comparison of Observed and Calculated Frequencies in the 0 Band of CD 81Br . 2 3 Molecular Constants of CD37gBr . Molecular Constants of CD3813r ....... Coincidences between Calculated Frequencies for the v Band of CD37QBr and Laser Frequencies 2 Coincidences between Calculated Frequencies for the v2 Band of CD381Br and Laser Frequencies Pure Quadrupole Frequencies of CD31 Infrared Pumping Frequencies for IR—RF Double Resonances of CD31 . . . . . . . . . . . . . Quadrupole and Spin-Rotation Interaction Parameters of CD31 . Pure Quadrupole Frequencies of CD37gBr Pure Quadrupole Frequencies of CD38lBr Quadrupole and Spin-Rotation Interaction Parameters of 79 CD3 Br ....................... Quadrupole and Spin-Rotation Interaction Parameters of 81 CD3 Br . . . . . . . . .......... F = J+1/2 . F = J-1/2 Transitions of CD37QBr . F = J+1/2 . F = J—1/2 Transitions of CD 81Br . 3 xi 109 114 115 117 119 157 161 162 164 .1167 170 171 174 175 LIST OF FIGURES Figure Page 2-1 Symmetry properties of rotational levels of molecules with a three-fold axis; (a) in a totally symmetric vibrational state, (b) in a degenerate vibrational state. The arrows show allowed transitions. . . . . . . . . . . 28 2-2 The rovibronic levels with K = 1 and J = 1,2 for vibronic E-states of a molecule of symmetry C3v' The transitions indicated by solid arrows are allowed; those indicated by dashed arrows are not. . . . . . . . . . . . . . . . . . 29 2-3 Coriolis forces during the degenerate vibration of an X3 molecule. . . . . . . . . . . . . . . . . . . . . . . . 32 2-4 Diagrammatic representation of the x,y—Coriolis coupling of the states with J = 3 and with the same k-lt. The dotted line connects states exhibiting giant l-type doubling. . . . . . . . . . . . . . . . . . . . . . . . 32 2-5 qé+), qé-), and rt l-resonance in an It = :1 degenerate state of an oblate symmetric top. The levels are labeled by K, with (+1) to the left of (-1); interactions are shown by broken lines. . . . . . . . . . . . . . . . . . 39 2-6 Mirror arrangement of a White-type cell. The small circles on mirror surface are the centers of curvature of the mirrors. . . . . . . . . . . . . . . . . . . . . . . 41 2-7 Modified optical arrangement for a White-type cell. The numbers show the sequence of reflection. . . . . . . . . 41 2-8 Block diagram of the infrared microwave Sideband laser xii 2-10 2-11 3-1 3-2 used in this study. . . . . ............ . . . 44 Portion of the spectrum of the v3+v6-v6 band Observed in the present work. The horizontal axis is the microwave frequency to be added to (+) or subtracted from (-) the 12 16 frequency of the 9P(12) C 02 laser to obtain the infrared frequency of the transition. . . . . . . . . . 46 Portion of the spectrum of the v3+v6-06 band observed in the present work. The horizontal axis is the microwave frequency to be added to (+) or subtracted from (-) the frequency of the 9P(6) 12C16O2 laser to obtain the infrared frequency of the transition. The transition marked 2123 is in the 2123-1)3 band and completely absorbs the positive sideband power. ........... . . . 47 Energy-level diagrams showing higher frequency (solid lines) and lower frequency (dashed lines) allowed transitions between rotational levels belonging to two vibrational states of E symmetry for C3v. For each of the diagrams, the J value of the levels in the lower state is assumed to be odd and the qv value of the lower state is assumed to be positive; the sign of the qv value (qu) for the rotational levels of the upper state is indicated above each diagram. ........ . . . . . 51 Block diagram of the infrared microwave sideband laser spectrometer used to record the Doppler-limited vibration- rotation spectra in this work. ...... . . . . . . 88 A portion of the infrared spectrum of the 02 band of CD31 recorded by the infrared microwave sideband laser spectrometer. The microwave frequency on the horizontal axis is added to (+) or subtracted from (-) the frequency 12 16 of the 10P(28) C 02 laser to obtain the infrared xiii 3-3 frequency. The sample pressure was 0.3 Torr and a l-m path length was used. ....... . ...... . . . 89 A small portion of the spectrum in the v2 band region of CD3Br showing the typical lineshapes and signal/noise obtained for the spectra reported. The horizontal scale is the microwave frequency that must be subtracted from the frequency of the 12C1602 10(28) laser to obtain the infrared frequency of the transitions. Transitions of CD379Br and CD3BIBr occur approximately alternately everywhere in this region. .............. . 90 Three level system showing double resonance technique. The infrared radiation pumps molecules from ll) to l2) according to the Doppler shift resonance condition v12 = vIR(1tv/c) which appears as "holes" in the Maxwellian velocity profile of ll) and "spikes" in |2>. The radiofrequency will then transfer the "spikes" from |2> to [3) creating deeper "holes" in ll). This causes an increase in the molecular absorption. The radiofrequency transition from l2) to l3) can thus be observed by detecting the infrared radiation. . . . . . . . . . . . 136 Block diagram of the infrared radiofrequency double- resonance spectrometer used to record the pure quadrupole transitions in this work. An infrared microwave sideband laser in the cavity mode serves as the infrared pumping source. A radiofrequency synthesizer whose output is chopped by a double-balanced mixer and amplified serves as the radiofrequency source. ....... . . . . . . 149 A portion of the infrared radiofrequency double resonance spectrum obtained by pumping the P(22,5) transition in the v band of CD I. The F quantum numbers of the 2 3 transitions in the upper and lower states of the xiv 4-4 5-1 vibration-rotation transition are shown. The horizontal axis is the absolute radiofrequency. the sample pressure was 3 mTorr and l-m path length was used. ..... . . 152 Example of infrared radiofrequency double resonance spectra obtained in the present study for CD3798r. For these transitions, the infrared sideband laser source was tuned to the center frequency of the Doppler-limited lineshape of the P(22,6) transition in the 02 hand. For the infrared microwave sideband laser source, the 10R(26) 1201602 laser was used with a microwave frequency of 11726 MHz; the lower frequency sideband was used. . . . 153 Example of infrared radiofrequency double resonance spectra obtained in the present study for CD3alBr. For these transitions, the infrared sideband laser source was tuned to the center frequency of the Doppler-limited 2 hand. For the infrared microwave sideband laser source, the 10R(18) 1201602 laser was used with a microwave frequency of 9747 lineshape of the P(30,6) transition in the v MHz; the lower frequency sideband was used. . . . . . . 154 Typical energy level pattern for the infrared radiofrequency double resonances observed for CD31. In most cases, a single infrared frequency pumps all of the allowed infrared transitions by interacting with molecules in different velocity groups. . . . . . . . . . . . . . 156 Typical energy level pattern for the infrared radiofrequency double resonance observed for CD3Br. A single infrared frequency pumps all of the allowed infrared transitions by interacting with molecules in different velocity groups. In general, four high- frequency an two low-frequency double resonances were observed for each infrared transition. . . . . . . . . . 182 XV 5-2 5-3 Energy level diagram for the four-interacting-level double resonance system. . . . . . . . . . . . . . . . . . . . 183 Comparison of observed and calculated infrared radiofrequency double resonance spectra for a four- interacting—level double resonance system. The upper trace is the calculated spectrum and the lower trace is the observed spectrum. The points below each trace are the residuals obtained when the lineshape is fitted by least squares to a sum of two Lorentz lineshapes. The experimental spectrum was observed with a sample pressure of 4 mTorr, infrared power ~2 mW, and radiofrequency power ~20 aw. The theoretical spectrum was calculated by means of Equation (5-26) with all xi = 20 kHz and with kd = k0 = 100 kHz. For the experimental spectrum, the infrared frequency was set at the center frequency of the Doppler- limited lineshape of the P(26,4) transition in the v2 band of CD37QBr; the 10R(22) 12C1602 laser was used with the lower frequency sideband generated by a microwave frequency of 12632 MHz. . . . . . . . . . . . . . . . . 194 Plot of the frequency shift caused by the four- interacting-level double resonance effect against the assumed frequency splitting between the two lower frequency hyperfine transitions for the conditions described in Fig. 5-3. The vertical axis is the difference in frequency between the center of the best Lorentz line approximation to the calculated lineshape and the assumed hyperfine frequency for the lower- frequency component of the infrared radiofrequency double resonance doublet. All of the conditions for the calculated lineshape in Fig. 5—3 apply, except that the difference between the hyperfine frequency in the upper vibrational state (vcd) and that in the lower xvi vibrational state (vba) is varied. This difference is plotted on the horizontal axis. . . . . . . . . . . . 196 xvii CHAPTER I INTRODUCTION Studies of the vibrational-rotational spectra of polyatomic molecules in the gaseous phase provide considerable information including intermolecular distances and angles, the vibrational frequencies and force constants, dissociation energies, and other data concerning the structures of the molecules. The information attainable from studies of the vibrational-rotational spectra of polyatomic molecules has recently been greatly increased by the advent of laser spectroscopy and by considerable progress in the theoretical and experimental studies of the fine structure of the vibrational-rotational spectra of molecules. For the research reported in this dissertation, high resolution spectroscopy was performed for the purpose of Obtaining frequency information for subsequent double resonance studies as well as for examination of the effect of various energy couplings. The purpose of this "Introduction" is to provide an outline of the organization of this dissertation. More details concerning the reasons for carrying out the work, results of previous studies, etc., are given in the chapters describing each project. Chapter 11 presents the high resolution infrared spectroscopy of the v3+06-v6 band of 12CH'3F by means of an infrared microwave sideband laser (IMSL) spectrometer. This band is located in the vibrational spectrum of CH3F in the important 10 pm region, which has been the l subject of many high resolution studies. Moreover, this band is of interest because it appears to be the first example of a high-resolution infrared study of an E~E band in a prolate C symmetric top. More than 3v 200 transitions with J and K values up to 20 and 10, respectively, have been identified and their frequencies measured to an accuracy of a few MHz. Among the identified transitions are the components of 14 l—type doublets in this hot band of E~E symmetry. The spectra have been fit to experimental accuracy by adjusting rotational parameters including centrifugal distortion constants through the sixth order as well as Coriolis coupling and l-resonance parameters. In Chapter III, high resolution infrared studies of the v2 bands of 79 CD 1, CD3 Br, and CD38lBr are described. About 200 transitions for 3 each species have been recorded and the frequencies have been determined to an accuracy of few MHz. The frequencies in these parallel bands have been fit by least squares to an energy expression containing centrifugal distortion parameters up to the eighth order. The strong Coriolis interaction with the 05 band has been taken into account in each case by using previously-reported parameters for the interaction and for the 95 band (for CD3I, interaction with the 2173 state has been also included). The resulting combination of the v2 parameters obtained in this work and the parameters from previous work is sufficient for each molecule to predict the vz-band frequencies up to high J and K (~40 and ~10) within a few MHz. Radiofrequency spectroscopy is known to be a powerful tool for investigation of various hyperfine energy structures. However, the scope of the technique has been seriously limited by the density of the spectra and the poor signal-to-noise ratio. When infrared- radiofrequency double resonance was introduced, which involves the simultaneous application of two fields of radiation to the sample, radiofrequency spectroscopy could be performed with greatly enhanced sensitivity and selectivity. In infrared-radiofrequency double resonance, hyperfine resonances are observed as a steady-state change in absorption of laser power simply due to the change in the population difference between the excited and ground states as the RF frequency passes through resonance. A molecular population change is made possible by pumping molecules from the ground state to the upper vibrational state by means of a strong infrared laser field which is resonant with an infrared transition. When the RF-field is resonant with the hyperfine levels, infrared absorption is increased by equilibrating the populations of the hyperfine energy states. The development of IR-RF double resonance spectroscopy in the last two decades has made it possible to determine the values of a large number of parameters for hyperfine states, and many of these can be used for the investigation of the electron distribution in molecules. These parameters are usually measures of weak interaction occurring between atomic nuclei having electric quadrupole moments and electrons, and as such yield information about the electronic structure of the molecule. As will be seen in Chapter IV, the nuclear quadrupole coupling energy is given as the inner product of the nuclear quadrupole tensor and the electrostatic field-gradient tensor evaluated at the nucleus. Such an inner product depends on the mutual orientation of the two axis systems to which the two tensors are referred; for the nuclear quadrupole tensor, the natural system is one in which one axis coincides with the spin axis of the nucleus. The interest in quadrupole coupling constants 4 lies in the different values of the field gradient seen by a given nucleus in different molecular environments. The electric field gradient at the nucleus may be extracted from the quadrupole interaction energy represented by the quadrupole coupling constants, by dividing by the appropriate nuclear quadrupole moment. The IR-RF double resonance technique has been applied to the v2 and 3798r, and CD381 IMSL as the infrared laser pump. The tunability of the laser allowed the ground vibrational states of CD31, CD Br by using an the selection of an appropriate set of transitions with a wide range of J and K quantum numbers without having to depend on accidental coincidences with laser lines; more than 150 pure quadrupole transitions for each species have been observed. To improve the accuracy of the frequency measurement, the RF radiation power was kept as low as is consistent with reasonably good signal-to-noise ratio, because IR-RF spectra are easily RF power broadened. The typical half width at half maximum for the transitions was as low as 70 and 100 kHz for 003I and CDBBr, respectively. As a result, it was possible to determine the spin-rotation constants as well as the centrifugal distortion constants for the quadrupole couplings in these molecules. The theoretical and experimental details are described in Chapter IV. During the IR-RF double resonance study stated above, it was realized that some effect was causing an apparent shift of the transitions that occur at low RF frequencies. This effect could be easily shown through the adjustment of parameters to fit the frequencies of the pure quadrupole spectra; experimental values for the two lowest radiofrequency transitions were found to be much closer together than predicted by the best values of the parameters. These shifts were 5 traced to a double-resonance effect that appears in calculations when four interacting levels are taken account, but is not evident in calculations based on the usual three-level system employed for double- resonance theory. The nature of the problem is described in detail in Chapter V. Essentially, it results from the fact that the hyperfine splittings in the upper state are not greatly different from those in the lower state for the double resonances in this work. As a result, quadrupole transitions of the upper and the lower vibrational states are often overlapped, and, generally, the lower frequencies are more seriously overlapped than the higher frequencies. Since both the upper and the lower states of the RF transitions are pumped by the strong infrared radiation and the RF radiation connects the hyperfine levels, the four levels must be considered as a four-interacting-level system. An appropriate linear equation was set up in the density matrix fermalism for the four-interacting-level system, and solved at each RF frequency for a sequence of values of the molecular velocity and a fixed value of the laser frequency; the resulting contributions to the absorption were multiplied by the appropriate Doppler weight and summed. The frequency shifts obtained by fitting the spectra calculated with estimated parameters show good agreement with the shifts observed experimentally. The details are described in Chapter V. CHAPTER II HIGH RESOLUTION INFRARED STUDY OF THE D - v BAND OF 12CH'3F 3””6 6 II-l Introduction Methyl fluoride and ammonia, with their relatively simple rotational structure and strong spectra, have been considered as model compounds in the development of infrared high resolution spectroscopy. Especially, the vibrational spectrum of CH3F in the 10 pm region has been the subject of a number of recent high-resolution infrared studies because the many strong transitions in this region include several that are in coincidence with 002 lasers, and therefore provide pumping sources for far-infrared lasers and for double-resonance effects. For this molecule, a series of spectroscopic works have been performed by means of infrared-microwave two-photon and infrared-microwave laser spectroscopy in our laboratory (1-3). As a result of extensive analyses for the v3 fundamental and 2123 - v3 hot bands of 12CH3F and 13CH3F, transition frequencies can be calculated to within a few MHz with the reported molecular constants. The obtained information has been successfully applied to an infrared-infrared double-resonance study of collisional energy transfer including a determination of the change in velocity upon collision (4). This chapter is concerned with a high resolution infrared study of l O- the v3 + v6 v6 band (1039.1 cm- ) of 12CH3F carried out with infrared 7 microwave sideband laser spectroscopy. Like other XY23 type symmetric top molecules, CHBF has three totally symmetric and three doubly degenerate vibrational bands. Among these, O3 is the totally symmetric C-F stretching band (1048.6 cm-l), vs the degenerate CH3 rocking band 1 (1182.7 cm‘l), and v3+v6 the combination band (2221.8 cm- ). Although the upper and lower state energy levels of the v3 + OS - band in CH3F ”6 have been studied previously during investigations of other bands by infrared and microwave spectroscopy (5—9), the present work is the first extensive high-resolution study of this hot band. Values for the vibrational energy and primary rotational parameters (A, B, and A!) of the v6 = 1 state were obtained by Smith and Mills from grating spectra taken at 0.2 - 0.4 cm.1 resolution (5). Hirota and his co-workers later determined B, A{nK, and |q6| by means of microwave spectroscopy (6,2). Later, Hirota, by means of diode laser spectroscopy, observed Q-branch transitions in the v6 band for J and K values up to 14 and 3, respectively (8). The frequencies of these transitions were used together with rotational frequencies to determine A, A{, A{nK, the band center (D0 + Afz), and the sign of qv for v6 = l. A set of constants for the v3 + OS state was determined by Nakagawa gt g1. from grating spectra taken at 0.06 cm-1 resolution (2). However, they were unable to assign Ak = -1 spectra and could not determine an accurate value for the l-doubling constant qv. A final piece of information on the spectrum of interest in the present work is the assignment of the QQ(6,4) transition in the v3 + OS - v6 band by an optical-optical double resonance method by Duxbury and Kate (19). In addition to its importance for double resonance experiments, the D3 + OS - ”6 band is also of interest because it appears to be the first 8 example of a high-resolution infrared study of an E - E band in a prolate C3v symmetric top. Previous high-resolution studies of transitions between doubly-degenerate vibrational states have included analyses of the 03h molecule BF3 (11) and the oblate 03v molecules CF3H (lgfimd CF30 (Li) . In the present study, infrared spectra of the v3 + OS - ”6 band in 12CH3F have been recorded at Doppler-limited resolution (ADD 5 34 MHz) by an infrared microwave sideband laser spectrometer with a White-type long path absorption cell. The frequencies of more than 230 transitions have been measured to an accuracy of a few MHz. The measured frequencies include transition frequencies from 14 l-type doublets which allow the determination of l-type doubling constants for both the upper and the lower vibrational states. For this work, it was first necessary to identify all of the transitions of the fundamental v3 bands of 12CH3F and 13CH3F (which occurs in natural abundance) and of the 2v3 - 9 hot 3 band of 12CH3F; the absorption lines in these bands dominate the spectra in this region. All of the observed transitions in the 03 + OS - v6 band that were assigned in the present study follow the selection rule, Ak = 0, A1 = 0. Spectra obeying other selection rules may also occur as a result of rotational R-type resonances, but they have not yet been identified, probably because of exceedingly weak transition intensities. The spectra were fit to experimental accuracy by adjusting rotational parameters, including centrifugal distortion constants through the 6th order, diagonal Coriolis coupling parameters, and l-doubling constants. It is expected that the results of the present work will be applied to a subsequent energy transfer study between nearby vibrational states with predicted 002 laser coincidences. For this purpose, resolved I- 9 type doublets may provide ideal two level systems which are similar to ammonia inversion doublets. The general theory for the present study is described briefly in the next section. The experimental details, analysis of the spectra, results of the study, and a discussion of the results follow in subsequent sections. 10 II-2 Theory Investigations of the vibration-rotation spectra of polyatdmic molecules in the gas phase have been of importance for determining precise molecular geometry and energy structure. With the advent of laser spectroscopy, both the resolution and feasibility of various types of experiments have been greatly improved. As a result, the importance of studies of the rovibrational states of polyatomic molecules has increased. The quantum mechanical description of the electronic and nuclear motions should yield the vibrational, rotational, and electronic energy levels as well as the corresponding wave functions for the systu. Since the electronic motion is so fast in comparison with the nuclear motion, at each point the electronic energy may be considered to have reached its equilibrium value corresponding to the nuclear geometry. Therefbre, we are normally justified to employ the Born-Oppenheimer approximation which treats the nuclear and the electronic motion separately. As a further approximation, the rigid rotor-harmonic oscillator may be employed to divide the Hamiltonian of nuclear motion into the vibrational and rotational parts, as follows: Hn = Ht + Hr + Hv , (2-1) where Ht is the Hamiltonian fer molecular translation, Hr the rotational Hamiltonian, and Hv the vibrational Hamiltonian. With these ll approximations, the energy of a molecule may be expressed simply by a sum of electronic, vibrational, rotational, and translational contributions; E = E + E + E + E e v r t r (2_2) r’ and Et are the electronic, vibrational, rotational, and translational energies. Since this thesis is concerned with the where Ee’ Ev, E vibration-rotation transitions in one electronic state, the electronic and translational parts will not be discussed further. The rigid rotor approximation is of course not sufficient to analyze experimental data on vibrational-rotational transitions. Higher-order corrections for the vibrational-rotational interactions, the centrifugal effect of molecular rotation, and the anharmonicity of molecular vibrations must be introduced to utilize fully the wealth of information involved in the data of high resolution experiments. The theoretical details will be discussed in this section especially for symmetric top molecules. II-2-l Hamiltonian for Harmonic Oscillator-Rigid Rotor Approximation To a good approximation, the electronic and vibrational-rotational motions are normally separated in molecular spectroscopy. However, it is necessary to introduce further approximations because the SchrOdinger equation is still too complicated to be solved exactly. Although these approximations are much cruder than the Born-Oppenheimer approximation, they are very important, since the known eigenfunctions will be used to 12 form the basis vectors for higher variation or perturbation calculations. As the first approximation, it is assumed that the vibrational displacements of the atomic nuclei in rigid molecules are limited in a small region around the equilibrium configuration. Hence the molecule keeps the equilibrium moment of inertia by neglecting the vibrational dependence: 2 (J 4092/ 2123+ 2 91/2 + v (2—3) H = _ vr m-x,y,z m k where PR is vibrational momentum, J“ and as are rotational and vibrational angular momenta, and.I;u is a moment of inertia along a molecular principal axis. As a further approximation, both the vibrational angular momentum and the anharmonicity are neglected. The obtained Hamiltonian operator for this case is 2 2 2 o 1 Jx J1 J2 l 3N-6 2 2 Hvr = 2 [ _3_ + o + _3— + 2' g [ Pk + ka ] ' (2-4) I I I k-l xx yy 22 II-2—1-l Harmonic Oscillator The harmonic oscillator leads to a wave equation for the nonlinear molecule that can be written in the form 13 —- 2 2k=l 1 3N‘6 [62 OZWV -Eoo _ 802 Mk V] - Ev wv (2 5) where 0k is the normal coordinate of the k-th mode of frequency 1/2 "k"‘k wave function depending on the normal coordinates. /2n, E3 is the vibrational energy, and 03 is the vibrational It is convenient to introduce dimensionless normal coordinates qk and corresponding operators of linear momenta pk which are defined by the equations _:k 1/2Q pk(=—i§ —q—k)= *1. ”4 fi‘l/Z P1. (2—7) where =4n2v 2 and P =-iha/ao . So that Eq. (2-5) becomes ’1: k k k --1-:g_6( 2)( 2+ 2w°< )-s° w°< ) (2—8) 2 ”‘1.“ pquvqk'vvqk° It is well known that the solutions of Eq. (2-5) are the vibrational energy levels Ev for which E(k)= hD k(v k+l/2) v : 0,1,2,.... (2'9) The eigenfunctions of the linear harmonic oscillator equations (Eqs. (2-2)~(2-5)) are 14 2 W - N; e k k HV (Yk GR) (2 10) ”k k k where rkf4nzvk/h and Hv,(yt{2 0k) is the hermite polynomial k of order of v expressed as a function of r1/2 0 ; N is a k k k vk normalization constant N = vk (2-11) (5‘) v [ Yk 1/2 1 1/2 2 k(vk!) For a doubly degenerate normal vibration, the SchrOdinger equation can be written in the form, %[(paz+pb2>+ = z . (2—27) JV. ’ k7. ’ m" Only the diagonal matrix elements of the operator, J5, are nonzero, = h2k2 . (2-28) On the other hand, Jx and Jy have diagonal as well as off-diagonal matrix elements. From the relations, (h/2)[(J:k)(J:h+1)11/2 <2-29) t(ih/2)[(J:k)(J:k+1)]1/2 , (2—30) the diagonal elements of J: and J: are = = (52/2)[J(J+1)-k2] (2—31) and the off-diagonal elements are 19 = - = (ha/4)[J(J+l)—k(ktl)]1/2[J(J+1)-(kil)(kt2)]1/2 . (2-32) Hence there are the following nonzero matrix elements of H: in the J, k, m representation: 2 2 = fl—[{-l— + -l—}[J(J+1)-k2] + 25—] , (2-33) r 4 Io IO 0 xx yy 22 : gi[_l_ _ _l_][J(J+1)-k(k:1)]1/2[J(J+1)—(k:1)(k:2)11/2. (2-34) 1° 1° XX YY II-2-l-2-3 Rotational Energy Levels of Symmetric Top Molecules . o _ o For a symmetric top molecule, Ixx - Iyy lies along the axis of symmetry. As a result, H: has only diagonal if the principal axis 2 nonvanishing matrix elements in the J, k, m representation; that is, the angular momentum quantum number k becomes a good quantum number: = fi— {iiiill + —l- - -1— k2} . (2—35) r 2 Io Io Io w 22 w The molecular rotation constants A, B, C can be introduced by the following relations: A = fiz/(4ncIa), a = fiz/(4ncl c = fiz/(4nc1c) , (2-36) b). 20 where c is the speed of light. In terms of the rotational constants, the rotational energy levels of the prolate symmetric top are given by the expression, Eg/hc = BJ(J+1) + (A—B)k2 ; (2—37) for an oblate top molecule, Eg/hc = BJ(J+1) + (c-B)k2 . (2-38) Hereafter, we will express all energies in multiples of hc, so that Er/hc = Er' II-2-l-2-4 Symmetric Top Rotational Wavefunctions In terms of the Euler angles a, O. x, the Schrodinger equation for a rigid prolate symmetric top can be written in the following form o 2 o 2 o 1 §_ [sine ——5] + l a wr [:osze A] 6 mr sine as a sm2e 802 in2e B ax2 2 o o 2cose 6 gr + Er 0° 0 sinze a¢ax B r (2-39) Variables in Eq. (2-39) can be separated and the wave function, W , can 21 be written as a product O:(e,¢.x) = 8(6) aim” eikx . (2-40) Since w: must be single valued if'o and.x are changed to ¢+2nn and.x+2nn (n=0,l,2,...), k and m in Eq. (2-39) can assume only integral values 0,11,:2,... Because variables O and x occur only in the derivatives in Eq. (2- 39), they appear in Eq. (2-40) in simple exponential terms. Function 8(a) is more complicated because it is the solution of the following equation: sine as . 2 in a sin e 2 2 1 a . 88 e I m cos a A 2 O - 399§9km - —§5 ] 8(a) = o . (2-41) sin e Physically acceptable solutions of Eq. (2-41) exist only if 8? satisfies the following conditions: 0 _ 2 Er - BJ(J+l) + (A-B)k , (2-42) where J is a positive integer with J 2 lkl or lml, i.e., J = 0,1,2,..., (2-43) k = 0,11,12,..., J, (2-44) m = 0,:1,32,..., J. (2-45) 22 Rayefunctions Bka(e) corresponding to eigenvalues E:(J,k) for k=m=0 are the Legendre polynomials P§(cose), whereas for m s 0 they are the associated Legendre polynomials (15). The function 8300(9) can be written as [<2J+1)/<8n2>11/2] dJ J (cosze-l)J . (2-46) 2 J! 8 (e) = [ J00 (dcose ) II-2-2 Selection Rules If the molecule is in a free space, the isotropy of the space makes it possible to consider any one of the three space-fixed principal axes. The electric dipole moment operator is given by N+Ne o = 2 ei(Zi-Zi) (2-47) p 2 i=1 where ei and 21 are the charge and space-fixed coordinate of the ith particle in the molecule; 2: is a coordinate of the molecular center of mass. We express pz in terms of the components ”x’ my, pz of 5 along the molecule-fixed axes: ”z = pxXZx + pyny + “2"22 (2‘48) where xZX, xzy, x22 are the direction cosines. 23 If the rovibronic wavefunctions are considered in the approximation as the product of electronic, vibrational, and rotational functions, we can write 000 nor") I n H i N) _ =rx2y ZOD'eWVIpal wee > - (O' [ODe In“ IOe >]Ov > - (WV In“ (e’ ,e )|@v> (2 50) where pa(e',e") depends still on the nuclear coordinates. we expand pa(e ,e") in terms of the normal coordinates of the electronic states about the point of the equilibrium configuration of the atomic nuclei of that state, ua(e' .e") = u:(e' .e") + i - O 0 n r n v n r r n r n __ — §[pa(e ,e )(Wv|0v> + 2(apa(e ,e )/an)°](Orlx2a|0r>. (2 52) The first term is responsible for pure rotational transitions where (O; = 0;, O; = O3). The intensities of such spectra are proportional to 0 r n 2 [pa] , the product of the square of a component of the permanent dipole moment and the square of the corresponding direction- cosine matrix element. Vibrational transitions within a given electronic state are controlled by the second term in the square brackets. From the harmonic oscillator approximation, <0;|Qkhws> # 0 only if Avk = :1. For the case of vibration-rotation transitions, we must consider the matrix elements of x2“ together to specify selection rules on the rotational quantum numbers J,k. It is convenient to write Eq. (2-49) in the form I l D N N N - 0 ' N N D I. - (Ovlpz(e ,e )IOvXOrlxlzltDr) + (1/2)<0;|xzx+ixzy|0;> + (l/2)<@£lx2x-ixzy|0;> . (2-53) It turns out that the only non-zero elements of>~zz are 0 n - v_ n ._.._ _ ,. 0 1f Ak k k 0 (2 54) and II l+ H v - n ' _ (Wr'xe'thylwr) ,. 0 1f Ak (2 55) 25 The general selection rules may be applied to symmetric top molecules by taking account of the fact that p: = p; = 0, p: x 0. For the pure rotation spectra of non-degenerate vibrational states of symmetric tops: Ak = 0, AJ = 0, :1. (2-56) Selection rules for the allowed vibration-rotation transitions can be obtained by combining the selection rules for vibrational and rotational transitions. There are two different types of allowed transitions in symmetric top molecules (16). When the electric dipole moment oscillates in a direction which is parallel to the z axis (parallel band), Griz/80190 # 0. (aux/0k)o = (my/3°90 = 0. (2-57) In this case, selection rules for the rotational quantum numbers are E 0, AJ 0, :1 for k s 0 , (2-58) g 0, AJ :1 for k = 0 . (2-59) When the electric dipole moment oscillates in a direction that is perpendicular to the z axis (perpendicular band), (apz/aok)o = o. (aux/30k)o . o, (any/aok)O . o. <2-60) Selection rules for the rotational quantum numbers are then 26 Ak = :1, AJ = 0, :1 . (2-61) In addition to the above selection rules for the rotational quantum numbers, there are also selection rules which are concerned with the symmetry properties of the rotational levels. Hougen derived general selection rules for electric dipole transitions by consideration of the fact that rovibronic energy levels can be classified according to certain symmetry species (11). The dipole moment operator is invariant to a permutation of the coordinates of identical particles since the operator pz is simply the sum of the charges ei of all the particles in the molecule multiplied by their 2 coordinates. It may be noticed that the transformation properties of ”Z are identical with those of the product Tsz, where T2 and R2 represent a translation and a rotation about the z axis (11). Selection rules may be formulated from the transformation properties of pz, which lead to the conclusion that the electric dipole transition between two rovibronic states, of species F' and r", is T x FR . Here FT and. FR 2 z z z allowed if and only if F'x F" contains F are the irreducible representations of T2 and R2 for the corresponding permutation-inversion group. Application of this rule to a C3v molecule leads to the consideration that the dipole moment operator is classified under A2 species from r x FR = A1 x A2: A2. Therefore, the allowed 2 T 2 transitions ought to be such that F'x F" contains A2. As a result, we may add two more selection rules: 27 AleaAZ and EvaE . (2-62) The principally allowed transitions are shown in Fig. 2-1 and Fig. 2-2. Hougen (11) introduced a convenient quantum number, G = Gev-k (for the ground electronic state, G = 1-k), which may replace the 1- designation originally proposed by Herzberg (16). This quantum number allows influence of the symmetry species of rovibronic energy levels to be specified without additional quantum numbers. The selection rule due to symmetry considerations may be described with the quantum number G as follows: An electric dipole transition between two states is allowed if and only if G'- G" 5 AG = 0 mod n, where n is the highest-fold axis of rotation in the molecule. As a result, the electric dipole transition selection rules, Ak = 0 for parallel transitions and Ak = :1 for perpendicular transitions, are proved by the fact that the connected states have the same symmetry as shown in Fig. 2-1. This rule may also be applied to the additional transitions allowed by Coriolis interactions, which need not obey the selection rules on k. Such transitions will normally be exceedingly weak compared to vibronically allowed transitions. It should be pointed out that the quantum number G by itself contains no more information than is contained in the symmetry species label of the rovibronic level. II-2-3 Nonrigid Symmetric Top Molecules II-2-3-1 Centrifugal Distortion Rotation about any axis in the molecule is accompanied by centrifugal forces which tend to alter the effective moments of inertia. Homemaker:- - . 1v i I V e .h I‘m ”-7 6 9 .un “owing... 28 on. Fl a I... r ‘1 Fl 3 7 E 6 E Ar: 5 z E E ‘— 2 a ‘ E3232 ~_’ E 3 E up? 2 E N— 6 E ‘ J J -’ 8—-—E J 7 E J 8 5 J E 7—____.—:.l E 6———E 7 6 7—5 5 7 IN 6 EC 5 E 6 {I S E 6 g E 3 “I O E b) 5——E 5 ‘___‘ 5 N ‘ E 4 E 3——*¢_.___~ 4 a 3 E 3 E 3 0. 53—5 2 E 5 a. K 3 0 K 3 1 K 3 2 K = 3 K = 4 K = 5 Figure 2-1. Symmetry properties of rotational levels of molecules with a three-fold axis; (a) in a totally symmetric vibrational state, (b) in a degenerate vibrational state. The arrows show allowed transitions. 29 KL. Hi}. Figure 2-2. The rovibronic levels with K = l and J = 1,2 for vibronic E-state of a molecule of symmetry C3v° The transitions indicated by solid arrows are allowed; those indicated by dashed arrows are not. 30 The resulting dynamic effect forces the atoms away from an axis of rotation and increases the moment of inertia about that axis. The centrifugal effects introduce into the energy level expression terms with high powers of J(J+l) and K2. For a prolate top molecule, E = BJ(J+1) + (ArB)K2 - DJJ2(J+1)2 - DKK4 - DJKJ(J+1)K2 +... , (2-63) where D D and DJK are the quartic centrifugal distortion constants. J! K! The correction terms for centrifugal distortion are found to depend only on even powers of the angular momentum because the distortion effects do not depend on the direction of rotation about any axis. II-2-3-2 Coriolis Interaction Coriolis resonance interactions in symmetric top molecules have been studied by Nielson and coworkers (lg-29) and later by diLauro and Mills (g1). According to Jahn’s rule (22), if the product of the symmetry species of two vibrational modes contains the species of rotation, P(Qk) x P(Qk.) = P(Ru), Coriolis interaction takes place between the vibrational nodes (11). The Coriolis force is represented in classical mechanics as the cross product of the linear velocity of the particle relative to the molecule-fixed axis system and the angular velocity of the rotation; = 2m; x u . (2‘64) Fig. 2-3 illustrates the effect of the Coriolis interaction between 31 Figure 2-3. Coriolis forces during the degenerate vibration of an X3 molecule. Figure 2—4. Diagrammatic representation of the x,y-Coriolis coupling of the states with J = 3 and with the same k-lt. The dotted line connects states exhibiting giant l-type doubling. 32 components of the v2 degenerate vibrational mode of the tri-atomic molecule X3. For a counter-clockwise rotation of the molecule the Coriolis forces are as shown by the short arrows (Fig. 2-3). It is noticed from the figure that they tend to excite the other component of the degenerate vibration. The result of this Coriolis interaction is a splitting of the degenerate vibrational levels into two levels whose separation increases with increasing rotation (K) about the top axis and is zero for K = 0. Coriolis interaction may be explained in quantum mechanics as the interaction between the vibrational and rotational angular momenta about the appropriate molecular axis: _ 2 _ 2 _ _ _ Hcor - (2A/h )< szz) + (zn/h )< Pxe pny) , (2 65) where A,B are the rotational constants of a prolate top molecule and Jx’ J . 32 and px. p Y Y angular momentum about the corresponding molecular axis. Eq. (2-65) , pz denote the components of over-all and vibrational indicates that there are basically two kinds of effects: (i) interaction due to the rotation about the top axis 2 (in a symmetric top molecule, interaction of two degenerate modes v and vt.), and (ii) interaction t due to the rotation about the x, y axes (in a symmetric top molecule, interaction between nondegenerate mode vs and the degenerate mode vt). When vt=v£, the z-axis Coriolis coupling contributes to the energy in the first order by the term _ z 2 _ 2[ 232;t + ntJJ(J+l) + nth Jitk (2 66) 33 where the term -ZBZ{:1tk represents the primary effect of the Coriolis interaction and the other terms describe the rotational dependence of the Coriolis coupling. The subscript t denotes a degenerate vibrational state. The result of this strong Coriolis interaction is a splitting of the degenerate vibrational levels into two levels whose separation increases with increasing rotation about the top axis. Hence the formula for the rotational energy levels in a vibrational level of a symmetric top molecule in which a degenerate vibration v is singly t excited, may be represented by _ _ 2 - _ E(v)(J,K) - B(V)J(J+1) + (A(v) 8(v))K + 2A(v){iK1 + .... (2 67) which differs from Eq. (2-42) only by the term 2A(v){iK£. Coriolis interactions due to rotation about the x, y axes appear as off-diagonal components: (vs-l,vt,£t;J,k|H Iv ,(vt-l),ltil;J,kil> cor s _ y - 1/2 - 1/2 _ - _nst{stBy[vs(vt+1t)] [(J+k)(th+l)] (2 68) where _ 1/2 _ nst- [(vs+vt)/2(vsvt) ] . (2 69) For simplicity, let us consider states with v8 = vt = 1. Since Ak = Alt = 11, the matrix elements given in Eq. (2-68) connect only the state |0,l+1;J,k+l) with the state |1,0;J,k> which is further connected to the state |0,l-1;J,k-l> (Fig. 2-4). Thus for each value of J the energy 34 matrix factorizes in separate blocks, each block being characterized by a particular value of (k-Rt). It is noticed that k is not a good quantum number any more whereas (k-lt) still remains as a good quantum number (ii). We can obtain the eigenvalues by building and diagonalizing the following 3x3 matrix for given J and Rent; |0,1 ;J,k+1> |l,0;J,k> |0,1 ,J,k-1> "'0 +F(J k+1)—ZB {2(k+1) 21/23 9 {V [J k] 0 l t ’ z t x st st ’ _ l/2 y _ ms+F(J,k) 2 B£n8t{st[3,k 1] L (Hermitian) mt+F(J,k-l)+282{:(k-l) J (2-70) where _ _ 2 _ F(J,k) - BXJ(J+1) + (82 Bx)k , (2 71) [J,k] = [J(J+1)-k(k+l)]1/2 . (2-72) Because for each rotational state Ikl g J, there are only two identical 2x2 blocks for the special case (k-lt) tJ, and only two identical lxl blocks (unperturbed states) for (k-lt) :(J+l). In addition, Garing gt a; (£3) showed that for k-lt = 0 the matrix given by Eq. (2—70) can be factorized by the transformation |A+> = 2'1/2[|o,1+1;J,1> t |0,1‘1;J,-1>] . (2—73) The transformed matrix has the form, 35 |A+> |1,0°;J,o> |A_> ' _ Z mt+F(J,1) zazat o o 1 y mS+F(J,0) ZBzflst{8t[J(J+1)] . . Z L (Hermitian) mt+F(J,l) 282!t j (2-74) Thus the pair of degenerate levels with k = it = :1 of the ”t state splits into two components A+ and A_. The A_ sublevel interacts with the k = 0 level of us but the A+ sublevel is unperturbed, that is, only one of the two energy levels (A1, A2) is affected by the Coriolis interaction. Nielson called this splitting "giant l-type doubling" (g3). Since l-type doublings provide a very good information source for Coriolis interactions, they have been probed to study existing Coriolis interactions (§,Z). Note that for odd J the species of A+ is A1 and that of A_ is A2, while for even J the species of A+ is A2 and A_ is Al. The effects of l-type doubling will be discussed in more detail in the following section. II-2-3-3 Rotational R-type Resonance Interaction Wilson showed by symmetry considerations that rotation-vibration interaction might split degenerate rovibrational energy levels of symmetric top molecules into a number of components (g5). For example, in a symmetric top molecule with C3v symmetry, if ken # 3n, then the 36 rotational and the vibrational wavefunctions belong to the degenerate species B and the total rovibrational wavefunctions should form bases for the irreducible representations of ExE = A1+A2+E. The splitting into an E level and AlAZ pair results from first order Coriolis coupling (see section II-2-3-2). The splitting of the AlAz pair into separate levels, however, is of higher order and explained by a more detailed treatment of vibration- rotation interaction (gg). There are off-diagonal matrix elements in the quantum numbers l and k which split and shift the zeroth—order energy levels. The most familiar example of the splitting of the A levels is R-type doubling. The associated effects, which are called rotational l-type doubling or l-type resonance, were first discussed by Nielson (g§,gz) and later described in detail by Grenier-Besson (gg). Selection rules for the matrix elements can be obtained from Amat’s rule (2_9) -Ak + E “t Alt = pN (2-75) where the value of N is determined by the N—fold principal symmetry axis of the point group; p is an arbitrary integer which is positive, negative or zero; and nt=l for 81 (or E) species, nt=2 for 82 species etc. This relation gives off-diagonal matrix elements of three types which, in the notation of Cartwright and Mills (39), are given as follows: 37 (Vt,1t+l;J,k+lIH/hclvt,£t-1,J,k-l> (p/4)qt*[2-n,211/2{[J(J+1>-k 2]1/2{[J(J+1)-k(k+1)][J(J+1)—k(k¢l)]}1/2 (2—77)

= prt[(vt+1)2-(£t¥1)2]1/2[J(J+l)-k(k+l)]1/2(2ktl) . (2—78) The Hamiltonian fl is obtained by the appropriate contact transformation and the constant p in Eqs. (2-76) - (2-78) is equal to either +1 or -1, depending on the sign of the constants qt and r Cartwright and Mills t’ (39) refer to the effects associated with the matrix elements as qt+ (or :2,i2)-type , qt_ (or tZ,¥2)-type, and rt (or t2,$l)-type interactions. According to Eq. (2-75), qt+ interactions occur for all El(or E, E Elu’ E'l, etc) type vibrational species in all symmetric top lg’ molecules; the qt- interactions occur for all Em species in symmetric top molecules with an even principal axis of symmetry (Cn or 8D with n even) when m=(n-2)/2 (E in DZd’ E in D4h’ etc.); the rt type 3,11 interaction occurs for El species in molecules with an odd principal axis of symmetry Cn if m = (n-l)/2 (E in 03v, E2 in CSv’ etc). Since this thesis is concerned with C3v molecules, qt— interactions will not be discussed further. we will follow the sign convention that Cartwright and Mills t = k = :1 levels leads to the rovibrational A1 level lying above the rovibrational A2 introduced; qt > 0 when the 1~type doubling in the 1 38 level for J even. In the (vt,llt )= (1, +1) vibrational state the doubling is thus given by the formula T(A1)-T(A2) qt+J(J+1) for J even (2-79) qt+J(J+l) for J odd (2-80) where T(A1), etc., denote the term values. The general formula for qt+ in terms of the vibration-rotation interaction parameters also has a definite sign if we follow these conventions (2§,§Q). Thus, 31)2 2 + : 2—2{— 01: +128 {y2 + flj—v—s. { X2 g3 v2 v2 st g v2 2 st vs t s ”t 2 _ xz o l/ _ sat /4122 + 2w(C/h) 220, t t. at.v / 3/2} (2 81) ”t where _ -l 3 2 _ is a cubic anharmonic constant, qr is a dimensionless normal coordinate, _ 1/2 yy _ qr - 2n(vr/h) or’ and at — The effects of k-resonances are illustrated in Fig. 2-5. The (aIyy/aot)o. reason that l-type doubling is large compared to other Al-Az splittings can be explained by the fact that the l-resonances take place between the two degenerate levels (k = 1t = :1). Finally, since subscripts s and t have been used here to denote the nondegenerate and degenerate vibrational states only for clarification, they will be dropped or switched with notation of the corresponding vibrational modes for convenience in the following sections. 39 +l -l H -l H 1 2 .. 3 ° 3 3 I. 1 1 J a 1:??- a 1 8 3 a a 3 3 3 4 S 5 (+) (-) Figure 2—5. qt , qt , and rt R-resonance in an 1t = :1 degenerate state of an oblate symmetric top. The levels are labeled by K, with (+2) to the left of (-£); interactions are shown by broken lines. 40 II-3 Experimental II-3-l White-Type Long Path Cell White-type cells have been applied to a number of applications in spectroscopy to provide long absorbing paths (31,32). This type of cell is useful for many cases: (1) inherently weak transitions, for example, combination and overtone bands; (2) low concentration samples such as transient molecules and reaction intermediates; (3) high resolution spectroscopy that needs to keep the pressure low for small pressure broadening. In 1942, White introduced the design which accomplished the desired result (33). The essential parts of the equipment are three spherical, concave mirrors that all have the same radius of curvature. The setup is shown in Fig. 2-6, where two mirrors A and A' are placed close together at one end and the third mirror B at the other end. The centers of curvature of A and A' are located on the front surface of B, and the center of curvature of B is half way between A and A'. Later Bernstein and Herzberg introduced a useful variation in the shape of the front mirror (B), which, in the case where the size of the source is appreciable, doubles the number of traverses obtainable without overlapping images (35). Fig. 2-7 shows the shape of a front mirror of this type together with the image location on it. In a multiple-reflection system, astigmatism can limit the maximum attainable number of passes even more than reflectivity. This aberration causes an increase of the size of each successive image and eventually image overlapping. In the double row alignment (Fig. 2-7), the tangential image elongation is the main result of the astigmatism. The general fOrmula for the image increase has been derived by Edward 41 —— —-—— —~_. ——__- Figure 2-6. Mirror arrangement of a White-type cell. The small circles on mirror surface are the centers of curvature of the mirrors. Figure 2—7. Modified optical arrangement for a White—type cell. The numbers show the sequence of reflection. 42 z hb 4 ( N — ‘) (2‘83) 12122 N 4 _ AL N N) — __§__( T 12Rfv where b is the total separation between the entrance and exit images, N the number of traverses, h the height of mirror, R the radius of curvature, and fv the vertical f number (h/R). From Eq. (2-83), it is clear that b should be as small as possible. For a source of width ws the minimum value of b which will give distinct images on the front mirror and, will allow the entrance and exit images to clear the mirror edges, is bmin=N/4ws and the corresponding width of the upper portion of the front mirror is (N/4-l)ws (3Q). One may wish to cut down the wide front mirror to reduce ALT. Reflectivities of mirrors also limit the number of traverses. For example, forty traverses with 98* reflectivity reduces energy to about 45% of that incident. The homemade White type cell used in this work includes three spherical mirrors with 1 m radius of curvature, two one inch diameter mirrors and a two inch diameter front mirror. Three micrometers provide required fine adjustment for appropriate alignment of each mirror. The cell body consists of a 6 inch glass cylinder, 1 inch Can windows located horizontally at the level of the center of the front mirror, and aluminium end plates, which are tightened with O-rings for seals. The whole structure is supported by the customized aluminium frame, and the actual volume of the cell is estimated to be about 11 liters. The windows provide enough room to adjust the incoming and outgoing laser for double row alignment (Fig. 2-7). Without particular difficulty, a 43 24 m path-length can be obtained with a 2 mm diameter He/Ne laser beam entering parallel. Throughout the study of the pa + v6 - 06 band of CH3F, the mirrors were arranged to give 8 m path-length, which is enough to provide the necessary signal to noise ratio when the cell is filled with CH3F to 0.5 Torr pressure. II-3-2 Infrared-Microwave Sideband Laser Spectrometer Fig. 2-8 is a block diagram of the infrared microwave sideband laser spectrometer used to record the spectra for this work. It is very similar to the spectrometer used for previous studies from this laboratory (2,2) except for the use of the White-type long path sample cell. Since the instruments used in the spectrometer have been described in detail elsewhere (2,2), only a brief explanation of the components will be given. The semisealed CO2 laser includes a 1.7 m plasma discharge tube with ZnSe Brewster angle windows in a 2.2 m laser cavity with a rotatable plane grating at one end and a partially transmitting (95X reflection) spherical concave mirror on a piezoelectric translator (PZT) at the other end. Microwave radiation was generated by a synthesizer (HP 8671B) and amplified by a traveling wave tube amplifier (Varian Model VZM-6991Bl) at specific frequencies in the 8-18 GHz region. Approximately 1 W of CO2 laser power (frequency v!) is mixed with ~20 W of microwaves (frequency vm) in a CdTe electrooptic crystal that is mounted in an impedance-matched housing. A detailed description of the CdTe electrooptic crystal and the electrooptic effect can be found in Shin-Chu Hsu’s thesis (2§). Since the generated sidebands (frequency ”1 1 um) are polarized in a vertical 44 CE]a LASER He/Ne Los Muthposs Ceu Coll Focusmg Lens Bean Polariza- Sputter- DET PREAMP PIN CONTROL PSD 33.3kH2 Mod. COMPUTER Figure 2-8. Block diagram of the infrared microwave sideband laser used in this study. 45 plane, they are efficiently separated from the horizontally—polarized carrier by means of a polarizer and later divided by a beam splitter into two portions. One of the beams is used as a reference while the other is allowed to pass through the White—type sample cell. Both beams are monitored by liquid N2 cooled HngTe detectors (Infrared Associates, Inc. HOT-100) cooled by liquid N The sidebands are 100% amplitude 2. modulated by chopping the microwave power with a PIN diode, and the detector signals (signal and reference) are processed by lock-in amplifiers at the modulation frequency (33 kHz). The signal from the reference lock-in amplifier is sent to a feedback circuit to stabilize the total sideband power by controlling the microwave power. The CO2 laser carrier reflected from the polarizer passes back and forth through a cell that contains CO2 and the 4.3 pm fluorescence signal that results from the additional vibrational excitation is detected at 90° angle to the beam by a liquid N2 cooled InSb photovoltaic detector (Judson Infrared, Inc. JlOD). The saturation dip in the fluorescence from this cell is used to stabilize the laser frequency. For this purpose the laser frequency is modulated at 100 Hz by means of a sinusoidal voltage applied to the PZT. The residual jitter in the laser frequency is estimated to be ~150 kHz, which is also the expected accuracy of the frequencies of the sidebands. The sidebands were not separated, but the spectra were recorded a second time with the CO2 laser locked at the edge of the fluorescence saturation dip in a known direction. The shift in the apparent center frequency of each spectral line (5-10 MHz) was enough to identify whether the positive or negative sideband had been absorbed. Figs. 2-9 and 2-10 are examples of spectra of the hot band of 46 Intensity(orb. units) ‘53 R(9,5.—1)‘ ‘ R 8,—1,—1 R 8.1.1 ‘ 452 ( ) ( ) d .1 .1 45* ‘2C‘602 9P(12) ‘ “‘35 I T FT* 1 I 12.0 12.5 13.0 13.5 14.0 14.5 15.0 Frequency(GHz) Figure 2-9. Portion of the spectrum of the v3+v6-v6 band observed in the present work. The horizontal axis is the microwave frequency to be added to (+) or subtracted from (-) the frequency of the 9P(12) 1201602 laser to obtain the infrared frequency of the transition. 47 35 1* I I I I 25- 1 E 15‘ + V ‘ 'E — + — 3 '1 ., d 5_ V R(12,6,-1) d S 4R(12,5,_1) 4 + '6 R(12,2.1) C '1 .8 -15~ ~ g * 2V3 R(17,0—6) -25~ . . 12C1602 9P(6) , -35 I 1 l 1 l 8.0 8.5 9.0 9.5 10.0 10.5 11.0 Frequency(GHz) Figure 2-10. Portion of the spectrum of the 03+v6-06 band observed in the present work. The horizontal axis is the microwave frequency to be added to (+) or subtracted from (—) the frequency of the 9P(6) l201602 laser to obtain the infrared frequency of the transition. The transition marked 2v3 is in the 2123-123 band and completely absorbs the positive sideband power. 48 interest in this work plotted as a function of the microwave frequency, which must be added to or subtracted from the appropriate laser frequency to obtain the infrared frequency of the transition; the laser frequencies were obtained from the report of Freed g2 g1. (21). Fig. 2- 9 is an example of a relatively clear region of the spectrum that shows a well-resolved B-doublet. Fig. 2-10 shows a portion of the spectrum that includes a 2D3 * v3 hot-band transition that is sufficiently strong to absorb the entire positive sideband power. Spectra were recorded for microwave frequencies from 8 to 18 GHz in 4-MHz steps for more than 40 laser lines. The frequencies of the transitions were obtained by fitting the spectra by least squares to Gaussian lineshapes; for overlapped transitions, the Doppler halfwidths were constrained to the appropriate value (~34 MHz). A commercial sample of CH3F from Peninsular Chemical Research was used as received with only the usual freeze-pump—thaw cycling. The spectra were recorded at room temperature (~29? K). 49 II-4 Results II-4-l Term Values and Selection Rules As mentioned in the introduction, both the upper and the lower vibrational states of the 03 + 06 — ”6 band in CH3F belong to E-type symmetry for 03v point group. The spectra were analyzed by calculating the frequencies as differences in term values E(v,J,k,£) for degenerate vibrational states (22,29) as follows: E(v,J,k,£) = W(v,J,k,1) + wq(v,J,k,£) (2-84) where W(v,J,k,£) = v0 + av J(J+1) + (Av- 3v) k2 - 211.v {k1 - n} J2(J+l)2 - DEX J(J+1)k2 - n; k4 + n} J(J+l)k9. + 1.; R39. + H} J3(J+1)3 + 33K J2(J+l)2k2 + HEJ J(J+1)k4 + a; k4 (2—85) In Eq. (2-85), ”0 is the vibrational band center; Av and Bv are the . , v v v v v v v . rotational constants, DJ, DJK’ DK’ HJ, HJK’ HKJ’ and HK are the quartic and sextic centrifugal distortion constants; and f. n}. and n; are Coriolis coupling constants. In Eq. (2-84), wq(v,J,k,1) is the 1- resonance contribution which, except when k = I, was taken into account explicitly as a second order perturbation: wq(v,J,k,£) = [qu(J+1) + q;J2(J+l)2]2f(v,J,k,£) for k , 1 (2-86) 50 where (J:k)(J:k-1)(J:k+1)(J:k+2) 4[W(v,J,k,£=:l) - W(v,J,k$2,£=$1)] f(v,J,k,1=il) = (2—87) When k = B = :1, the l-resonance term becomes l-type doubling: wq(v,J,k,1) = % [qu(J+l) + q;J2(J+1)2] for k = i . (2-88) The l—resonance term described above is referred as the (12,32)- interaction (29). Another possible l-resonance in a 03v symmetric top, the ($2.11) interaction, can not be included in the least squares fitting of the frequencies because of linear dependence. The details will be described later. During the vibrational transition, 03 + v6 ~ ”6’ the dipole moment may be considered to change parallel to the principal axis of symmetry. Therefore the selection rules for allowed transitions were taken to be AJ = 0 or 11, Ak = 0, and.A1 = 0 (11). Since off-diagonal l-resonance elements mix the rotational levels (Ak = Al = 12 and Ak = :1, A1 = $2) of degenerate vibrational states, in principle, other transitions, (Ak = AI = $2,.A(k<1) = :3), are also allowed, but they are expected to be much weaker and no attempt has been made to assign them. The primary selection rules were used for all of the transitions except those for which k = 1, for which k and 1 are not good quantum numbers because of the linear combination of the states. For these transitions, it was necessary to use the fundamental selection rule A1 .. A2, where the identification of A1 and A2 levels is shown in Fig. 2-11 for odd J and qv > 0 for the ”6 state (q6 is known to be positive (2)) and for the two 51 qu>0 qu<0 qu>0 qu<0 Aa-w— A1 fir- A1 ‘7"- AZT— A1 ‘7‘ Aan— A2 "5"!— A1 "'1? i i i 1 i E i 1 A2 -LJ— A2 —-J— A2 ——L A2 ——-1— A1 4— A1 4—— A1 —— A1 —— Q-Bronch P,R-Bronc:h Figure 2-11. Energy-level diagrams showing higher frequency (solid lines) and lower frequency (dashed lines) allowed transitions between rotational levels belonging to two vibrational states of 8 symmetry for C3v‘ For each of the diagrams, the J value of the levels in the lower state is assumed to be odd and the qv value of the lower state is assumed to be positive; the sign of the qv value (qu) for the rotational levels of the upper state is indicated above each diagram. 52 possible signs of qv for the v3+v6 state. As indicated in Fig. 2-11, we followed the sign convention suggested by Cartwright and Mills (22). II-4—2 Analysis The most tedious part of the assignment of the spectra was the identification and labeling of the many transitions from the 03 fundamentals of 12CH3F and 13CH3F and the 203 - v3 hot band of 12CH3F, all of which were considerably stronger than the transitions desired for the present study. Fortunately, we had precise constants available (2,2) for the interfering bands and were able to calculate the frequencies of the overlapping transitions to high accuracy (within few MHz). A first attempt at assignment was made by combining the reported frequencies of the D6 and v3+v6 bands, as reported by Hirota (2) and Nakagawa (2) g: 22., respectively. This method led to the assignment of three J = 6+5 transitions about 500 MHz from their predicted values. The Q(6,4) transition, in which 0 denotes the transition J~J and the numbers are the J and K quantum numbers, was also found near the value reported by Duxbury and Kato (lg), although it was seriously overlapped with another transition which was assigned later as the Q(lO,lO). However, assignment of higher J and k transitions by this method was not possible because a limited number of experimental frequencies were reported. We then calculated energy levels of the two states by using the parameters reported by these workers and obtained frequencies from differences in the energies. This procedure was also not useful because the calculated frequencies were far from the experimental values. The 53 problem was traced to the fact that rather different ground state constants were used in Refs. 2 and 2. Successful assignment of the v3 + v6 - v6 band transitions was obtained when the constants in the paper by Hirota (2) were used to calculate frequencies of the 06 band and the constants in the paper by Nakagawa (2) were used to calculate frequencies in the 03-1-1)6 combination band. Then the desired frequencies of the v3+06-06 band were obtained as combination differences of the calculated frequencies. This procedure led to assignment of additional transitions for 1 = +1, but the 1 = -1 transitions could not be assigned with confidence until after several iterations of least-squares fittings of the l = +1 frequencies with proposed assignments of the 1 = -1 transitions gave better values of the constants. Strong correlations between A! and the centrifugal distortion constants DK and DJK could not be broken until the 1 = -1 transitions were included. The Coriolis terms in the energy expression give contributions to the energies that are large enough to cause the transitions for adjacent k values for a given J to be separated by about 3 GHz. The 1 = +1 and.k -1 transitions spread out in different directions from the k 0 transition for each J; the separation between 1 = +1 components for adjacent k is somewhat larger than for the corresponding 1 = -1 components. In case of oblate top molecules one can actually observe a series of doublets (1 = +1, -1) with k for a given J because the Coriolis interaction term, |C{l is smaller than the term, |(C-B)k2| (22). As shown in Fig. 2-11, both components of the l-type doublets occur for P, Q, and R transitions according to Al-A2 selection rule. It can be seen that the va+v6-06 band frequencies are sensitive to the absolute 54 magnitudes and the relative signs of qv for the upper and lower states, but cannot be used to determine the absolute signs of the qv’s. We took the sign of qv for the 126 state from Ref. 2. Fig. 2-9 shows the 1- doublet pair for the QR(8,l) transition, which was the first pair found. By using the splitting for this pair and constraining the qv constant for the 06 state to that determined by Hirota (2) it was possible to identify one or both components of 13 P- or R-branch l-type doublets for 3 S J S 20 and one Q-branch pair, QQ(4,1); the frequencies of these transitions are shown in Table 2-1. Additional Q—branch transitions were not identified because of the density of the Q—branch region and the low intensity of Q-branch transitions for k = 1. In the final 1 fitting, which included the microwave frequencies for the direct 1- doublet transitions in the 06 state (1), the qv constants for both states were adjusted (q6 was constrained to be positive) and it was necessary to include the higher-order constant q; for high J l-doubling transitions as shown in Eq. (2-88). In principle, the contribution of l-resonance to the energy includes rv-dependent terms that result from the following matrix elements (22,29): = 2rv(2k + l)[(J - k)(J + k + 1111/2 . (2-39) An attempt was made to include the effect of these terms for both states at the level of second-order perturbation, but unstable fittings with unpredictable correlations were obtained. In order to trace the origin of the problem, the data were fit, including rv for the v6 state only, by means of a least-squares routine that calculates the eigenvalues of 55 TABLE 2-1 Observed Transition Frequencies 12 from l-type Doublets of the 03+ vs— vs Band of 083F Trans.a Laserb v.c v/Mflz O—Cd Uhc. v/cm l f P(17, 1, 1) 1301602 9P(12) -13 805.5 30 199 220.6 2.5 5.0 1007.337 57( 8) P(l7,-l,-l) 1301602 9P(12) -10 667.9 30 202 358.2 2.1 5.0 1007.442 22( 7) P(l5,-1,-1) 1301602 9P( 8) 9 081.4 30 324 127.7 0.2 5.0 1011.504 01( 1) P( 7, l, 1) 1201602 9P(40) -15 094.5 30 785 048.2 -0.3 5.0 1026.878 67( -l) P( 7.-l.-l) 1201602 9P(40) -14 513.9 30 785 628.8 4.4 10.0 1026.898 04( 15) P( 5,-1,-1) 1301602 9R(18) -17 955.5 30 894 523.2 0.9 3.0 1030.530 36( 3) P( 3, l, 1) 1301602 98(22) 13 210.6 31 000 682.6 0.4 5.0 1034.071 45( l) P( 3,-1,-1) 1301602 98(22) 13 324.5 31 000 796.4 -3.4 5.0 1034.075 26( -11) O( 4, 1. 1) 1201602 9P(28) -11 040.4 31 148 467.8 -3.4 5.0 1039.001 05( -11) O( 4,-l,-1) 1201602 9P(28) -10 908.2 31 148 600.0 -0.2 5.0 1039.005 46( -1) R( 4, 1, 1) 1201602 9P(20) 15 308.6 31 399 209.0 -3.7 5.0 1047.364 87( -12) R( 5,-1,-1) 1201602 9P(18) 8 229.4 31 446 289.5 3.5 5.0 1048.935 31( 12) R( 8, l, 1) 1201602 9P(12) -13 892.7 31 581 939.0 2.8 3.0 1053.460 09( 9) R( 8,-l,-l) 1201602 9P(12) -13 072.6 '31 582 759.1 -0.1 3.0 1053.487 45( 0) R(ll. l, 1) 1201602 9P( 8) 14 634.8 31 711 696.3 1.1 5.0' 1057.788 33( 4) R(ll,-1,-l) 1201602 9P( 8) 16 115.8 31 713 177.2 1.1 5.0 1057.837 72( 4) R(lZ,-1,-1) 1201602 9P( 6) 8 815.6 31 755 299.4 0.3 3.0 1059.242 77( 1) 8(18, 1, 1) 1201602 9R( 4) -13 901.0 31 990 116.4 -l.9 5.0 1067.075 41( -6) R(18,-l,-1) 1201602 SR( 4) -10 192.3 31 993 825.1 -0.9 5.0 1067.199 12( -3) R(19,-1,-1) 1201602 98( 6) -17 028.8 32 031 207.5 0.6 3.0 1068.446 06( 2) 8(20, 1, 1) 1201602 98( 6) 15 166.7 32 063 403.0 2.0 5.0 1069.519 99( 7) 8Numbers are J, k, and l of the lower vibrational state. lower energy components of the l-type doublets. bLaser line used; laser frequencies were taken from Ref. 21. cMicrowave frequency in MHz. The signed microwave frequency was added to the laser frequency to obtain the absorption frequency. Levels with k,1 = -1,-1 are the dObserved minus calculated frequency in MHz; the parameters for the calculation are in Tables 2-3 and 2-4. eEstimated uncertainty in the observed frequency in MHz. fCbserved wavenumber in cm.1. wavenumbers in units of 0.00001 cm The 9 umbers in parentheses are observed minus calculated 56 the normal equations matrix after scaling. It is known that the occurrence of one or more small eigenvalues in this procedure is evidence of linear dependence (22); we found one small eigenvalue for which the corresponding eigenvector contained a substantial contribution from the parameter r6. The origin of this problem then became obvious when we expanded the second-order perturbation contribution from the matrix element in Eq. (2-89) and found that the contribution to the energy, wr, could be written as wr(v,J,k,1) = r'[-J(J+l) + 3k2 + ki - 2J(J+l)k1 + 2k31] (2—90) where 4r: r' = . (2—91) Av — Bv + ZAV; The detailed derivation of this equation is in the Appendix. Apparently, at this level of approximation, by redefining the parameters v v . . . B Av Bv, Av" nJ. and "K to include a contribution from rv, the v’ effects of the matrix elements in Eq. (2-89) are included completely. It is therefore not surprising that a linear dependence was encountered when rv was included as a parameter in the fitting. A linear dependence involving rv was already implicit in the equation given by Grenier- Besson and Amat for the rotational frequencies in an E state of a 03v molecule (29). Ultimately, the measured frequencies of’more than 220 transitions in the v3+v6-v6 band were assigned and used to obtain vibration-rotation parameters for the two states. The final least squares fitting included 57 the rotational frequencies reported in Refs. (2,1), in which each data point was weighted by the inverse of the squares of the uncertainty. In order to avoid linear dependence, vo, (Av-Ev), DK’ Av{, andnK of the v6=1 state were constrained to the values reported by Hirota (2), and HK for this state was constrained to zero. The standard deviation for an object of unit weight and the root-mean-square deviation are calculated 1.05 and 8.05 MHz, respectively. The frequencies of assigned transitions are compared in Table 2-2 to calculated frequencies that were obtained from the determined vibration-rotation parameters in Tables 2-3 and 2-4. 58 TABLE 2-2 Comparison of Observed and Calculated Frequencies in the v3+ v6- ”6 Band of 12CH3F Trans.a Laserb v-c v/MHz O—Cd U’nc.e v/cm l f P(17, l,-l) 1301602 9P(12) —17 765.8 30 195 260.3 -2.1 3.0 1007.205 46( -7) P(l7, 0, 1) 1301602 9P(12) -15 063.0 30 197 963.2 0.1 5.0 1007.295 62( P(17, l. 1) 1301602 9P(12) -13 805.5 30 199 220.6 2.5 5.0 1007.337 57( P(17,-1,-1) 1301602 9P(12) -10 667.9 30 202 358.2 2.1 5.0 1007.442 22( P(17. 2. 1) 1301602 9P(12) -9 277.2 30 203 748.9 5.3 5.0 1007.488 61( 18) P(16, 5,-1) 1301602 9P(10) -17 314.9 30 247 154.2 4.7 3.0 1008.936 46( 16) P(16. 4,-1) 1301602 9P(10) -15 158.6 30 249 310.5 4.7 5.0 1009.008 38( 16) P(16, 3.-1) 1301602 9P(10) -12 865.7 30 251 603.3 -2.2 3.0 1009.084 87( -7) P(16, 2.-l) 1301602 9P(10) -10 431.8 30 254 037.3 -6.4 5.0 1009.166 06( -21) P(16, 5, 1) 1301602 9P(10) 10 431.8 30 274 900.8 -0.1 5.0 1009.861 98( P(16, 7, 1) 1301602 9P(10) 17 708.2 30 282 177.3 -ll.7 5.0 1010 104 70( —39) P(15, 9,-1) 1301602 9P( 8) -14 201.7 30 300 844.6 0.1 5.0 1010.727 38( P(15, 8,-1) 1301602 9P( 8) -12 708.1 30 302 338.2 4.7 5.0 1010.777 19( 16) P(15, 7.-1) 13C1602 9P( 8) -11 039.2 30 304 007.1 1.5 5.0 1010.832 86( P(15, 6,-1) 1301602 9P( 8) -9 186.5 30 305 859.8 11.0 30.0 1010.894 67( 37) P(15,-1,-1) 1301602 9P( 8) 9 081.4 30 324 127.7 0.2 5.0 1011.504 01( P(15, 2. 1) 1301602 9P( 8) 10 826.9 30 325 873.2 1.1 3.0 1011.562 23( P(15. 3. 1) 1301602 9P( 8) 13 952.5 30 328 998.8 0.6 5.0 1011.666 50( P(15, 4, 1) 1301602 9P( 8) 17 220.8 30 332 267.1 -0.8 5.0 1011.775 52( -3) 9. 5.-1) 1201602 9P(44) -16 006.7 30 658 439.0 -3.8 5.0 1022 655 44( -l3) 9. 2.-1) 1201602 9P(44) -9 045.1 30 665 400.7 1.5 5.0 1022.887 65( 9, 4, 1) 1201602 9P(44) 8 739.0 30 683 184.8 -22.1 30.0 1023.480 87( -74) 9, 5, 1) 1201602 9P(44) 12 253.1 30 686 698.8 0.7 3.0 1023.598 08( 9, 6, 1) 1201602 9P(44) 15 917.4 30 690 363.2 7.7 5.0 1023.720 32( 26) 8, 3.-l) 1301602 9R( 8) 9 306.3 30 719 078.4 -2.7 3.0 1024.678 15( -9) 8, 1,-1) 1201602 9P(42) -13 484.1 30 724 172.6 3.2 20.0 1024.848 07( 11) 8, 3, 1) 1301602 98(10) -16 001.5 30 736 057.4 1.4 3.0 1025.244 51( 8, 4, 1) 1301602 9R(10) -12 664.1 30 739 394.8 -0.8 3.0 1025 355 83( -3) 8, 5, 1) 1301602 9R(10) —9 161.6 30 742 897.3 4.0 5.0 1025 472 67( 13) 8, 6, 1) 1201602 9P(42) 8 917.0 30 746 573.7 16.4 20.0 1025 595 29( 55) 8, 7, l) 12C1602 9P(42) 12 765.2 30 750 421 9 24.0 10.0 1025 723 66( 80) 7, 6,-1) 1301602 99(10) 16 001.5 30 768 060 4 18.4 20.0 1026.312 02( 61) 7. 2.-1) 1301602 98(12) -16 422.5 30 777 049.4 0.6 3.0 1026.611 85( 7, 0, 1) 1201602 9P(40) -17 696.7 30 782 446.0 13.5 20.0 1026.791 87( 45) 7, 1, 1) 1201602 9P(40) -15 094.5 30 785 048.2 -0.3 5.0 1026.878 67( -l) 7.-1.-1) 1201602 9P(40) -14 513.9 30 785 628.8 4.4 10.0 1026 898 04( 15) 7, 2, 1) 1201602 9P(40) -11 743.0 30 788 399 7 16.3 20.0 1026 990 46( 54) 7, 3, 1) 1201602 9P(40) -8 555.1 30 791 587 6 10.8 20.0 1027.096 80( 36) 6, 3, 1) 1201602 9P(38) -15 467.0 30 846 430.5 -3.3 5.0 1028.926 16( -11) 6, 3, 1) 1301602 98(14) 12 421.6 30 846 433.6 -O.2 3.0 1028 926 26( -l) 6. 4, 1) 1201602 9P(38) -12 116.2 30 849 781.3 -0 7 5.0 1029.037 93( -2) 6, 4, 1) 1301602 9R(14) 15 771.0 30 849 782 9 0 9 3.0 1029.037 99( 6, 5, 1) 1201602 9P(38) -8 608.0 30 853 289.5 1 7 5.0 1029.154 96( 5, 3,-1) 1301602 9R(16) 9 876.0 30 883 556.4 -8.6 10.0 1030.164 55( -29) 5, 2,-1) 1301602 9R(16) 12 375.5 30 886 055.9 1.9 3.0 1030.247 92( 5, l,-l) 1301602 9R(16) 15 003.6 30 888 684.0 -1.4 3.0 1030.335 58( -5) 5, O, 1) 1301602 99(16) 1? 778.0 30 891 458.4 0.8 3.0 1030.428 13( 5.-1,-l) 1301602 9R(18) -17 955.5 30 894 523.2 0.9 3.0 1030.530 36( 5, 3, 1) 1301602 9R(18) -11 855.8 30 900 622.9 -2.2 5.0 1030.733 82( -7) 5, 4, 1) 1301602 99(18) -8 504.4 30 903 974.3 -l.3 5.0 1030.845 62( -4) 59 TABLE 2-2 (cont’d) Tranl.a Laserb v-C v/Mflz 0—0d Uhc. D/CI-l f P( 4, 3,-l) 1201602 9P(36) 14 150.8 30 937 066.3 1.1 5.0 1031.949 45( 4) P( 4, 2,-1) 1201602 9P(36) 16 647.5 30 939 562.9 2.7 5.0 1032.032 72( 9) P( 4, 1,-1) 1301602 98(20) -8 207.4 30 942 201.1 4.3 5.0 1032.120 73( 15) P( 3, 2,-1) 1201602 9P(34) 9 209.7 30 992 400.5 0.8 3.0 1033.795 20( 3) P( 3, 1,-1) 1201602 9P(34) 11 852.5 30 995 043.3 1.9 3.0 1033.883 36( 6) P( 3, 0, 1) 1201602 9P(34) 14 631.5 30 997 822.3 0.4 3.0 1033.976 05( 1) P( 3, 1, 1) 1301602 98(22) 13 210.6 31 000 682.6 0.4 5.0 1034.071 45( l) P( 3,-1,-1) 1301602 98(22) 13 324.5 31 000 796.4 -3.4 5.0 1034.075 26( -11) P( 3, 2, 1) 1301602 98(22) 16 328.5 31 003 800.4 0.0 5.0 1034.175 45( 0) 0(17, 8,-1) 1201602 9P(32) -12 184.2 31 030 533.9 20.0 OMIT 1035.067 19( 67) 0(17, 7,-1) 1201602 9P(32) -10 201.3 31 032 516.8 10.2 20.0 1035.133 34( 34) 0(16, 9,-1) 1301602 98(24) 16 510.3 31 040 181.7 23.2 OMIT 1035.389 01( 77) 0(16, 7,-1) 1301602 98(26) -15 065.0 31 043 944.3 -4.2 5.0 1035.514 51( -14) 0(19, 7, 1) 1301602 98(26) -12 374.6 31 046 634.6 0.7 5.0 1035.604 26( 2) 0(15,12,-1) 1301602 98(26) -12 374.6 31 046 634.6 2.2 5.0 1035.604 26( 7) P( 2, 1,-1) 1301602 98(26) -11 791.9 31 047 217.4 -0.2 5.0 1035 623 70( -1) 0(15,11,-1) 13C1602 98(26) -11 109.9 31 047 899.4 2.4 5.0 1035.646 44( 8) 0(16, 5,-1) 1301602 98(26) -10 734.8 31 048 274.4 5.2 5.0 1035.658 95( 17) P( 2, 0, 1) 1301602 98(26) -9 011.5 31 049 997.7 -4.1 5.0 1035 716 43( -14) 0(15, 5,-1) 1201602 9P(32) 16 284.0 31 059 002.0 -6.5 10.0 1036 016 78( ~22) 0(l4, 5,-1) 1301602 98(26) 10 063.5 31 069 072.8 -9.4 20.0 1036.352 72( -31) Q(13,10,-1) 1301602 98(26) 10 063.5 31 069 072.8 13.1 20.0 1036.352 72( 44) 0(13. 8,-1) 1301602 98(26) 13 368.5 31 072 377.7 5.5 5.0 1036.462 96( 18) 0(13, 7,-1) 1301602 98(26) 15 261.1 31 074 270.3 0.7 5.0 1036 526 09( 2) 0(16, 5, 1) 1301602 98(28) -17 173.7 31 076 314.8 -7.7 5.0 1036 594 28( -26) 0(13, 6,-1) 13C1602 98(28) -17 173.7 31 076 314.8 2.9 3.0 1036.594 28( 10) 0(12,11,-l) 1301602 98(26) 17 532.7 31 076 541.9 -3.6 5.0 1036.601 85( -12) 0(15, 4, 1) 1201602 9P(30) -17 664.3 31 083 827.9 8.2 10.0 1036.844 89( 27) 0(11,11,-1) 1201602 9P(30) -16 759.0 31 084 733.1 -6.3 5.0 1036.875 09( -21) 0(12, 6,-1) 1201602 9P(30) -16 426.0 31 085 066.1 1.8 5.0 1036 886 19( 6) 0(11, 9,-1) 1201602 9P(30) -13 926.2 31 087 566.0 -16.9 20.0 1036.969 57( -56) 0(12, 4,-1) 1201602 9P(30) -11 968.7 31 089 523.5 -0.2 5.0 1037.034 87( -1) 0(15, 6, 1) 1201602 9P(30) -10 939.4 31 090 552.8 -8.5 5.0 1037.069 21( -28) 0(16. 9, 1) 1201602 9P(30) -10 751.5 31 090 740.7 -37.2 40.0 1037.075 47("124) 0(11, 7,-1) 1201602 9P(30) -10 361.5 31 091 130.7 -6.2 5.0 1037.088 49( -21) 0(12, 3,-1) 1201602 9P(30) -9 545.7 31 091 946.5 3.7 5.0 1037.115 70( 12) 0(11, 6,-1) 1201602 9P(30) -8 349.0 31 093 143.2 -4.3 5.0 1037.155 61( -14) 0( 9, 9,-1) 1301602 98(28) 8 337.1 31 101 825.6 -9.8 20.0 1037.445 23( ~33) 0(14, 7, 1) 1301602 9R(28) 10 828.9 31 104 317.3 -6.9 3.0 1037.528 35( -23) 0(10, 4,-1) 13C1602 98(28) 11 489.4 31 104 977.9 -2.0 20.0 1037.550 37( -7) 0(15,10, 1) 1301602 98(28) 12 313.9 31 105 802.4 28.0 OMIT 1037.577 88( 94) 0(13, 5, 1) 13C1602 98(28) 13 235.3 31 106 723.8 -2.7 5.0 1037.608 61( -9) 0( 9, 6,-1) 1301602 98(28) 13 805.0 31 107 293.5 -8.6 10.0 1037.627 61( -29) Q( 9, 5,-1) 1301602 98(28) 15 941.1 31 109 429.6 -4.0 5.0 1037.698 86( ~13) O( 8, 8,-1) 1301602 98(28) 16 092.9 31 109 581.3 -6.0 5.0 1037.703 92( -20) 0(13, 6, 1) 1201602 9P(30) 8 719.7 31 110 211.9 -0.9 5.0 1037.724 96( -3) O( 8, 7,-1) 1201602 9P(30) 9 903.1 31 111 395.3 -4.2 3.0 1037.764 43( -14) 0( 9, 4,-1) 1201602 9P(30) 10 208.8 31 111 700.9 -3.4 5.0 1037.774 64( -11) 0(14. 9. 1) 1201602 9P(30) 10 510.2 31 112 002.4 10.3 5.0 1037.784 68( 35) 0(12. 4. 1) 1201602 9P(30) 10 654.3 31 112 146.5 -0.6 5.0 1037.789 50( -2) 60 TABLE 2-2 (cont’d) Trans.a Laserb v-C v/Mflz 0-0d Unc.e D/CI-1 f 0( 8, 6,-1) 1201602 9P(30) 11 877.5 31 113 369.7 -2.2 5.0 1037.830 30( -7) 0( 8, 5,-1) 1201602 9P(30) 14 012.5 31 115 504.7 10.3 10.0 1037.901 51( 34) 0( 7, 7,-1) 1201602 9P(30) 15 307.5 31 116 799.7 -7.4 5.0 1037.944 70( -25) 0(13, 8, 1) 1201602 9P(30) 16 131.3 31 117 623.5 -4.3 5.0 1037.972 18( —14) 0( 8, 4,-1) 1201602 9P(30) 16 265.2 31 117 757.4 -1.2 5.0 1037.976 66( -4) 0( 7, 6.-l) 1201602 9P(30) 17 275.3 31 118 767.4 -1.8 3.0 1038.010 35( -6) O( 5, 2,-1) 1301602 98(30) 9 699.6 31 136 811.7 4.3 10.0 1038.612 23( 14) 0( 8, 3, 1) 1301602 98(30) 10 111.6 31 137 223.8 0.8 5.0 1038.625 99( 3) 0( 4, 3.-1) 1301602 98(30) 10 542.3 31 137 654.5 6.6 5.0 1038.640 34( 22) Q( 9, 5. 1) 1301602 98(30) 10 748.0 31 137 860.2 1.7 20.0 1038.647 22( 6) 0(10, 7, 1) 1301602 98(30) 11 239.1 31 138 351.3 9.0 5.0 1038.663 60( 30) 0( 5, 1,-1) 1301602 98(30) 12 340.8 31 139 452.9 -11.0 5.0 1038.700 34( -37) 0( 7, 2, 1) 1301602 98(30) 12 340.8 31 139 452.9 0.9 5.0 1038.700 34( 3) 0( 4, 2,-1) 1301602 98(30) 13 057.7 31 140 169.9 -1.4 20.0 1038.724 25( ~5) Q( 3, 3,-1) 1301602 98(30) 13 248.8 31 140 360.9 20.6 20.0 1038.730 63( 08) 0( 8, 4, 1) 1301602 9R(30) 13 403.4 31 140 515.6 -3.5 5.0 1038.735 78( -12) 0( 9, 6, 1) 1301602 98(30) 14 322.3 31 141 434.5 6.5 5.0 1038.766 44( 22) 0( 7. 3. 1) 1201602 9P(28) -16 891.7 31 142 616.5 -5.7 10.0 1038.805 86( -19) O( 3. 2.-1) 1201602 9P(28) -16 644.0 31 142 864.2 1.3 10.0 1038.814 12( 4) 0( 2. 2.-1) 1201602 9P(28) -14 625.1 31 144 883.1 1.3 5.0 1038.881 48( 4) 0( 9, 7, 1) 1201602 9P(28) -14 338.9 31 145 169.3 15.5 5.0 1038.891 02( 52) 0( 7, 4, 1) 1201602 9P(28) -13 579.8 31 145 928.4 -0.3 3.0 1038.916 33( -1) 0( 6, 3, 1) 1201602 9P(28) -12 163.1 31 147 345.0 -2.9 3.0 1038.963 60( -10) O( 2, 1,-1) 1201602 9P(28) -11 970.7 31 147 537.4 -1.3 20.0 1038.970 01( -4) Q( 8, 6, 1) 1201602 9P(28) -11 970.7 31 147 537.4 -4.4 20.0 1038.970 01( -15) Q( 5, 2, 1) 1201602 9P(28) -11 293.4 31 148 214.8 ~1.4 3.0 1038.992 61( -5) 0( 4, 1, 1) 1201602 9P(28) -11 040.4 31 148 467.8 -3.4 5.0 1039.001 05( -11) 0( 4,-1,-1) 1201602 9P(28) -10 908.2 31 148 600.0 -0.2 5.0 1039.005 46( -1) 0( 1, 1.-1) 1201602 9P(28) -10 615.6 31 148 892.5 7.6 30.0 1039.015 21( 26) O( 9, 8, 1) 1201602 9P(28) -10 426.2 31 149 082.0 34.7 30.0 1039.021 52( 116) O( 7. 5. 1) 1201602 9P(28) -10 130.8 31 149 377.4 -0.6 5.0 1039.031 39( -2) O( 6, 4, 1) 1301602 98(32) -9 213.6 31 150 670.0 6.6 10.0 1039.074 50( 22) Q( 8, 7, 1) 1201602 9P(28) -8 207.8 31 151 300.4 14.0 10.0 1039.095 53( 47) 0( 5, 3. 1) 1201602 9P(28) -8 113.1 31 151 395.0 -4.6 5.0 1039.098 69( -15) 0( 4, 2, 1) 1301602 98(32) -8 293.9 31 151 589.8 1.6 5.0 1039.105 18( 5) R( 0, 0, 1) 1201602 9P(26) -14 243.5 31 202 517.8 4.6 5.0 1040.803 95( 15) R( 3, 3,-l) 1201602 9P(22) 11 965.4 31 340 926.9 3.8 5.0 1045 420 78( 13) R( 3. 2.‘1) 1201602 9P(22) 14 516.3 31 343 477.8 3.8 5.0 1045 505 87( 13) R( 4, 1, 1) 1201602 9P(20) 15 308.6 31 399 209.0 -3.7 5.0 1047 364 87( -12) R( 5,-1,-1) 1201602 9P(18) 8 229.4 31 446 289.5 3.5 5.0 1048 935 31( 12) R( 5. 2. 1) 1201602 9P(18) 11 088.4 31 449 148.6 -1.6 3.0 1049 030 68( -5) R( 5, 3, 1) 1201602 9P(18) 14 249.7 31 452 309.8 -3.9 3.0 1049 136 13( -13) R( 5. 4. 1) 1201602 9P(18) 17 538.8 31 455 599.0 -5.3 3.0 1049 245 84( -18) R( 6, 6,-1) 1201602 9P(16) -17 196.3 31 474 241.1 20.4 20.0 1049.867 68( 68) R( 6. 5.-1) 1201602 9P(16) -15 009.9 31 476 427.5 4.5 5.0 1049.940 61( 15) R( 6, 4,-1) 1201602 9P(16) -12 678.5 31 478 758.9 3.2 3.0 1050.018 37( 11) R( 6. 3.-l) 1201602 9P(16) -10 227.3 31 481 210.1 -2.0 5.0 1050.100 14( -7) R( 6, 4, 1) 1201602 9P(16) 10 227.3 31 501 664.7 -6.1 5.0 1050.782 42( -20) R( 6. 5. 1) 1201602 9P(16) 13 640.0 31 505 077.4 -0.4 5.0 1050.896 25( -1) R( 6. 6. 1) 1201602 9P(16) 17 196.3 31 508 633.7 11.4 20.0 1051.014 88( 38) 61 TABLE 2-2 (cont’d) Trans . a Laserb v“: v/Mflz O-Cd Unc . p/cn-l f B( 7, 3,~1) 1201602 99(14) ~17 414.9 31 526 614.0 0.2 3.0 1051.614 64( 1) R( 7, 2,~1) 1201602 9P(14) ~14 825.3 31 529 203.6 5.5 5.0 1051.701 02( 19) E( 7, 1,~1) 1201602 9P(14) ~12 132.0 31 531 896.8 2.7 3.0 1051.790 86( 9) R( 7, 0, 1) 1201602 9P(14) ~9 329.4 31 534 699.5 ~1.2 3.0 1051.884 35( ~4) R( 7. 6. 1) 1201602 9P(14) 9 938.3 31 553 967.1 4.3 3.0 1052.527 04( 14) R( 8, O, 1) 1201602 9P(12) ~16 395.6 31 579 436.2 1.6 3.0 1053.376 61( 5) R( 8. 1. 1) 1201602 9P(12) ~13 892.7 31 581 939.0 2.8 3.0 1053.460 09( 9) R( 8.~1.~l) 1201602 9P(12) ~13 072.6 31 582 759.1 ~0.1 3.0 1053.487 45( 0) R( 3. 2. 1) 1201602 99(12) ~10 469.0 31 585 362.8 ~5.8 5.0 1053.574 29( ~19) R( 9, 8,-1) 1201602 9P(12) 8 209.2 31 604 041.0 ~34.4 OMIT 1054.197 32(-115) E( 9, 7,-1) 1201602 9P(12) 10 247.7 31 606 079.4 ~2.7 3.0 1054.265 32( ~9) R( 8, 8, 1) 1201602 9P(12) 10 247.7 31 606 079.4 42.5 OMIT 1054.265 32( 142) R( 9, 6.~1) 1201602 9P(12) 12 393.7 31 608 225.5 1.7 3.0 1054.336 90( 6) R( 9, 5,-1) 1201602 9P(12) 14 661.7 31 610 493.4 2.9 3.0 1054.412 55( 10) R( 9, 4,-1) 1201602 9P(12) 17 040.0 31 612 871.8 ~3.1 3.0 1054.491 89( ~10) R( 9, 2. 1) 1201602 9P(10) ~17 439.9 31 629 403.5 ~3.6 3.0 1055.043 33( ~12) R( 9, 3, 1) 1201602 9P(10) ~14 321.4 31 632 522.0 ~4.6 3.0 1055.147 35( ~15) R( 9, 4, 1) 1201602 9P(10) ~11 091.2 31 635 752.2 ~4.7 3.0 1055.255 11( ~16) 8(10, 4,-1) 1201602 9P(10) 9 373.4 31 656 216.8 2.5 3.0 1055.937 73( 8) 8(10, 3,-1) 1201602 9P(10) 11 883.3 31 658 726.7 3.1 3.0 1056.021 44( 10) 8(10, 2,~1) 1201602 9P(10) 14 494.1 31 661 337.5 2.5 5.0 1056.108 53( 8) R(10, 1,~1) 1201602 9P(10) 17 204.6 31 664 047.9 2.7 3.0 1056.198 94( 9) 8(10, 6, 1) 1201602 9P( 8) ~11 214.8 31 685 846.6 ~0.5 3.0 1056.926 07( ~2) 8(11, 1,~1) 1201602 9P( 8) 9 677.3 31 706 738.7 10.1 20.0 1057.622 95( 34) 8(11, 0, 1) 1201602 9P( 8) 12 478.7 31 709 540.1 3.6 3.0 1057.716 40( 12) 8(11, 1, 1) 1201602 9P( 8) 14 634.8 31 711 696.3 1.1 5.0 1057.788 33( 4) R(11,~1,~1) 1201602 9P( 8) 16 115.8 31 713 177.2 1.1 5.0 1057.837 72( 4) 8(12, 8,-1) 1201602 9P( 6) ~14 767.6 31 731 716.2 1.1 3.0 1058.456 12( 4) 8(11, 7, 1) 1201602 9P( 6) ~14 516.1 31 731 967.7 2.3 3.0 1058.464 51( 8) 8(11, 8, 1) 1201602 9P( 6) ~10 832.4 31 735 651.4 13.2 10.0 1058.587 37( 44) 8(12. 6.~1) 1201602 9P( 6) ~10 437.5 31 736 046.2 ~10.8 10.0 1058.600 55( ~36) 8(12, 5,-1) 1201602 9P( 6) ~8 080.2 31 738 403.6 6.6 5.0 1058.679 19( 22) R(12,-1,~l) 1201602 9P( 6) 8 815.6 31 755 299.4 0.3 3.0 1059.242 77( 1) 8(12, 2, 1) 1201602 9P( 6) 10 927.2 31 757 410.9 0.2 5.0 1059.313 20( 1) 8(12, 3, 1) 1201602 9P( 6) 14 002.6 31 760 486.4 ~0.4 3.0 1059.415 79( -l) 8(12, 4, 1) 1201602 9P( 6) 17 174.2 31 763 657.9 ~0.7 5.0 1059.521 58( ~2) 8(13, 6,~1) 1201602 9P( 4) ~17 814.1 31 777 294.6 0.1 20.0 1059.976 45( 0) 8(12, 8, 1) 1201602 9P( 4) ~17 653.5 31 777 455.2 7.6 5.0 1059.981 80( 26) 8(13, 5,-1) 1201602 9P( 4) ~15 448.3 31 779 660.4 ~0.4 3.0 1060.055 37( ~1) 8(13, 4,-1) 1201602 9P( 4) ~12 991.0 31 782 117.7 ~6.0 20.0 1060.137 33( ~20) 8(13, 3,~1) 1201602 9P( 4) ~10 431.7 31 784 677.0 ~0.4 3.0 1060.222 70( ~1) 8(13, 4, 1) 1201602 9P( 4) 9 804.0 31 804 912.6 -3.0 5.0 1060.897 69( ~10) 8(13, 5, 1) 1201602 99( 4) 13 054.0 31 808 162.7 0.6 10.0 1061.006 10( 2) R(14,10,~1) 1201602 9P( 4) 14 245.1 31 809 353.8 8.5 5.0 1061.045 83( 28) 8(14, 9,-1) 1201602 9P( 4) 16 182.4 31 811 291.1 2.9 5.0 1061.110 44( 10) 8(13, 6, 1) 1201602 9P( 4) 16 398.6 31 811 507.3 ~4.9 3.0 1061.117 65( ~16) 8(16, 9, 1) 1201602 98( 2) ~17 740.2 31 941 255.8 ~15.4 5.0 1065.445 60( ~51) 8(17, 3,~1) 1201602 9R( 2) ~15 986.7 31 943 009.4 ~9.l 5.0 1065.504 10( ~30) R(16,10, 1) 1201602 98( 2) ~14 069.6 31 944 926.5 ~25.7 30.0 1065.568 05( ~86) 8(17, 1,-1) 1201602 98( 2) ~10 559.4 31 948 436 7 ~5.7 3.0 1065.685 14( ~19) 62 TABLE 2~2 (cont’d) Trans.a Laserb -c v/MHz 0-0d Unc. v/cm 1 f 8(18, 8,-1) 1201602 98( 2) 9 385.3 31 968 381.4 18.9 30.0 1066.350 41( 63) 8(17, 6, 1) 1201602 98( 2) 10 380.0 31 969 376.0 5.3 3.0 1066.383 59( 18) 8(18, 7,-1) 1201602 98( 2) 11 749.6 31 970 745.7 22.5 30.0 1066.429 29( 75) 8(18, 6,~1) 1201602 QR( 2) 14 169.2 31 973 165.3 2.0 5.0 1066.509 99( 7) 8(18, 5,-1) 1201602 98( 2) 16 674.9 31 975 671.0 ~3.8 5.0 1066.593 57( ~13) 8(17, 8, 1) 1201602 98( 2) 17 041.8 31 976 037.9 ~4.8 5.0 1066.605 81( ~16) 8(18, l,~1) 1201602 98( 4) ~17 696.5 31 986 320.9 ~5.9 5.0 1066.948 82( ~20) 8(18, 0, 1) 1201602 98( 4) ~14 902.2 31 989 115.2 ~12.6 20.0 1067.042 03( ~42) R(18, 1, 1) 1201602 98( 4) ~13 901.0 31 990 116.4 ~1.9 5.0 1067.075 41( ~6) H(18,~1,~l) 1201602 QR( 4) ~10 192.3 31 993 825.1 ~O.9 5.0 1067.199 12( ~3) 8(18, 2, 1) 1201602 98( 4) ~9 141.0 31 994 876.4 6.1 3.0 1067.234 20( 20) 8(19, 5,-1) 1201602 98( 4) 8 795.5 32 012 812.9 ~1.6 3.0 1067.832 49( ~5) 8(18, 8, 1) 1201602 9R( 4) 9 640.6 32 013 658.0 ~11.3 10.0 1067.860 68( ~38) 8(19, 3,~1) 1201602 9R( 4) 14 041.3 32 018 058.7 ~11.1 10.0 1068.007 47( ~37) 8(19, 2,~1) 1201602 98( 4) 16 741.5 32 020 758.9 ~14.5 20.0 1068.097 54( ~49) R(19,~1,~l) 1201602 98( 6) ~17 028.8 32 031 207.5 0.6 3.0 1068.446 06( 2) 8(19, 2, 1) 1201602 QR( 6) ~16 187.3 32 032 048.9 10.8 3.0 1068.474 14( 36) 8(19, 3, 1) 1201602 98( 6) ~13 240.9 32 034 995.4 15.3 5.0 1068.572 41( 51) 8(20, 2,~1) 1201602 98( 6) 9 030.6 32 057 266.8 ~12.8 10.0 1069.315 31( ~43) 8(20, l,~1) 1201602 QR( 6) 11 788.4 32 060 024.6 ~10.4 3.0 1069.407 31( ~35) 8(20, 0, 1) 1201602 98( 6) 14 588.8 32 062 825.1 ~7.2 10.0 1069.500 72( ~24) 8(20, 1, 1) 1201602 98( 6) 15 166.7 32 063 403.0 2.0 5.0 1069.519 99( 7) 8(20, 4, 1) 1201602 9R( 8) ~17 229.4 32 074 423.3 24.6 10.0 1069.887 60( 82) 8(20, 5, 1) 1201602 98( 8) ~14 222.9 32 077 429.8 17.9 10.0 1069.987 87( 60) The aNumbers are J, k, and 1 of the lower vibrational state. -l,~1 level is the lower energy component of an l-type doublet. k,1 = bLaser line used; laser frequencies were taken from Ref. 31. cMicrowave frequency in MHz. The signed microwave frequency was added to the laser frequency to obtain the absorption frequency. dObserved minus calculated frequency in MHz; the parameters for the calculation are in Tables 2~3 and 2~4. eEstimated uncertainty in the observed frequency in MHz. An "OMIT" means that the frequency was omitted from the least squares fits. f0bserved wavenumber in cm-l. The numbers in parentheses are observed minus calculated wavenumbers in units of 0.00001 cm 63 TABLE 2-3 Molecular Constants of the v6 = 1 State of 1201135‘8 Parameterb This Workc Hirotad av /GHz 35 455.736 0e 35 455.736 0(240) av /MHz 25 418.931 7(144) 25 416.92(48)f (Av-8v) /MHz 130 491.1e 130 491.1(42) DJ /kHz 61.613 5(4190) 59.669g nJK /kHz 457.251(4225) 440.27g nK /kHz 2 108.e 2 108.8 HJ /Hz 1.961(1061) HJK /Hz 7.231(8791) HKJ /Hz ~160.30(3447) HK /Hz o.h A( /MHz 46 279.8 46 279.(33) nJ /kHz 1 146.40(454) 1 120.(60)f “2 /kHz -9 600.e -9 600.(6600) qv /an 8.720 5(396) 8.70(13)f q'v /kHz -2.147 7(258) 8Values in parentheses are one standard deviation in multiples of the last digit in the parameter. bVibration-rotation parameters. cObtained from a fit of the vibration-rotation frequencies listed in Table 2-2. dRef. g, Table 2—3. eConstrained to the value reported in Ref. 8. tRef. 1, Table I. gAssumed to be the same as in the ground state (Ref. g). hConstrained to zero. 64 TABLE 2-4 Molecular Constants of the v3=1,v6=1 Vibrational State of 83F 12C 3 Parameterb This WorkC Nakagawa gt _1.d Ev /GHz 66 608.085 00(109) 66 605.04(36) Bv /MHz 25 082.214 8(305) 25 080.(39) (Av-8v) /MHz 130 557.989 9(961) 127 452.(60) DJ /kHz 58.076 9(4107) 55.2(45) DJK /kHz 519.867(3725) 528.(6) DK /kHz 2 039.099(2173) 2 370.(30) HJ /Hz 1.166(855) HJK /Hz 8.966(6712) 11KJ /Hz ~186.89(3241) AHK /Hz 13.26(1270) A! /MHz 44 850.096(97) 41 800.(150) nJ /kHz 942.86(433) 1 020.(60) “K /kHz ~9 479.44(41) 3 900.(300) qv /an -2.204 7(50) -90.e q’ /kHz ~0.959 8(207) 8Values in parentheses are one standard deviation in multiples of the last digit in the parameter. bVibration-rotation parameters. cObtained from a fit of the vibration—rotation frequencies listed in Table 2~2. dRef. g, Table 1. eRef. 9, constrained. 65 II~5 Discussion The frequencies of the transitions in Table 2~2 were fit without consideration of Coriolis interaction with other vibrational states. It is known that the levels of the v6 = 1 state are in mild Coriolis resonance with the levels of v3 = 1 (1,21) and presumably a similar resonance occurs between (v3,v6)=(l,l), (2,0), and (0,2). As was discussed in the studies of the v3 band from this laboratory (1,2), the mild v3~v6 Coriolis resonance in CH3F can be taken into account for reasonable J and k by adjustment of the rotational and centrifugal distortion constants for the states involved. As can be seen in Table 2~2, the transitions in the present work are limited to J S 20 and K i 10, and for K = 10 the residuals are beginning to show Coriolis effects that cannot be simulated by adjustment of the parameters. Since the necessary frequency information was not available for the v6 = 2 vibrational state, we did not examine the Coriolis interaction with nearby vibrational states in detail. The comparisons in Table 2~2 show that the frequencies of the transitions in the v3+v6~v6 band can be computed from the parameters in Tables 2~3 and 2~4 to within a few MHz for lower J and K and to within :10 MHz for J S 20, K S 10. In Tables 2~3 and 2~4 the parameters obtained in the present study are csmpared to previously-determined values. Except for the 1-doubling constant, the newly-determined constants agree with the older values to within the experimental accuracy of the latter. However, the new constants are much more precise, as the older data led to predictions of the frequencies that differed by as much as 1 GHz (0.03 cm-l) from the experimental values. Coriolis parameters for 03+v6 have been also 66 determined from the frequencies of the assigned 1=~1 transitions of v3+v6~06 band. Finally, the parameters in Tables 2~3 and 2~4 have been used to predict coincidences within 100 MHz of laser lines for the various isotopes of 002. The predicted coincidences are in Table 2~5, which may be helpful for various studies such as infrared-infrared double resonance. There are intriguing aspects of this work that suggest interesting topics for future study. First, there are unanswered questions about the effects of Coriolis coupling, or possibly Fermi resonance, in the 1234-1)6 state. Two pieces of evidence suggest that such effects should not be ignored: (1) the qv constants in the v6 and v3+v6 states differ not only in magnitude, but in sign, whereas they are expected to be of similar value (Eq. (2~81)); and (2) the ratio of the intensities of the transitions in the 203-v3 band to those in the v3+v6~96 band, although not measured, seemed to be greater than the value of ~2 that is inferred from the Boltzmann factor. A second interesting subject for future research would be an attempt to observe transitions in the 03+06-v6 band that obey selection rules other than the AR = 0, A1 = 0 rules observed in this work. In principle, transitions with Ak = :2, AI = :2 and with Ak = :1, A9. = :2 are allowed via the (1.2.:2) and (12,71) type 9.- resonances, respectively. However, their intensities may be as much as two orders of magnitude or more below the intensities observed in this study as inferred from the fact that frequency corrections due to 2- resonances are usually less than 20 MHz except for 1~type doublets. Nevertheless, the molecular constants reported here are sufficiently accurate to predict these frequencies to within a few MHz for low J and k, so that it may be possible to observe them if a region can be found 67 TABLE 2~5 Coincidences between Calculated Frequencies for the v3+v6~v6 Band of 1 201131? and Laser Frequencies Trans.a Frequencyb vo~v Laserd P(12, 8,-1) 30 480 581.7 54.7 1201602 BAND II P(50) P(10, 3,~1) 30 606 125.4 14.9 120160180 BAND II P(58) P(10, 7, 1) 30 637 314.3 ~19.4 120160180 BAND II P(57) P( 8, 1, l) 30 730 197.3 74.3 120160180 BAND II P(54) 0(18, 3,~1) 31 029 621.8 ~78.6 120160180 BAND II P(44) 0(20, 6, 1) 31 029 700.6 0.3 120160180 BAND II P(44) 0(17, 3,~l) 31 041 668.1 ~35.l 1301802 BAND II R(12) 0(18, 4, 1) 31 049 480.4 0.5 1201802 BAND II P(58) 0(15, 5,~1) 31 059 008.1 ~1.l 1301602 BAND II R(26) 0(13, 1, 1) 31 093 513.9 25.4 1301602 BAND II R(28) Q(lO,lO,-l) 31 093 552.5 64.0 1301602 BAND II R(28) P( l, 0, 1) 31 101 511.4 19.2 1201602 BAND II P(30) 0(13, 5, l) 31 106 726.8 ~25.7 1201802 BAND II P(56) Q( 9, 2,~l) 31 116 638.7 42.8 120160180 BAND II P(4l) 0(11, 6, l) 31 127 170.8 58.6 1301602 BAND II R(30) Q( 9, 7, 1) 31 145 153.8 ~96.6 120160180 BAND II P(40) Q( 5, 1, l) 31 145 263.9 13.5 120160180 BAND II P(40) Q( 6, 4, l) 31 150 663.4 1.7 1301802 BAND II R(18) R( 8, 6, l) 31 598 614.4 58.3 1201802 BAND II P(38) R( 9, 5,~1) 31 610 490.6 ~43.4 1301802 BAND II R(48) R(10, 2,~1) 31 661 334.8 ~96.8 1301802 BAND II 8(52) R(10, 9, l) 31 696 998.2 ~63.3 1201602 BAND II P( 8) R(15, 3, 1) 31 882 260.9 ~45.9 120160180 BAND II P(12) R(18, 5, 1) 32 003 944.4 ~73.0 1201602 BAND II R( 4) a . . . 12 , Transition in the v3+v6~v6 band of CH3F, J i 20, k S 10. cFrequency of the v d frequency in MHz. 3+v6~v6 band transition minus the laser bFrequency of the 03+v6~v6 band transition in MHz. Identification of the CO laser; Band II is the 9 pm band. Laser frequencies were 0 tained from Ref. 31. 68 in which the transitions are not strongly overlapped. 69 II~6 Appendix The contribution to the energy of the state |v,J,k,1=+1> from the (12,11) interaction given in Eq. (2~89) can be represented by a second order perturbation, 4r3(2k+1)2[J(J+1)-k(k+1)1 W(v,J,k,1=+1)~W(v,J,k+1,£=-1) ° Wr(v,J,k,£=+1) = (2~92) The energy difference between the corresponding rotational levels may be calculated approximately by W(v,J,k,1=+1) ~ W(v,J,k+l,£=-l) = vo+BJ(J+1)+(A~B)k2~2A{k ~[vo+BJ(J+1)+(A-B)(k+l)2+2A{(k+l)] = ~(2k+l)(A—B+2A{) . (2~93) By substituting Eq. (2~93) into Eq. (2~92), 4r2 wr(2k+1)[J—k is calculated in similar fashion, it will be seen that the result is the same except that the signs of the terms including odd powers of k are reversed. Therefore, since 1 = :1 only for v = l, we can write for the energy of either state, 2 w (v,J,k,£=tl) = r'[-J(J+l)+3k +k1-2J(J+1)k1+2k31] . (2—96) 71 II-7 References 1. CO 10. 11. 12. 13. 14. 15. 16. 17. 18. 19. P. Shoja-Chagervand and R. H. Schwendeman, J. Mol. Spectrosc. 98, 27—40 (1983). . S. K. Lee, R. H. Schwendeman, and G. Magerl, J. Mol. Spectrosc. 117, 416-434 (1986). . S. K. Lee, R. H. Schwendeman, R. L. Crownover, D. D. Skatrud, and F. C. DeLucia, J. Mol. Spectrosc. 123, 145-160 (1987). . Y. Matsuo and R. H. Schwendeman, J. Chem. Phys. 91, 3966-3975 (1989). . W. L. Smith and I. M. Mills, J. Mol. Spectrosc. 11, 11~38 (1963). . T. Tanaka and E. Hirota, J. Mol. Spectrosc. 54, 437-446 (1975). . E. Hirota, T. Tanaka, and S. Saito, J. Mol. Spectrosc. 68, 478-484 (1976). . E. Hirota, J. M01. Spectrosc. 74, 209—216 (1979). . J. Nakagawa, I. Suzuki, T. Shimanouchi, and T. Fujiyama, Bull. Chem. Soc. Japan 47, 1134-1138 (1974). G. Duxbury and H. Kato, Chem. Phys. 66, 161-167 (1982). S. Yamamoto, R. Kuwabara, M. Takami, and K. Kuchitsu, J. Mol. Spectrosc. 115, 333-352 (1986). G. Graner, R. Anttila, and J. Kauppinen, Mol. Phys. 38, 103~128 (1979). Z. Yao, B. R. Foy, J. R. Hetzler, and J. I. Steinfeld, Spectrochim.Acta. 42A, 1337-1339 (1986). W. H. Shaffer, Rev. Mod. Phys. 16, 245—259 (1944). A. J. Merer, J. K. 0. Watson, J. Mol. Spectrosc. 47, 499-514 (1973). G. Herzberg, "Molecular Spectra and Molecular Structure. II. Infrared and Raman Spectra of Polyatomic Molecules". D. Van Nostrand, Princeton, New Jersey 1959. J. T. Hougen, J. Chem. Phys. 37, 1433-1441 (1962). H. H. Nielsen, Rev. Mod. Phys. 23, 90-136 (1951). H. H. Nielsen, in Handb. Physik, Vol. 37, Part I, Springer, Berlin 1959. 20. 21. 22. 23. 24. 25. 26. 27. 28. 29. 30. 31. 32. 33. 34. 35. 36. 37. 38. 39. 72 G. Amat, H. H. Nielsen, and G. Tarrago, "Rotation-Vibration of Polyatomic Molecules". M. Dekker, New York 1971. C. DiLauro and I.M. Mills, J. Mol. Spectrosc. 21, 386-413 (1966). H. A. Jahn, Phys. Rev. 56, 680-683 (1939). J. S. Caring, H. H. Nielsen, and K. N. Rao, J. Mol. Spectrosc. 3, 496-527 (1959). E. B. Wilson, Jr., J Chem. Phys. 3, 818-821 (1935). T. Oka, J. Chem. Phys. 47, 5410-5426 (1967). H. H. Nielsen, Phys. Rev. 75, 1961 (1949). H. H. Nielsen, Phys. Rev. 77, 130-135 (1950). M. L. Grenier-Besson, J. Phys. Radium 21, 555-565 (1960). G. Amat, Compt. Rend. 250, 1439 (1960). G. J. Cartwright and I. M. Mills, J. Mol. Spectrosc. 34, 415-439 (1970). A. Biernacki, D. 0. Moule, and J. L. Neale, Appl. Spectrosc. 26, 648-650 (1972). D. Horn and G. 0. Pimental, Appl. Opt. 10, 1892-1898 (1971). J. U. White, J. Opt. Soc. Am. 32, 285-288 (1942). H. J. Bernstein and G. Herzberg, J. Chem. Phys. 16, 30-39 (1948). T. H. Edwards, J. Opt. Soc. Am. 51, 98-102 (1961). S. 0. Hsu, Ph. D. Thesis, Michigan State University, 1988. C. Freed, L. 0. Bradley, and R. G. O’Donnell, IEEE J. Quantum Electron. QE~16, 1195- 1206 (1980). R. M. Lees, J. Mol. Spectrosc. 33, 124-136 (1970). M. L. Grenier-Besson and G. Amat, J. Mol. Spectrosc. 8, 22-29 (1962). CRBPTER III HIGH RESOLUTION INFRARED STUDY OF THE v BANDS 0F 2 CD31 AND CD38r III—l Introduction The fundamental halides, CD I and 0D Br, have been the subject of a 3 3 number of spectroscopic studies in the microwave and infrared regions. Especially the 02 bands are of importance because they occur in the CO2 laser region and have therefore provided considerable spectroscopic information by means of linear and nonlinear spectroscopic techniques. The 02 band is identified to be the symmetric deformation of symmetry A1, a parallel band, among the six fundamental bands of the 03V prolate symmetric top. The v2 bands for both molecules appear in almost the 1, v2(0D3Br)=991.4cm_1), and were reported same region (92(CD3I)=949.4cm- to have sufficient intensity that a long path cell is not necessary for observation of the spectra as long as the sample pressure is higher than 0.1 Torr (l—Z). This chapter is concerned with high resolution infrared studies of the 02 bands of these molecules by means of an infrared-microwave sideband laser spectrometer. As for other methyl halide molecules, the Coriolis interactions between the v2 bands and the v5 bands (asymmetric deformation) of these molecules have been long-standing subjects of study (2,§,§,z). A question concerning the effects of the Coriolis coupling for these bands was one of the reasons for our interest in 73 74 studying the molecules. The main reason for studying them, however, was to determine the magnitude of the nuclear quadrupole coupling constants of the iodine and bromine atoms by the method of infrared-radiofrequency double resonance. The presence of a single nucleus of spin I > 1 in each of these molecules causes each rotational level to be split into 2I+l sublevels. As a result, the lineshapes of transitions in the infrared spectra of these species are distorted and sometimes, especially in CD31 spectra, even split. Direct observations of pure quadrupole transitions by means of infrared-radio frequency double resonance allowed us to determine the magnitude of the quadrupole interaction between the nuclear quadrupole and the electric field gradient at the I or Br nucleus. However, in order to perform the double-resonance study, it was first necessary to have accurate frequencies for linear infrared spectra for the vibration-rotation bands. The experimental frequencies and parameters are reported in this chapter; the infrared-radiofrequency double resonance results are described in the next chapter. 79 3 3 recorded at Doppler-limited resolution. About 200 transitions for each In this work, the v2 bands of 0D I, CD Br, and CD381Br were species, including transitions of high J,K (higher than 40,8), were recorded and the frequencies measured to an accuracy of few MHz. The effect of the quadrupole interaction has been observed for some transitions in the infrared spectrum and the infrared frequencies have been converted to hypothetical unsplit frequencies where necessary. The frequencies in these parallel bands have been combined with frequencies reported from previous microwave, millimeter, and infrared studies and fit by least squares to an energy expression containing centrifhgal 75. distortion parameters up to the eighth order. The Coriolis interaction with the v5 band has been taken into account in each case by using previously-reported parameters (1,1) for the interaction and for the v5 band. The resulting combination of the 02 parameters obtained in this work is sufficient to predict the frequencies within a few MHz for the appropriate range of J and K. The determined parameters have been used to calculate coincidences with CO2 laser frequencies. In a series of microwave studies of the ground vibrational state of CD31 by Simmons and co-workers (8—19) the rotational constant 80 and the centrifugal distortion constants D and DJK were determined. Kuczkowski J (11) extended this microwave work to transitions in the low-lying vibrational states v2, v3, v5, v6, 2v3, and v3+v6. More recently, higher J transitions have been recorded in the millimeter wave region and more accurate quadrupole constants were reported for low-lying vibrational states by Demaison 91 g1. (12) and by Wlodarczak g1 g1. (13.) . The first vibration—rotation spectra of 0D3I were taken by Jones _1 21. (1) with grating spectrometers in the 500-5000 cm.1 region. A series of studies of several bands by different investigators followed (14-19). In 1976 Matsuura and Shimanouchi reported a study of Coriolis coupling of the ”2’ v5, and 2v3 bands (2). Then, as a result of laser- Stark and laser-microwave double resonance spectroscopy, Kawaguchi g; 91. (3) obtained the rotational constant B2, the centrifugal distortion constants DJ and DJK’ and the quadrupole coupling constant qu for the 02 vibrational state in a study in which they found no need to include Coriolis coupling to other states for the rather low J transitions that they recorded. In addition to the vibration-rotation parameters 76 obtained by infrared studies of deuterated methyl iodide, the rotational constant A0 and the centrifugal distortion constant DK were determined by studying the 124 band by Raman spectroscopy (19). Sakai and Katayama (11,11) have performed level-crossing and level-anticrossing experiments in CD31 by using the coincidence of the band with the CO °P(4,1) transition of the v 10P(16) laser line. They 2 2 determined the dipole moments of the ground and v2 vibrational states in this laser Stark study. An intracavity cell and an external cavity White cell were used by Caldow g1 g1. (11) to record laser Stark Lamb dips for this molecule. Infrared radio frequency double resonance at 1- MHz resolution was reported by Rackley and Butcher (14) as part of a study of Stark-tuned non—linear spectroscopy. Mbre recently, Demaison g1 g1. (11) used infrared-radiofrequency double resonance to measure the frequencies of pure quadrupole transitions in the ground state of this molecule with 100 kHz accuracy. Vibrational energy transfer has been studied in CD31 by using coincidences with Q-switched 002 laser lines and detecting fluorescence from v1, v4, ”6’ and 2v5 levels (1Q). The influence of nuclear quadrupole coupling on rotational relaxation has been investigated by means of microwave double resonance (16). Finally, submillimeter wave laser emission has been observed from CD31 pumped by a number of CO2 laser lines (11). Even with all of these spectroscopic studies, there has been no systematic study at Doppler~limited resolution of high J and K transitions in the very important v2 band region of CD31. Such a study would be expected to provide more precise frequency information and to allow investigation of the effect of Coriolis coupling in the calculations of the energies of the levels in the v =1 state. It would 2 77 also allow accurate calculation of possible coincidences between v2~band transitions and CO2 laser lines. The infrared and microwave spectra of CD3Br are rather complicated compared with CD31 for two reasons: First, CD38r consists of two isotopes with almost the same natural abundance (CD37QBr = 50.54%, 81 3 same J,K appear about 500 MHz apart, depending on the value of J and K. CD Br = 49.46%); thus, the transitions of the two species with the Second, the Coriolis interaction between the v2 (991.4 cm-l) and the v5 (1055.5 cm-l) bands is much more serious than in CD31 since the bands lie only 64 cm-1 apart and the Coriolis coupling constants are about 1.5 times larger than that of CD31. As a result, CD Br has not been studied 3 previously in as much detail as CD31. Infrared spectra of the v2 bands of CD379Br and CD381Br recorded with grating instruments have been reported by Morino and Nakamura (4) and by Jones _5 _1. (5). More recently, Betrencourt-Stirnemann £1 _1. (6) analyzed the 02 and v5 bands recorded by Fourier transform spectroscopy at a resolution of 0.01 cm_l. Also, Harada _1 91. observed low J,K transitions and investigated the Coriolis coupling between the 02 and v5 hands by laser—Stark spectroscopy (1) and Edwards and Broderson determined the rotational constant AG by analysis of Raman spectra of the v4 band (18). Microwave spectra in the ground states of CD379Br and CD3818r have been reported by Garrison g1 g1. (19) and have been extended to low—lying excited states by Morino and Hirose (gg). Frequencies reported by these workers (6,1,19,19) were included in our analysis. band of CD Br As implied by the studies performed to date, the 02 3 78 has been one of the major concerns and the Coriolis interaction between the v2 and the 05 bands is very important for analyzing the corresponding rotational energy structure. However, for possible double resonance studies, the previous FT-IR (6) and laser-Stark (1) studies had not provided precise enough frequency information because of the limited resolution as well as a frequency calibration problem. Therefore, experimental frequencies and rovibrational parameters were obtained in this study and are reported for both species. 79 III-2 Theory III-2~l Term Values 2 = 1 states of CD31 and both CD37QBr and CD381Br are The v nondegenerate, so the vibration-rotation energy levels of these states and the ground states of these species can be expressed as the usual power series in J(J+l) and K2, as follows: - _ 2 WR(v,J,K) - vv + Bv J(J+l) + (Av Bv) K J2(J+l)2 - DEX J(J+1)K2 — n” K4 _D K J3(J+l)3 + H3 94¢ Ltd 2 2 2 v 4 v 6 K J (J+1) K + HKJ J(J+1)K + BK K 4 4 3 3 2 v 2 2 4 J (J+1) + L J (J+1) K + LJJKK J (J+1) K v JJJK v 8 6 + LJKKK J(J+1)K + LK K . (3-1) <‘-1< In this expression, ”v is the vibrational energy of the state V (v0 = 0), Av and Bv are rotational constants for the state v, and the D’s, H’s, and L’s are quartic, sextic, and octic centrifugal distortion constants for the state v, respectively. The frequencies corresponding to the experimental frequencies were computed by taking differences in energy levels calculated with the term value written above; the usual selection rules for a parallel band, AJ = 0, :1 and.Ak = 0 (K = lkl) were used. III-2~2 Coriolis Interaction In order to include the effect of the Coriolis coupling on the fitting of the frequencies reported here, we calculated the effect of 80 the coupling for each of the transitions in the fitting and subtracted these effects from the experimental frequencies before completing the fitting. For this purpose, the appropriate matrix was set up for each transition and the eigenvalue was obtained by diagonalizing each matrix; the second order perturbation method is considered not to be adequate because of the large Coriolis effect and the accuracy of frequency determination of this work. The zero-order energy was subtracted from the desired eigenvalue and the difference was subtracted from the experimental frequency. The coupling effects and the subtracted zero- order energies were calculated with the parameters, including the parameters for v2 = 1, reported in previous works where the Coriolis interaction constants are derived. This was done to insure a treatment of the Coriolis effects that was equivalent to the previous analysis, since we do not have any additional data for the other vibrational states involved. III-2~2-l CD3I There are three vibrational states, v2=1 (A1, 949.4 cm-l), v5=l (B, 1049.3 cm_1), and v =2 (A1, 999.0 cm-l), involved in the mid- 3 infrared Coriolis interaction system in CD31 (1). In order to calculate the effect of the Coriolis interaction, the appropriate matrix was set up for each transition as discussed in Ref. (1): 81 |0,0,1,~1;J,k~1> l1,0,0,0,J,k> |0,2,0,0;J,k> |0,0,l,+l;J,k+l> rEo(v5=1,15=~1;J,k~l) ~£25f(J,k~1) ~4335f(J,k~1) ~q5f(J,k-1)f(J,k+1)/27 Eo(v2=1,J,k) 0 £25f(J,k+1) Eo(v3=2;J,k) £335f(J,k+l) (Hermitian) E (v :1’1 0 5 5=l;J.k+1)_ (3-2) In this equation, Eo denotes the unperturbed energy, the "ket" notation is |v2,v3,v5,15;J,k>, the ~q5f(J,k~l)f(J,k+l)/2 term accounts for the (22,12) interaction in the v5=l state, and f(J,ktl) = [J(J+1)~k(ktl)]1/2 . <3-3) For K=0, the matrix is reduced to 3x3 matrices; for the A+ species |1,0,0,0;J,0> l0,2,0,0;J,0> |0,0,l,tl;J,l> E (v =l'J k=0) 0 e {2[J(J+1)]}1/2 I o 2 ’ ' 25 l E (v =2°J k:0) e {2[J(J+l)]}1/2 o 3 ’ ' 335 1 (Hermitian) Eo(v5=l,15=1;J,k=l)+q5J(J+l)/2J (3‘4) and for A_ species that do not affect the v2=l state, . _ O - — o — _ _ |0,0,1,tl,J,1> - E (vs—1,15—1,J,k-l) q5J(J+l)/2 . (3 5) The parameters used in our calculation are given in Table II of Ref. (1). The only ambiguity in this procedure was the specific value to 82 use for B{éfg which affects the value of £25. In Table II of Ref. (1) only the value of [{éfgl is given; the value of B used to obtain the desired product is not mentioned. A value of 3106.495 MHz was used for the combined constant B‘éf; by using the B2 rotational constant of the v2=1 state in the following equation. :25 = <1/2>1/2[(vs/.2)1/2+<.2/.5>1/2]a.;fg . (3-6) The resulting value of £25 was 4398.7 MHz. III-2~2-2 CD3Br The Coriolis coupling between the v2 and v5 bands in these molecules is, as indicated before, somewhat stronger than that between the same bands in CD31 and it was necessary to include this interaction in order to obtain a satisfactory fitting of the frequencies. For this purpose, the effect of the coupling was calculated for each of the transitions by setting up, for the upper state of the transition, the appropriate matrix with elements defined by Eq. (4), (5) and (7) in Ref. (1). The matrix is essentially the same as the one in Eq. (3-2) except that the v3=2 state (1154cm_1) is not included because its effect has been considered to be satisfactorily included in the usual Coriolis contribution to the molecular constants (1). The energies needed to compute the Coriolis contribution were calculated with the parameters, including the parameters for the v2 = 1 state, given in Table V of Ref. (1). 83 III-2~3 Effect of Nuclear Quadrupole Coupling In order to obtain the frequencies of rotational and ro-vibrational transitions, it is necessary to subtract the effect of nuclear quadrupole interactions from the spectra. In order to calculate the effect of quadrupole coupling, the appropriate energy matrix was set up and diagonalized. In this matrix, we also included the effects of centrifugal distortion of the quadrupole coupling and the nuclear spin rotation interaction. To carry out this calculation the energy matrix was written H = HR + H0 + H0 + H8 . (3—7) The matrix HR was assumed to be diagonal with diagonal elements equal to the rotational energies given in Eq. (3-1). The elements of H6, the nuclear quadrupole coupling, were taken to be the elements proportional to er = xzz in the Appendix of the paper by Benz g1 g1. (19); the matrix elements are listed in the Appendix of Chapter IV. The matrices HD and H were also assumed to be diagonal with non— 8 zero matrix elements as follows: e1{[3K2~ J(J+l)][xJJ(J+1) + xKKZ] + *6 K2(4K2~1)} (3-8) 2 _ _ l _ ___§__ _ — 2 [cN+(cK cN) J(J+1)] G . (3 9) In these equations F is the total angular momentum quantum number and e1 is the Casimir function divided by J(J+l); 34 61: [(3/4)G(G+l)-I(I+1)J(J+l)]/[2I(21~1)J(J+1)(2J~1)(2J+3)] (3-10) with G = F(F+1) ~ I(I+l) ~ J(J+1) . (3-11) The constants xJ, XK’ and xd are centrifugal distortion constants for the quadrupole coupling (11,11), whereas CN and CK are spin-rotation constants (11). The signs of the spin rotation constants are taken to be consistent with the signs in the previous work on CD31 (11). Inclusion of the spin-rotation and the centrifugal distortion of the quadrupole coupling terms on the diagonal before the diagonalization was done for convenience. This is almost equivalent to what is desired ~ a first-order perturbation treatment of these terms in a zero-order basis which diagonalizes the quadrupole coupling effects. The only difference is that the distortion and spin-rotation terms have a small effect on the diagonalization. The matrix H, as defined, is diagonal in F, I, and K; therefore, submatrices with rows and columns indexed by J (usually 6x6 for CD3I and 4x4 for CD3Br) were set up and diagonalied to obtain the energy levels. The nuclear quadrupole coupling is discussed in greater detail in the next chapter. III-2~4 Hypothetical Unsplit Frequencies III-2~4-l CD3I In order to obtain the experimental frequencies of the infrared transitions, each experimental lineshape as a function of microwave frequency was fitted by least squares to a sum of Gaussian functions. The relative intensities and separations of the Gaussians were 85 constrained to the values calculated with the highest quality set of quadrupole parameters available at the time of the fitting. Since there was little change in quadrupole parameters and since the quadrupole splittings of many of the transitions were rather small, the hypothetical unsplit frequencies obtained did not depend on the specific set of quadrupole parameters used. Each experimental infrared frequency was obtained by adding or subtracting the resonant microwave frequency to or from the appropriate laser frequency; the laser frequencies were obtained from the report of Freed g1 g1. (15). The microwave and millimeter-wave frequencies measured in previous studies were also converted into hypothetical unsplit frequencies by subtracting the frequency shifts caused by the quadrupole couplings. The frequency shifts were calculated with the same set of quadrupole parameters used for the frequency determination of infrared transitions. The rovibrational parameters were adjusted by a least squares fitting of the modified experimental frequencies including, in addition to the present measurements, microwave and millimeter wave frequencies from Refs. (§~11) and infrared frequencies from the laser-Stark study (1). III-2~4-2 CD3Br In order to obtain the experimental frequencies of the infrared- micrave sideband-laser transitions, each experimental lineshape as a function of microwave frequency was fitted by least squares to a single Gaussian function. Because the shifts in frequency resulting from the hyperfine splitting were less than 5 MHz in nearly every case, it did not seem necessary to fit the lineshapes to a sum of Gaussians, one for 86 each hyperfine component, as was done for CD31 (15); there was no apparent evidence of hyperfine splitting in the Doppler-limited spectra recorded in this work. Each experimental infrared frequency was obtained by adding or subtracting the resonant microwave frequency to or from the appropriate laser frequency, which was obtained from the report of Freed _1 _1. (14). On the other hand, the microwave and millimeter wave frequencies were converted into the corresponding hypothetical unsplit frequencies with the quadrupole coupling constants reported in Ref. (11). The rovibrational parameters were adjusted by a least squares fitting of the experimental frequencies including, in addition to the present measurements, converted microwave and millimeter wave frequencies from Refs. (19) and (11) and infrared frequencies from the FTIR (6) and laser-Stark (18) studies. Each experimental frequency was given a weight equal to the reciprocal of the square of its estimated uncertainty. 87 III-3 Experimental All of the spectra in this work were recorded with an infrared microwave sideband laser spectrometer that has been assembled in our laboratory. Fig. 3~l shows block diagram of the spectrometer used in this study. The design of the electrooptic modulator used is that of Magerl g1 g1. (16) and a detailed description of our spectrometer has already been given in Chapter II. As examples, portions of the spectra of the v bands of CD I and CD38r are shown in Figs. 3~2 and 3~3. The 2 3 horizontal axes of Figs. 3~2 and 3~3 are the microwave frequencies that must be added to or subtracted from the laser frequency to obtain the sideband frequency depending on the sign. The overall accuracy of the frequency scale is limited entirely by our ability to reproduce the known laser frequencies; we estimate this accuracy to be 1150 kHz. The accuracy of the reported frequencies of the transitions was limited by our ability to determine the center frequency of the Doppler-limited absorption lines (Av = ~18.5 MHz); this uncertainty ranges from 2~10 D MHz. The sample cell was a l~meter glass tube with NaCl windows and the samples were obtained from Merck & Co. and used as received except for the usual freeze-pump-thaw cycles. Sample pressures, which were about 0.3 Torr for CD31 and 0.5 Torr for CD3Br, were measured with a capacitance manometer. All spectra were recorded at room temperature (~297 K). 88 ‘ P27 5 EH!” ‘~ , X DET @ CUE LASER V : - 0C. sou “m. 1.1m ln Sample Cell + \ x j DOD. LI Bean \ J [cos I Splrttor :i: REF DET DET PR AMP - - w... m "" PSD PSD ' comm 33.3kHz , PIN Mod. 1 . . W m. COMPUTER Eli Figure 3-1. Block diagram of the infrared microwave sideband laser spectrometer used to record the Doppler-limited vibration-rotation spectra in this work. 88 F27 I n Y 1 4: Hr” P J k DST my (:02 LASER v % - oc. Coll :' Mm 1n Sample Cell Y: ‘—7 F'cumng uni 3,un“—~ 11 L:ns Splitter REF DET PREAMP .___i__,. "" PSD ’cm‘rnm. 33.3kHz ‘ Mod. COMPUTER *4: m Figure 3~1. Block diagram of the infrared microwave sideband laser spectrometer used to record the Doppler-limited vibration-rotation spectra in this work. 89 35 r 1 r 1 . 1 T— 25 - « A 3 1s - cg _- - + £5 5- .J o + + V g, -5)- P(31,8) ‘.’:’ .2 ~15 ~P(2a.0) P(28.1) P(28.2)- -25- - Laser Line: 1201602 10P(28) ._3 . 1 . 1 . L . L, . 154.0 14.2 14.4 14.6 14.8 15.0 Microwave Frequency (GHz) Figure 3~2. A portion of the infrared spectrum of the v2 band of CD31 recorded by the infrared microwave sideband laser spectrometer. The microwave frequency on the horizontal axis is added to (+) or subtracted from (~) the frequency of the 10P(28) 1201502 laser to obtain the infrared frequency. The sample pressure was 0.3 Torr and a l~m path length was used. 90 35 1 1 r 1 a . 254 .v _ 7 1; 4 \N =°-'-' 15- - C 3 4 .1 .9' 5-1 - o 1 . v >4 ~5- -‘ 3:1 61 2 J co; Br man) J 0 -15-4 g . co;"8r P(2o.3) cofar P(20.1) : ~25- "0“02 10R(28) - J . -35 . . . , . , . r . 15.0 15.2 15.4 15.6 15.8 16.0 Microwave Frequency (MHz) Figure 3~3. A small portion of the spectrum in the 02 band region of CD38r showing the typical lineshapes and signal/noise obtained for the spectra reported. The horizontal scale is the microwave frequency that must be subtracted from the frequency of the 1201502 10(28) laser to obtain the infrared frequency of the transitions. Transitions of CD379Br and CD381Br occur approximately alternately everywhere in this region. 91 III-4 Results The Coriolis effects were eliminated from all the experimental frequencies, including the new, more precise infrared frequencies for each species, and the modified frequencies were fit to the differences in energy levels calculated by Eq. (3~1). In the least squares g, H;, and L; were constrained to zero or to the previously-reported values. This was done fittings, the ground-state parameters A0, D to avoid the linear dependence, which is a result of the selection rule, AK=0 for a parallel band. In addition, it was found that all of the L constants for the ground states were too small to affect the calculated frequencies significantly; consequently, these parameters were constrained to zero in the fittings for all three species. III-4-l CD31 Approximately 175 vibration-rotation transitions were recorded with J’s up to 43 and K’s up to 10. Some transitions of higher K were recorded, but these frequencies show the effects of a resonance that cannot be fully accounted for by a power series expansion in J(J+l) and K2; this appears to be the Coriolis resonance with us and 2v3 reported by Matsuura and Shimanouchi (1). A small portion of the infrared spectrum is shown in Fig. 3~2. The frequencies of the infrared transitions measured in this work are shown in Table 3~l with their estimated uncertainties. Also shown in Table 3~l are the observed minus calculated frequencies for the parameters derived in this work. The rotational and centrifugal £32 TABLE 3~1 Comparison of Observed and Calculated Frequencies in the v2 Band of CD31 a b c -1 e Trans. Laser 1:. v/MHz O—C Unc v/cm P(43, 8) 10P(34) ~16 281.8 27 894 439.0 ~l.4 2.0 930.458 33( ~4) P(43, 9) 10P(34) ~14 549.9 27 896 170.9 1.2 2.0 930.516 10( 4) P(43,10) 10P(34) ~13 276.1 27 897 444.7 ~O.8 2.0 930.558 59( ~2) P(42, 0) 10P(34) ~11 245.0 27 899 475.8 ~0.1 2.0 930.626 34( 0) P(42, 1) 10P(34) ~11 065.0 27 899 .8 0.0 2.0 930.632 34( 0) P(42, 2) 10P(34) ~10 523.8 27 900 .0 1.8 2.0 930.650 40( 5) P(42, 4) 10P(34) ~8 427.0 27 902 .8 0.3 2.0 980.720 34( 1) P(4l, 7) 10P(34) 11 582.2 27 922 .0 ~1.7 2.0 931.387 77( ~5) P(41, 9) 10P(34) 15 616.4 27 926 .2 3.0 2.0 931.522 34( 9) P(4l,10) 10P(34) 17 209.9 27 927 .7 0.2 2.0 931.575 49( 0) P(40, 0) 10P(34) 17 931.4 27 928 .2 ~0.2 2.0 931 599 56( 0) P(39, 8) 10P(32) ~15 410.7 27 954 .l ~0.5 2.0 932 446 38( ~1) P(39, 9) 10P(32) ~13 208.4 27 956 .4 0.8 2.0 932 519 84( 2) P(39,10) 10P(32) ~11 300.8 27 958 .0 .9 2.0 932 583 47( ~6) P(38, 0) 10P(32) ~11 854.6 27 957 .2 .3 2.0 932 564 99( ~1) P(38, 2) 10P(32) ~11 076.9 27 958 .9 .5 2.0 932 590 94( ~5) P(38, 4) 10P(32) ~8 788.5 27 960 .3 .2 2.0 932 667 27( 0) P(37, 6) 10P(32) 9 350.3 27 978 .1 .9 10.0 933 272 31( ~2) P(37, 8) 10P(32) 14 007.1 27 983 .9 .6 2.0 933 427 65( ~2) P(37, 9) 10P(32) 16 427.3 27 985 .1 .7 OM T 933 508 38(-25) P(36, 0) 10P(32) 16 854.0 27 986 .8 .2 2.0 933.522 61( 0) P(36, 1) 10P(32) 17 055.9 27 986 .7 .2 2.0 933.529 35( 0) P(35, 7) 10P(30) ~17 386.1 28 010 .8 .0 2.0 934.314 56( 3) P(35, 8) 10P(30) ~14 815.2 28 012 .7 .2 2.0 934.400 31( 0) P(35, 9) 10P(30) ~12 168.2 28 015 .7 .5 2.0 934.488 61( 1) P(35,10) 10P(30) -9 654.9 28 017 .0 .5 2.0 934.572 44( ~1) P(34, 0) 10P(30) ~12 657.9 28 014 .0 .8 2.0 934.472 27( ~2) P(34, 1) 10P(30) ~12 448.6 28 014 .3 .2 2.0 934.479 26( 0) P(34, 2) 10P(30) ~11 823.6 28 015 .3 .1 2.0 934.500 10( 0) P(34, 3) 10P(30) ~10 789.0 28 016 .9 .2 2.0 934.534 61( 4) P(34, 4) 10P(30) ~9 363.5 28 018 .4 1.2 2.0 934.582 16( ~3) P(33, 6) 10P(30) 8 860.2 28 036 .1 0.8 0.0 935.190 04( 2) P(33, 7) 10P(30) 11 352.8 28 038 .7 0.2 2.0 935.273 18( 0) P(33, 9) 10P(30) 16 941.7 28 044 .6 1.9 2.0 935.459 61( 6) P(32, 0) 10P(30) 15 576.1 28 043 .0 0.5 2.0 935.414 06( l) P(32, 1) 10P(30) 15 790.6 28 043 .5 ~0.1 2.0 935.421 21( 0) P(32, 2) 10P(30) 16 429.3 28 043 .2 ~5.4 2.0 935.442 52(-l7) P(32, 3) 10P(30) 17 502.3 28 044 .2 1.5 2.0 935.478 31( 5) P(3l, 7) 10P(28) ~17 404.3 28 067 . ~0.9 2.0 936.223 20( ~2) P(3l, 8) 10P(28) ~14 522.9 28 070 ~0.4 2.0 936.319 32( ~1) 533 Table 3~1 (cont’d) Trans . Laser“ vlb v/MHz O-Cc Unc v/cm 1 e P(31, 9) 10P(28) ~11 463.1 28 073 206.7 ~0.1 2.0 936.421 P(3l,10) 10P(28) ~8 384.2 28 076 285.6 ~0.5 2.0 936.524 P(30, 0) 10P(28) ~13 669.8 28 071 000.0 ~0.1 2.0 936.347 P(30, l) 10P(28) ~13 448.8 28 071 221.0 ~0.2 2.0 936.355 P(30, 2) 10P(28) ~12 784.6 28 071 885.2 1.9 2.0 936.377 P(30, 3) 10P(28) ~11 689.7 28 072 980.1 ~0.3 2.0 936.413 P(30, 4) 10P(28) ~10 166.3 28 074 503.5 1.1 2.0 936.464 P(30, 5) 10P(28) ~8 238.5 28 076 431.3 ~1.7 2.0 936.528 P(29, 7) 10P(28) 10 818.0 28 095 487.8 ~0.1 2.0 937.164 P(29, 8) 10P(28) 13 843 l 28 098 512.9 0.4 2.0 937.265 P(29, 9) 10P(28) 17 095.8 28 101 765.6 0.9 2.0 937.374 P(28, 0) 10P(28) 14 084.6 28 098 754.4 3.4 2.0 937.273 P(28, 1) 10P(28) 14 308.5 28 098 978.3 0.6 2.0 937.281 P(28, 2) 10P(28) 14 987.7 28 099 657.5 0.7 2.0 937.303 P(28, 3) 10P(28) 16 115.2 28 100 785.0 1.7 2.0 937.341 P(28, 4) 10P(28) 17 678.4 28 102 348.2 ~0.3 2.0 937.393 P(27, 7) 10P(26) ~17 720.3 28 123 445.7 ~0.9 2.0 938.097 P(27, 8) 10P(26) ~14 559.0 28 126 607.0 0.0 2.0 938.202 P(27, 9) 10P(26) ~11 124.4 28 130 041.6 ~0.4 2.0 938.317 P(26, 0) 10P(26) ~14 908.7 28 126 257.3 ~1.2 2.0 938.190 P(26, l) 10P(26) ~14 676.6 28 126 489.4 ~l.l 2.0 938.198 P(26, 2) 10P(26) ~13 979.0 28 127 187.0 1.4 2.0 938.221 P(26, 3) 10P(26) ~12 826.5 28 128 339.5 ~0.1 2.0 938.260 P(26, 4) 10P(26) ~11 221.0 28 129 945.0 ~0.2 2.0 938.313 P(26, 5) 10P(26) ~9 176.3 28 131 989.7 ~1.4 2.0 938.382 P(25, 7) 10P(26) 9 975.2 28 151 141.2 1.0 2.0 939.020 P(25, 9) 10P(26) 16 869.6 28 158 035.6 0.3 2.0 939.250 P(24, 0) 10P(26) 12 355.6 28 153 521.6 0.4 2.0 939.100 P(24, 1) 10P(26) 12 592.1 28 153 758.1 0.0 2.0 939.108 P(24, 3) 10P(26) 14 480.2 28 155 646.2 ~1.4 2.0 939.171 P(24, 4) 10P(26) 16 126.1 28 157 292.1 1.1 2.0 939.226 P(24,ll) 10P(24) ~16 992.6 28 179 930.0 ~4.8 OMIT 939.981 P(23, 8) 10P(24) ~14 950.7 28 181 971.9 ~1.3 2.0 940.049 P(23, 9) 10P(24) ~11 182.7 28 185 739.9 ~1.3 2.0 940.175 P(22, 0) 10P(24) ~16 385.3 28 180 537.3 ~0.3 2.0 940.001 P(22, l) 10P(24) ~16 143.2 28 180 779.4 0.4 2.0 940.009 P(22. 2) 10P(24) ~15 421.2 28 181 501.4 ~1.2 2.0 940.033 P(22, 3) 10P(24) ~14 215.7 28 182 706.9 1.0 2.0 940.073 P(22, 5) 10P(24) ~10 388.8 28 186 533.8 3.6 2.0 940.201 P(21, 7) 10P(24) 8 800.3 28 205 722.9 ~0.1 2.0 940.841 94» Table 3~1 (cont'd) a b ~1 e Trans. Laser 0 u/MHz O E O c \ 8 P(Zl, 8) 10P(24) 12 316. 28 209 239.3 ~0. 940.958 94( ~1) 7 4 2.0 P(21, 9) 10P(24) 16 234.9 28 213 157.5 0.8 2.0 941.089 64( 2) P(20, l) 10P(24) 10 628.1 28 207 550.7 ~l.l 2.0 940.902 61( ~3) P(20, 2) 10P(24) 11 365.9 28 208 288.5 0.5 2.0 940.927 22( 1) P(20, 4) 10P(24) 14 301.8 28 211 224.4 1.4 2.0 941.025 15( 4) P(20, 5) 10P(24) 16 491.1 28 213 413.7 0.5 2.0 941.098 18( l) P(19, 8) 10P(22) ~15 718.6 28 236 223.1 ~2.1 2.0 941.859 02( ~7) P(19, 9) 10P(22) ~11 664.3 28 240 277.4 ~1.4 2.0 941.994 26( ~4) P(18, l) 10P(22) ~17 867.0 28 234 074.7 ~0.3 2.0 941.787 36( ~1) P(18, 2) 10P(22) ~17 119.7 28 234 822.0 ~0.6 2.0 941.812 29( ~1) P(18, 3) 10P(22) ~15 874.7 28 236 067.0 0.0 2.0 941.853 81( 0) P(18, 4) 10P(22) ~14 135.8 28 237 805.9 ~0.1 2.0 941.911 82( 0) P(18, 5) 10P(22) ~11 905.3 28 240 036.4 0.1 2.0 941.986 22( 0) P(l7, 9) 10P(22) 15 162.6 28 267 104.3 ~0.3 2.0 942.889 11( ~1) P(16, 0) 10P(22) 8 153.0 28 260 094.7 ~0.2 2.0 942.655 29( 0) P(16, l) 10P(22) 8 406.6 28 260 348.3 0.8 2.0 942.663 75( 2) P(16, 2) 10P(22) 9 179.5 28 261 121.2 16.1 OMIT 942.689 53( 53) P(16, 3) 10P(22) 10 425.2 28 262 366.9 ~0.1 2.0 942.731 08( 0) P(16, 4) 10P(22) 12 190.9 28 264 132.6 0.7 2.0 942.789 98( 2) P(16, 5) 10P(22) 14 456.3 28 266 398.0 0.2 2.0 942.865 55( 0) P(16, 6) 10P(22) 17 220.9 28 269 162.6 0.3 2.0 942.957 76( 1) P(15, 8) 10P(20) ~16 881.2 28 289 343.7 ~0.4 2.0 943.630 93( ~1) P(15, 9) 10P(20) ~12 599.2 28 293 625.7 ~6.0 2.0 943.773 77(-20) P(l4, 3) 10P(20) ~17 813.8 28 288 411.1 ~0.5 2.0 943.599 83( ~1) P(l4, 4) 10P(20) ~16 026.6 28 290 198.3 ~0.8 2.0 943.659 44( ~2) P(l4, 5) 10P(20) ~13 729.2 28 292 495.7 ~0.8 2.0 943.736 07( ~2) P(14, 6) 10P(20) ~10 923.4 28 295 301.5 ~1.7 2.0 943.829 66( ~5) P(12, 4) 10P(20) 9 781.8 28 316 006.7 0.3 2.0 944.520 32( 0) P(12, 5) 10P(20) 12 106.5 28 318 331.4 0.6 2.0 944.597 86( 2) P(12, 6) 10P(20) 14 948.9 28 321 173.8 ~0.1 2.0 944.692 67( 0) P(10, 5) 10P(18) ~15 872.4 28 343 901.4 2.0 2.0 945.450 78( 6) P( 9, 0) 10P(18) ~9 728.1 28 350 045.7 ~l.5 2.0 945.655 73( ~4) P( 9, 1) 10P(18) ~9 467.5 28 350 306.3 ~1.9 2.0 945.664 43( ~6) P( 9, 2) 10P(18) ~8 683.1 28 351 090.7 ~0.6 2.0 945.690 59( ~1) P( 7, O) 10P(18) 15 400.3 28 375 174.1 ~0.7 2.0 946.493 93( ~2) P( 7, 1) 10P(18) 15 662.7 28 375 436.5 ~0.7 2.0 946.502 68( ~2) P( 7, 2) 10P(18) 16 450.7 28 376 224.5 ~0.2 2.0 946.528 97( 0) P( 7, 3) 10P(18) 17 764.3 28 377 538.1 ~0.1 2.0 946.572 78( 0) P( 5, 0) 108(16) ~12 543.2 28 400 046.5 0.6 2.0 947.323 58( 2) P( 5, 2) 10P(16) ~11 491.8 28 401 097.9 ~1.9 4.0 947.358 65( ~6) 95 Table 3~1 (cont’d) Trans. Lasera v-b v/MHz O—Cc Dnc v/cm 1 e P( 5, 3) 10P(16) ~10 167.9 28 402 421.8 3.1 2.1 947.402 81( 10) 0(16,10) 10P(14) 12 199.1 28 476 872.8 5.0 2.0 949.886 23( 16) 0(15, 9) 10P(14) 8 835.1 28 473 508.8 ~0.5 2.0 949.774 02( ~1) 0(15,10) 10P(14) 13 516.7 28 478 190.4 0.5 2.0 949.930 18( 1) 0(14, 9) 10P(14) 10 001.5 28 474 675.2 1.9 10.0 949.812 93( 6) 0(14,10) 10P(14) 14 757.4 28 479 431.1 0.3 2.0 949.971 57( 0) 0(13, 9) 10P(14) 11 087.6 28 475 761.3 0.7 2.0 949.849 16( 2) 0(13,10) 10P(14) 15 918.9 28 480 592.6 2.2 2.0 950.010 31( 7) 0(12, 9) 10P(14) 12 096.0 28 476 769.7 ~1.4 2.0 949.882 79( ~4) 0(12,10) 10P(14) 16 996.0 28 481 669.7 1.4 2.0 950.046 24( 4) 0(11, 8) 10P(14) 8 621.4 28 473 295.1 ~1.9 2.0 949.766 89( ~6) 0(11,10) 10P(14) 17 990.2 28 482 663.9 ~0.4 10.0 950.079 40( ~1) 0(10, 8) 10P(14) 9 438.0 28 474 111.7 ~0.5 2.0 949.794 13( ~1) 0(10, 9) 10P(14) 13 886.2 28 478 559.9 ~0.9 2.0 949.942 51( ~3) 0( 9, 8) 10P(14) 10 177.8 28 474 851.5 ~2.2 2.0 949.818 81( ~7) 0( 9, 9) 10P(14) 14 666.1 28 479 339.8 0.0 2.0 949.968 52( 0) 0( 8, 8) 10P(14) 10 848.7 28 475 522.4 1.1 2.0 949.841 19( 3) R( 5, 1) 10P(12) 16 448.8 28 532 475.5 0.1 2.0 951.740 94( 0) R( 5, 2) 10P(12) 17 233.2 28 533 259.9 0.8 2.0 951.767 10( 2) R( 7, 0) 10P(10) -ll 252.3 28 555 396.9 ~1.9 2.0 952.505 51( ~6) R( 7, 1) 10P(10) ~10 992.5 28 555 656.7 ~1.5 2.0 952.514 18( ~4) R( 7, 2) 10P(10) ~10 211.9 28 556 437.3 0.9 2.0 952.540 22( 3) R( 7, 3) 10P(10) ~8 915.9 28 557 733.3 ~0.8 2.0 952.583 45( ~2) R( 9, 0) 10P(10) 11 672.2 28 578 321.4 ~0.4 2.0 953.270 19( ~1) R( 9, 1) 10P(10) 11 929.9 28 578 579.1 0.2 2.0 953.278 79( 0) R( 9, 2) 10P(10) 12 701.2 28 579 350.4 0.1 2.0 953.304 52( 0) R( 9, 3) 10P(10) 13 986.8 28 580 636.0 ~0.2 2.0 953.347 40( 0) R( 9, 4) 10P(10) 15 789.5 28 582 438.7 1.1 2.0 953.407 53( 3) R(1l, 0) 10P(8) ~15 560.0 28 600 981.8 ~0.9 2.0 954.026 06( ~3) R(ll, 1) 10P(8) ~15 306.5 28 601 235.3 ~l.8 2.0 954.034 52( ~6) R(ll, 2) 10P(8) ~14 542.2 28 601 999.6 ~0.8 2.0 954.060 01( ~2) R(ll, 3) 10P(8) ~13 269.7 28 603 272.1 ~0.3 2.0 954.102 46( O) R(ll, 5) 10P(8) ~9 200.1 28 607 341.7 ~1.2 2.0 954.238 21( ~3) R(13, 3) 10P(8) 9 100.3 28 625 642.1 ~0.2 2.0 954.848 64( 0) R(13, 4) 10P(8) 10 860.5 28 627 402.3 3.0 2.0 954.907 35( 10) R(13, 5) 10P(8) 13 119.0 28 629 660.8 4.5 2.0 954.982 69( 15) R(13, 6) 10P(8) 15 877.0 28 632 418.8 7.0 2.0 955.074 69( 23) R(14, 0) 10P(8) 17 940.5 28 634 482.3 0.2 2.0 955.143 52( 0) R(14, 8) 10P(6) ~15 337.9 28 650 366.7 ~0.8 2.0 955.673 36( ~2) R(14, 9) 10P(6) ~11 154.5 28 654 0.1 ~0.8 2.0 955.812 91( ~2) S36 Table 3~1 (cont’d) Trans. Lasera v-b v/MHz O—Cc Uncd v/cm 1 e R(15, 3) 10P(6) ~17 959.0 28 647 745.6 ~0.1 2.0 955.585 93( 0) R(15, 4) 10P(6) ~16 229.2 28 649 475.4 ~0.3 2.0 955.643 63( ~1) R(15, 5) 10P(6) ~14 008.4 28 651 696.2 0.5 2.0 955.717 71( l) R(15, 6) 10P(6) ~11 304.5 28 654 400.1 ~1.7 2.0 955.807 90( ~5) R(16, 0) 10P(6) ~9 217.4 28 656 487.2 0.6 2.0 955.877 52( 2) R(16, l) 10P(6) ~8 972.9 28 656 731.7 ~0.8 2.0 955.885 68( ~2) R(16, 2) 10P(6) ~8 238.0 28 657 466.6 ~3.3 2.0 955.910 19(-10) R(16,10) 10P(6) 14 915.2 28 680 619.8 21.7 OMIT 956.682 50( 72) R(17, 6) 10P(6) 10 408.6 28 676 113.2 1.2 2.0 956.532 18( 3) R(17, 8) 10P(6) 17 084.6 28 682 789.2 ~0.8 2.0 956.754 86( ~2) R(18, 0) 10P(6) 12 524.0 28 678 228.6 0.4 2.0 956.602 74( 1) R(18, l) 10P(6) 12 766.5 28 678 471.1 1.2 2.0 956.610 83( 3) R(18, 3) 10P(6) 14 696.9 28 680 401.5 0.6 2.0 956.675 22( 2) R(18, 4) 10P(6) 16 381.8 28 682 086.4 1.7 2.0 956.731 42( 5) aCO2 laser line used (1201602); laser frequencies were taken from Ref. 34. bMicrowave frequency in MHz. The signed microwave frequency was added to the laser frequency to obtain the absorption frequency. cObserved minus calculated frequency in MHz; the parameters for the calculation are in the second column in Table 3~2 and the second column of Table 3~4. dEstimated uncertainty in the observed frequency in MHz. An "OMIT" means that the frequency was omitted from the least squares fits. eObserved wavenumber in cm-l. The numbers in parentheses are observed minus calculated wavenumbers in units of 0.00001 cm 7 97 distortion constants obtained by least squares fitting of the hypothetical unsplit rotation and vibration-rotation frequencies are given in Tables 3~2 and 3~3 for the ground and v = 1 states, 2 respectively. In Table 3~3 the Coriolis effects described above were ignored. Table 3-4 contains the corresponding parameters for v2 = l for fittings in which the Coriolis coupling to us and 2v3 was included. Finally, the parameters in Tables 3~2 and 3~3 have been used to calculate coincidences within 1200 MHz of CO2 laser frequencies for transitions with J S 40 and K S 10 in the v2 band of CD31, and these are listed in Table 3~5. For this calculation, the laser frequencies were taken from Refs. (14) and (18). III~4~2 003Br The infrared frequencies measured in this work are given in Tables 3~6 and 3~7 for CD 7gBr and CD 3 fitting was done with more than 1200 experimental frequencies for each 3818r, respectively. The least squares species, including approximately 230 and 190 new, more precise infrared frequencies for CD37QBr and CD3818r, respectively. For both species, ground state molecular parameters A0 and DK were constrained to the values reported by Edwards and Broderson (11). H; and L; are constrained to zero so that only AHK and ALK for v2 = l are reported. The determined molecular constants are shown in Tables 3-8 and 3~9 for 3798r and CD381Br, respectively. Although the values in these tables CD are approximations to deperturbed parameters, with the effects of the v2~v5 Coriolis coupling removed, until a complete fitting of both bands 98 TABLE 3~2 Comparison of Ground State Rotational Constants of CD318 Parameter This Workb This Workc Wlodarczakd Bo /MHz ’6 040.297 40 (47) 6 040.297 77 (22) 6 040.297 28 (38) DJ /kHz 3.722 63 (60) 3.722 60 (32) 3.721 88 (30) DJK /kHz 48.294 8 (40) 48.294 5 (16) 48.296 3 (36) BJ /Hz ~0.001 346(145) ~0.001 358(78) ~0.001 530(60) HJK /Hz 0.043 41 (320) 0.033 47(152) 0.037 75(192) HKJ /Hz 0.998 5 (108) 1.017 8 (38) 1.008 0 (63) 8Values in parentheses are one standard deviation in multiples of the last digit in the parameter. bObtained from fit of vibration-rotation frequencies listed in Table 3~1 and hypothetical unsplit rotational frequencies calculated from References (1,11-11). cObtained from fit of rotational frequencies from references (11-11) and pure quadrupole frequencies in Table V of Ref. 5 and in Table 4-1. dFrom Table VI in Ref. 6. Molecular Constants of the v2 539 TABLE 3~3 Coriolis Corrections = 1 State of CD I Without Parameterb This Workc This Workd Kawaguchie Ev /GHz 28 461.093 3 (9) 28 461.093 3 (15) 28 461.093 8(14) Bv /MBz 6 007.878 0 (28) 6 007.878 4 (46) 6 007.873 (8)f 6(Av-Bv) /MHz 264.71 (13) 264.71 (22) 266.4 (4) DJ M12 3.557 4(171) 3.557 4(287) 3.6‘ f DJK /kRz 102.265 (249) 102.263 (421) 106. (2) ADK /kHz 19.6 (58) 19.6 (98) 121. (34) BJK /Bz 1.374 (182) 1.362 (309) HEJ /Hz ~186.01 (400) ~185.95 (677) AH: /Bz 1136. (93) 1136. (157) LJJJK /mHz ~0.242 (57) ~0.242 (96) LJJKK /mHz 48.77 (157) 48.78 (27) LJKKK /mBz ~1988.5 (243) ~1988.4 (411) ALK /mBz ~3562. (475) ~3563. (804) .Values in parentheses are one standard deviation in multiples of the last digit in the parameter. b Vibration-rotation parameters. AP = P(v2=l) - P(v2=0). constrained to zero in both fits in this work. HJ and LJ were cObtained from a fit of the vibration-rotation frequencies listed in Table 3~3 and hypothetical unsplit rotational frequencies calculated from References (1,11~_l_3_). dObtained from a fit of the frequencies described in previous footnote with the ground state parameters constrained to the parameters in Table 3~2 (Column 2). 3Obtained from Table V in Ref. 1. f Obtained from Ref. 11 (Tables VIII and X). ‘Assumed to be the same as in the ground state. 1(10 TABLE 3~4 Molecular Constants of the v2 3 = 1 State of CD I with Coriolis Correctiona Parameterb This Workc This Workd Matsuurae Ev /GBz 28 461.095 4 (6) 28 461.095 4 (14) 28 461.094 7 (18) Bv /M82 6 020.287 0 (33) 6 020.287 2 (75) 6 020.339 2 (180) A( Av-Bv) /MHz 252 . 328 (47) 252 . 328 (105) 250 . 600 (180) DJ /kHz 3.692 3 (50) 3.692 1 (113) 4.197 1(8894) DJK /kHz 52.56 (16) 52.56 (37) 54.86 (60) ADK /kHz 13.8 (5) 13.8 (12) 8.1 (15) BJ /Hz ~0.006 4 (20) ~0.006 5 (46) 833 /Hz 0.454 (137) 0.439 (311) HEJ /Hz ~13.46 (22) ~13.38 (50) LJJJK /mHz ~0.059 (50) ~0.057 (113) LJJEK /mHz 2.78 (106) 2.77 (240) LJKEK /mHz ~77.9 (111) ~77.8 (251) aEffects of Coriolis interaction with us and 203 states were subtracted from the experimental frequencies before fitting. The Coriolis parameters in Table II of Ref. 1 were used except that (25 = 4398.7 MHz. Values in parentheses are one standard deviation in multiples of the last digit in the parameter. b . . . _ _ _ _ Vibration-rotation parameters. AP - P(vz-l) P(vz-O). ABK, ALK, and were constrained to zero for both fittings in this work. LJ cObtained from full fit of vibration-rotation frequencies listed in Table 3~1 and hypothetical unsplit rotational frequencies calculated from References (gall-1:3.) . dObtained from fit of frequencies described in previous footnote with the ground state parameters constrained to the parameters in Table V (Column 2). eObtained from Table 11 in Ref. 2. 101 TABLE 3~5 Coincidences between Calculated Frequencies for the 02 Band of CD31 and Laser Frequencies Trans.a Frequencyb vO-DLC Laserd P(40,10) 27 943 074.3 ~62.5 N20 P( 8) P(39, 0) 27 943 156.3 19.5 N20 P( 8) P(38, 8) 27 968 783.7 ~79.4 N20 P( 7) P(34, 4) 28 018 067.4 ~140.9 1301802 BAND I R( 8) P(34, 5) 28 019 870.2 ~142.8 N20 P( 5) P(32, 6) 28 050 509.7 ~15.6 120160180 BAND P(36) P(31, l) 28 057 251.8 7.2 1201802 BAND I P(38) P(27, 2) 28 113 451.9 ~15.0 1201802 BAND I P(36) P(25, 4) 28 143 652.0 ~192.6 1301602 BAND I R(36) P(24, 7) 28 164 886.5 ~63.3 120160180 BAND P(32) P(23, 4) 28 170 871.8 ~161.5 N20 R( 0) P(20, 5) 28 213 414.7 ~90.7 1301602 BAND I R(40) P(19, 0) 28 220 595.4 35.0 N20 R( 2) P(19, l) 28 220 843.5 ~135.5 120160180 BAND P(30) P(19, 8) 28 236 223.1 ~98.7 1301802 BAND 1 R(20) P(l7, l) 28 247 241.6 ~145.5 1301602 BAND I R(42) P(16, 8) 28 276 169.4 ~53.6 120160180 BAND P(28) P(15, 4) 28 277 199.9 ~89.9 1201802 BAND I P(30) P(12, 5) 28 318 329.9 ~59.0 N20 R( 6) P( 9, 8) 28 366 860.0 171.8 N20 R( 8) P( 8, 4) 28 366 837.5 149.3 N20 R( 8) P( 4, l) 28 412 648.0 58.3 1201602 BAND I P(16) P( 4, 3) 28 414 762.8 186.9 N20 R(lO) P( 2, 1) 28 437 133.0 16.8 1301602 BAND I R(54) Q( 2, 2) 28 461 956.9 ~94.1 N20 R(12) Q( 4, 4) 28 464 662.3 ~ll.5 1201602 BAND I P(l4) Q( 6, 3) 28 462 093.1 42.1 N20 R(12) Q( 6, 5) 28 466 291.8 -138.9 1301602 BAND I R(56) Q( 7, 4) 28 463 462.3 41.6 120160180 BAND P(21) Q( 9, 2) 28 459 216.0 ~108.5 1301802 BAND I R(34) Q( 9, 5) 28 464 664.9 ~8.8 1201602 BAND I P(14) 0(11, 3) 28 459 132.4 ~192.l 1301802 BAND I R(34) 0(11, 5) 28 463 242.3 ~178.4 120160180 BAND P(21) 0(13, 4) 28 459 266.8 ~57.7 1301802 BAND I R(34) 0(14, 6) 28 463 370.0 ~50.7 120160180 BAND P(21) 0(17, 7) 28 463 223.4 ~197.3 120160180 BAND P(21) 0(18, 7) 28 461 944.5 ~106.6 N20 R(12) 0(20, 7) 28 459 176.5 ~148.0 1301802 BAND I R(34) 0(20, 9) 28 466 547.9 117.2 1301602 BAND I R(56) 102 Table 3~5 (cont’d) Trans.a Frequencyb vo~vLc Laserd 0(22, 8) 28 459 502.0 177.5 1301802 BAND I R(34) 0(22, 9) 28 463 233.7 ~187.0 120160180 BAND I P(21) Q(24,10) 28 463 420.8 0.1 120160180 BAND I P(21) Q(26,10) 28 459 271.3 ~53.2 1301802 BAND I R(34) 0(28, 4) 28 438 387.0 21.8 N20 R(ll) 0(29, 2) 28 433 887.0 1.6 1201802 BAND I P(24) 0(29, 5) 28 438 378.2 13.0 N20 R(ll) 0(33, 8) 28 437 044.5 ~7l.7 1301602 BAND I R(54) 0(34, 6) 28 429 733.7 160.7 1301802 BAND I R(32) 0(34, 9) 28 437 165.9 49.7 1301602 BAND I R(54) 0(35, 7) 28 429 619.7 46.8 1301802 BAND I R(32) 0(36, 8) 28 429 459.2 ~ll3.8 1301802 BAND I R(32) Q(36,10) 28 433 976.2 90.8 1201802 BAND I P(24) 0(39, 1) 28 411 108.9 198.8 120160180 BAND I P(23) 0(39, 3) 28 412 554.7 ~35.0 1201602 BAND I P(16) 0(40, 5) 28 412 686.6 96.9 1201602 BAND I P(16) 0(40, 6) 28 414 451.0 ~124.9 N20 R(lO) R( 3, l) 28 509 030.3 ~82.0 N20 R(l4) R( 5, 1) 28 532 474.6 ~12.7 N20 R(15) R( 7, l) 28 555 657.3 ~101.1 N20 R(16) R( 8, 4) 28 571 030.1 ~156.3 1301802 BAND I R(42) R(ll, 2) 28 602 001.0 13.0 N20 R(l8) R(12, 4) 28 616 261.8 ~31.4 120160180 BAND I P(15) R(15, 3) 28 647 747.7 ~52.3 N20 R(20) R(17, 4) 28 671 284.9 ~136.7 1301802 BAND I R(50) R(18, 7) 28 689 934.8 ~180.2 120160180 BAND I P(12) R(19, 2) 28 689 958.4 ~156.6 120160180 BAND I P(12) R(21, 4) 28 714 089.3 ~48.4 1201602 BAND I P( 4) R(22, 6) 28 729 166.7 132.0 1301602 BAND II P(60) R(22, 9) 28 738 957.4 169.5 1301802 BAND I R(56) R(26,10) 28 782 703.7 ~12.0 N20 R(26) R(30, 3) 28 805 022.6 190.4 N20 R(27) R(31, 4) 28 816 383.4 ~17.l 1201802 BAND I P( 8) R(32, 7) 28 832 413.2 ~127.6 120160180 BAND I P( 6) R(35, 4) 28 855 419.2 ~183.2 120160180 BAND I P( 5) R(36, 7) 28 870 580.4 36.0 N20 R(30) R(37, 6) 28 877 919.1 16.7 1201602 BAND I R( 2) R(39, 3) 28 892 201.6 ~33.9 N20 R(31) R(3l, 4) 28 816 383.4 ~l7.1 1201802 BAND I P( 8) aTransition in the v2 band of CD3I; J S 40, k S 10. Frequency of the 02 band transition in MHz. 103 cFrequency of the v2 band transition minus the laser frequency in MHz. dIdentification of 002 or N20 laser. Band I is 10 pm band; band 11 is 9 pm band. Laser frequencies were obtained from Refs. 14 and 11. 104 TABLE 3~6 79 Comparison of Observed and Calculated Frequencies in the 02 Band of CD3 Br Trans.a Laserb v-c v/MBz v/cm l f P(45, 5) 1201602 10R( 4) 854.1 28 907 192.3 5.0 964.240 13( ~17) P(45, 4) 1201602 10R( 4) 408.0 28 910 638.4 5.0 964.355 09( ~9) P(45, 3) 1201602 lOR( 4) 318.5 28 912 728.0 5.0 964.424 79( 6) P(44, 7) 1201602 10R( 4) ~9 531.6 28 913 514.9 10.0 964.451 04( 13) P(45, 2) 1201602 10R( 4) ~9 098.0 28 913 948.4 5.0 964.465 50( 6) P(45, 1) 1201602 10R( 4) -8 464.0 28 914 582.4 5.0 964.486 65( ~2) P(45, 0) 1201602 10R( 4) ~8 269.5 28 914 776.9 5.0 964.493 14( ~12) P(44, 4) 1201602 lOR( 4) 8 086.2 931 132.7 10.0 965.038 71( ~9) P(44, 3) 1201602 lOR( 4) 029.2 933 075.6 5.0 965.103 52( 11) P(44, 1) 1201602 lOR( 4) 729.7 934 776.1 20.0 965.160 24( 5) P(43, 7) 1201602 10R( 4) 769.3 934 815.7 20.0 965.161 56( 35) P(44, 0) 1201602 10R( 4) 909.3 934 955.8 5.0 965.166 23( 7) P(43, 4) 1201602 10R( 6) 917.3 951 539.8 5.0 965.719 42( ~4) P(43, 3) 1201602 10R( 6) 125.6 953 331.4 5.0 965.779 l7( 4) P(43, 2) 1201602 10R( 6) 101.6 954 355.4 5.0 965.813 34( 5) P(42, 7) 1201602 10R( 6) 435.7 956 021.3 5.0 965.868 91( 14) P(38,10) 1201602 10R( 6) 085.6 958 371.5 5.0 965.947 30( 3) P(41, 7) 1201602 10R( 6) 691.5 977 148.6 10.0 966.573 62( 13) P(40, 8) 1201602 lOR( 6) 369.9 984 826.9 10.0 966.829 75( 5) P(41, 6) 1201602 10R( 6) 513.5 984 970.6 5.0 966.834 55( ~13) P(4l, 3) 1201602 lOR( 8) 557.5 993 575.5 .0 967.121 57( 5) P(4l, 2) 1201602 10R( 8) 730.1 994 402.9 .0 967.149 18( 1) P(41, 1) 1201602 10R( 8) 319.2 994 813.8 .0 967.162 87( ~5) P(41, 0) 1201602 lOR( 8) 191.9 994 941.1 .0 967.167 13( 4) P(40, 7) 1201602 10R( 8) 944.9 998 188.1 5.0 967.275 44( 10) P(39, 6) 1201602 10R( 8) 013.3 026 146.3 20.0 968.208 02( ~17) R(37, 9) 1201602 lOR( 8) 056.7 026 189.7 OMIT 968.209 47(-649) P(38, 8) 1201602 10R( 8) 622.2 027 755.2 5.0 968.261 69( 0) P(38, 7) 1201602 10R(10) 072.1 040 000.6 5.0 968.670 15( 14) R(37, 6) 1201602 10R(10) 870.9 066 943.6 5.0 969.568 86( ~10) P(36, 8) 1201602 10R(10) 283.9 070 356.6 5.0 969.682 72( 8) P(33,10) 1201602 10R(10) 030.5 071 103.2 OMIT 969.707 62(-628) R(37, 4) 1201602 10R(10) 958.3 072 031.0 5.0 969.738 56( ~1) P(36, 7) 1201602 10R(12) 840.2 081 434.2 5.0 970.052 23( 8) P(36, 6) 1201602 108(12) 082.8 087 191.6 5.0 970.244 28( ~15) P(35, 6) 1201602 10R(12) 067.8 107 342.2 5.0 970.916 42( ~6) P(35, 4) 1201602 10R(12) 145.5 111 419.9 5.0 971.052 44( ~4) P(35, 3) 1201602 10R(12) 772.1 112 046.5 5.0 971.073 00( 5) P(34, 8) 1201602 10R(12) 325.7 112 600.1 5.0 971.091 81( 3) P(33, 9) 1201602 10R(12) 756.4 114 030.8 5.0 971.139 53( ~22) P(34, 6) 1201602 lOR(l4) 350.5 127 385.6 5.0 971.585 00( ~10) P(33, 6) 1201602 10R(14) 590.9 147 327.0 5.0 972.250 18( ~2) P(33, 5) 1201602 10R(14) 737.2 149 473.3 5.0 972.321 77( 26) P(33, 4) 1201602 10R(14) 662.6 150 398.8 5.0 972.352 63( ~23) P(32, 8) 1201602 108(14) 727.7 154 463.8 5.0 972.488 23( 0) P(32, 7) 1201602 10R(16) 357.0 163 098.6 5.0 972.776 25( 15) P(32, 6) 1201602 10R(16) 301.0 167 154.7 5.0 972.911 56( ~14) P(32, 5) 1201602 10R(16) 453.9 169 001.8 5.0 972.973 16( ~8) P(32, 4) 1201602 10R(16) 714.9 169 740.8 5.0 972.997 82( ~6) P(31, 5) 1201602 108(16) 9 978.9 188 434.6 5.0 973.621 38( ~3) Table 3~6 (cont’d) 105 Trans.a Laserb v-c v/MHz O-Cd Unc.e v/cm‘.1 f P(30, 8) 1201602 10R(16) 17 464.9 29 195 920.6 0.7 5.0 973.871 08( 2) P(30. 7) 1201602 108(18) ~15 150.1 29 203 280.6 2.1 5.0 974.116 58( 7) P(30, 6) 1201602 10R(18) ~11 945.7 29 206 485.0 ~5.8 5.0 974.223 47( ~19) P(28, 7) 1201602 10R(20) ~14 656.4 29 243 002.1 0.1 5.0 975.441 55( 0) P(28, 3) 1201602 10R(20) ~11 958.0 29 245 700.6 4.0 5.0 975.531 56( 13) P(26, 0) 1201602 10R(22) ~14 206.7 29 281 929.7 ~4.4 5.0 976 740 04( ~15) P(26, 1) ' 1201602 108(22) ~14 084.0 29 282 052.3 ~4.0 5.0 976 744 13( ~14) P(26, 7) 1201602 10R(22) ~13 892.5 29 282 243.8 2.4 5.0 976 750 52( 8) P(26, 2) 1201602 10R(22) ~13 728.0 29 282 408.3 2.0 5.0 976 755 99( 7) P(26, 2) 1201602 10R(22) ~13 728.0 29 282 408.4 2.1 5.0 976 756 00( 7) P(26, 3) 1201602 10R(22) ~13 205.8 29 282 930.6 3.7 5.0 976.773 42( 12) P(26, 4) 1201602 10R(22) ~12 632.3 29 283 504.1 1.0 5.0 976.792 55( 3) P(24, 8) 1201602 108(24) ~16 332.6 29 317 528.6 4.1 5.0 977.927 49( 14) P(24, 0) 1201602 10R(24) ~15 405.9 29 318 455.2 ~1.3 5.0 977.958 39( ~4) P(24. 1) 1201602 10R(24) ~15 254.7 29 318 607.0 0.5 5.0 977.963 46( 2) P(22.10) 1201602 10R(24) ~15 071.8 29 318 789.4 27.1 OMIT 977.969 55( 90) P(24. 2) 1201602 108(24) ~14 818.0 29 319 043.1 0.8 5.0 977.978 01( 3) P(24, 3) 1201602 108(24) ~14 143.3 29 319 717.9 1.7 5.0 978.000 52( 6) P(24, 7) 1201602 10R(24) ~12 883.9 29 320 977.3 3.8 5.0 978 042 53( 13) P(24. 6) 1201602 10R(24) ~12 175.4 29 321 685.8 ~2.3 5.0 978 066 15( ~8) P(22, 0) 1201602 10R(26) ~16 290.8 29 354 533.8 ~11.6 OMIT 979.161 84( ~39) P(22, 1) 1201602 10R(26) ~16 109.7 29 354 719.9 ~1.5 5.0 979.168 05( ~5) P(22, 2) 1201602 108(26) ~15 589.6 29 355 240.0 2.1 5.0 979.185 41( 7) P(22, 3) 1201602 108(26) ~14 771.9 29 356 057.7 1.7 5.0 979.212 67( 6) P(22, 5) 1201602 10R(26) ~12 622.9 29 358 206.7 ~0.5 5.0 979.284 36( ~2) P(19,10) 1201602 10R(26) 15 422.9 29 386 252.5 ~28.8 OMIT 980.219 87( ~96) P(20, 0) 1201602 lOR(28) ~16 845.0 29 390 193.3 ~0.9 5.0 980.351 31( ~3) P(20, 1) 1201602 lOR(28) ~16 643.4 29 390 394.8 0.4 5.0 980.358 05( l) P(20, 2) 1201602 lOR(28) ~16 050.7 29 390 987.5 1.6 5.0 980.377 82( 5) P(20. 3) 1201602 lOR(28) ~15 096.5 29 391 941.8 3.3 5.0 980.409 65( 11) P(20, 4) 1201602 lOR(28) ~13 839.5 29 393 198.7 9.7 5.0 980.451 56( 32) P(20, 5) 1201602 lOR(28) ~12 422.2 29 394 616.1 .~1.3 5.0 980.498 84( ~4) P(20, 7) 1201602 lOR(28) ~10 219.5 29 396 818.7 ~1.3 5.0 980.572 31( ~4) P(19, 8) 1201602 lOR(28) 8 132.9 29 415 171.2 5.7 5.0 981.184 49( 19) P(19, 7) 1201602 lOR(28) 8 386.4 29 415 424.6 ~2.8 5.0 981 192 94( ~9) P(18. 0) 1201602 108(30) ~17 088.7 29 425 394.6 ~2.0 5.0 981 525 51( ~7) P(18, 1) 1201602 10R(30) ~16 867.2 29 425 616.1 ~2.9 5.0 981 532 90( ~10) P(18, 2) 1201602 10R(30) ~16 201.1 29 426 281.8 2.2 5.0 981 555 ll( 7) P(18. 3) 1201602 108(30) ~15 119.7 29 427 363.6 7.7 5.0 981 591 18( 26) P(18, 4) 1201602 10R(30) ~13 678.7 29 428 804.6 3.7 5.0 981 639 26( 12) P(18, 5) 1201602 lOR(30) ~11 960.4 29 430 522.9 ~0.4 5.0 981 696 56( ~1) P(18, 6) 1201602 10R(30) ~10 144.3 29 432 339.0 ~5.3 5.0 981 757 15( ~18) P(18, 7) 1201602 10R(30) -8 599.5 29 433 883.9 ~3.5 5.0 981 808 67( ~12) P(l7, 7) 1201602 10R(30) 9 710.7 29 452 194.0 ~3.0 5.0 982.419 44( ~10) P(16,10) 1201602 10R(30) 11 564.0 29 454 047.4 ~42.3 OMIT 982.481 26(-141) P(16, 0) 1201602 10R(30) 17 661.0 29 460 144.4 ~2.4 5.0 982.684 63( ~8) P(16. 1) 1201602 108(32) ~16 774.0 29 460 386.9 ~2.4 5.0 982.692 72( ~8) P(16, 4) 1201602 10R(32) ~13 251.0 29 463 909.8 ~13.5 10.0 982.810 24( ~45) P(16, 6) 1201602 108(32) ~9 019.6 29 468 141.3 ~6.3 5.0 982.951 38( ~21) P(15, 6) 1201602 10R(32) 8 671.3 29 485 832.1 ~6.2 5.0 983.541 48( ~21) 106 Table 3~6 (cont’d) Trans.a Laserb v-c v/Mflz O—C Unc v/cm-1 f P(15, 8) 1201602 10R(32) 13 251.0 29 490 411.9 ~6.4 20.0 983.694 25( ~21) P(15, 9) 1201602 10R(32) 13 251.0 29 490 411.9 208.7 OMIT 983.694 25( 696} P(14, 0) 1201602 108(32) 17 277.9 29 494 438.6 ~0.8 5.0 983.828 57( ~3) P(14, 1) 1201602 10R(34) ~16 367.6 29 494 699.1 ~0.8 5.0 983.837 26( ~3) P(14, 2) 1201602 10R(34) ~15 593.2 29 495 473.4 ~5.5 5.0 983.863 09( ~18) P(14, 3) 1201602 108(34) ~14 295.4 29 496 771.3 3.1 5.0 983.906 38( 10) P(14, 4) 1201602 10R(34) ~12 516.2 29 498 550.5 2.0 5.0 983.965 73( 7) P(14,10) 1201602 10R(34) ~11 422.7 29 499 644.0 ~19.5 5.0 984.002 20( ~65) P(14, 5) 1201602 108(34) ~10 287.2 29 500 779.5 ~1.3 5.0 984.040 07( ~4) P(13, 6) 1201602 108(34) 9 716.6 29 520 783.3 ~6.3 5.0 984.707 34( ~21) P(l3,10) 1201602 10R(34) 11 588.8 29 522 655.5 1.1 5.0 984.769 78( 4) P(13, 7) 1201602 10R(34) 12 807.3 29 523 874.0 ~3.9 5.0 984.810 42( ~13) P(l3, 8) 1201602 108(34) 15 922.6 29 526 989.3 10.1 OMIT 984.914 35( 34) P(12, 0) 1201602 108(34) 17 201.1 29 528 267.7 ~1.7 5.0 984.956 99( ~6) P(12, 1) 1201602 10R(36) ~15 652.7 29 528 543.6 ~1.9 5.0 984.966 18( ~6) P(12, 2) 1201602 108(36) ~14 822.0 29 529 374.3 0.9 5.0 984.993 90( 3) P(12, 3) 1201602 10R(36) ~13 444.4 29 530 751.9 1.6 5.0 985.039 85( 5) P(12, 5) 1201602 10R(36) ~9 087.5 29 535 108.8 ~4.4 5.0 985.185 19( ~15) P(ll, 6) 1201602 108(36) 10 942.5 29 555 138.8 ~18.6 OMIT 985.853 30( ~62) P(lO, 0) 1201602 108(36) 17 433.5 29 561 630.1 ~2.4 5.0 986.069 83( ~8) P(10, 1) 1201602 108(38) ~14 625.5 29 561 919.7 ~2.2 5.0 986.079 50( ~7) P(10, 2) 1201602 108(38) ~13 754.1 29 562 791.0 0.0 5.0 986.108 56( 0) R(10, 4) 1201602 10R(38) ~10 265.9 29 566 279.2 0.1 5.0 986.224 91( 0) R( 3, 1) 1301602 9P(28) 11 473.0 29 782 141.2 ~0.9 10.0 993.425 29( ~3) R( 5, 1) 1301602 9P(26) ~17 264.2 29 811 661.3 ~2.5 10.0 994.409 98( ~8) R( 5, 2) 1301602 9P(26) ~16 353.0 29 812 572.5 -2.8 10.0 994.440 38( ~9) R( 5, 4) 1301602 9P(26) ~12 653.6 29 816 271.9 7.0 20.0 994.563 77( 23) R( 7, 0) 1301602 9P(26) 11 476.3 29 840 401.9 ~5.1 5.0 995.368 66( ~17) R( 7, 1) 1301602 9P(26) 11 770.9 29 840 696.4 ~3.4 5.0 995.378 49( ~11) R( 7, 2) 1301602 9P(26) 12 653.6 29 841 579.1 -l.0 20.0 995.407 92( ~3) R( 7, 3) 1301602 9P(26) 14 127.1 29 843 052.6 0.1 5.0 995.457 08( 0) R( 7. 4) 1301602 9P(26) 16 201.4 29 845 127.0 2.2 20.0 995.526 28( 7) R( 9, 0) 1301602 9P(24) ~17 377.5 29 868 967.0 ~3.8 5.0 996.321 50( ~13) R( 9, 1) 1301602 9P(24) ~17 105.1 29 869 239.4 ~ll.8 30.0 996.330 58( ~39) R( 9, 2) 1301602 9P(24) ~16 249.5 29 870 095.0 2.6 20.0 996.359 11( 9) R( 9, 3) 1301602 9P(24) ~14 849.0 29 871 495.5 0.8 10.0 996.405 84( 3) R( 9, 4) 1301602 9P(24) ~12 889.4 29 873 455.2 ~1.0 10.0 996.471 19( ~3) R( 9, 5) 1301602 9P(24) ~10 380.1 29 875 964.5 ~5.8 10.0 996.554 90( ~19) R(10, 7) 1301602 9P(24) 9 719.0 29 896 063.5 9.2 20.0 997.225 33( 31) R(11, 0) 1301602 9P(24) 10 709.4 29 897 053.9 ~0.0 10.0 997.258 37( 0) R(ll, 1) 1301602 9P(24) 10 973.0 29 897 317.5 ~1.8 5.0 997.267 16( ~6) R(ll, 2) 1301602 9P(24) 11 770.8 29 898 115.3 1.3 5.0 997.293 77( 4) R(10, 8) 1301602 9P(24) 13 089.1 29 899 433.6 ~137.4 OMIT 997.337 75(-525) R(11, 3) 1301602 9P(24) 13 089.1 29 899 433.6 1.1 20.0 997.337 75( 4) R(11, 4) 1301602 9P(24) 14 918.9 29 901 263.4 1.4 10.0 997.398 78( 5) R(1l, 5) 1301602 9P(24) 17 229.2 29 903 573.7 ~1.4 5.0 997.475 85( ~5) R(13, 2) 1301602 9P(22) ~17 273.8 29 925 646.9 ~0.2 5.0 998.212 13( ~1) R(13, 3) 1301602 9P(22) ~16 043.1 29 926 877.6 8.7 5.0 998.253 19( 29) R(13, 4) 1301602 9P(22) ~14 374.0 29 928 546.8 0.5 5.0 998.308 85( 2) R(13, 5) 1301602 9P(22) ~12 290.6 29 930 630.1 2.1 5.0 998.378 36( 7) Table 3~6 (cont’d) 107 Trans.a Laserb one v/Mflz O-Cd Unc e 12/cm-1 f R(13, 6) 1301602 9P(22) ~9 917.0 29 933 003.8 ~8.1 5.0 998.457 53( ~27) R(15, 0) 1301602 9P(22) 8 864.7 29 951 785.4 ~l.l 5.0 999.084 02( ~4) R(15, 1) 1301602 9P(22) 9 093.6 29 952 014.3 ~0.6 5.0 999.091 64( ~2) R(15, 2) 1301602 9P(22) 9 774.0 29 952 694.8 ~0.1 10.0 999.114 34( 0) R(15, 3) 1301602 9P(22) 10 890.8 29 953 811.6 4.0 5.0 999.151 61( 13) R(15, 4) 1301602 9P(22) 12 393.2 29 955 314.0 0.5 5.0 999.201 72( 2) R(15, 5) 1301602 9P(22) 14 214.6 29 957 135.3 ~0.0 5.0 999.262 47( 0) R(15, 6) 1301602 9P(22) 16 195.5 29 959 116.3 ~4.7 5.0 999.328 54( ~16) R(17, 4) 1301602 9P(20) ~17 080.8 29 981 569.3 0.4 5.0 1000.077 49( 1) R(17, 5) 1301602 9P(20) ~15 546.2 29 983 103.9 ~0.6 5.0 1000.128 69( ~2) R(17, 6) 1301602 9P(20) ~13 999.3 29 984 650.8 ~2.9 5.0 1000.180 29( ~10) R(17, 8) 1301602 9P(20) ~13 193.0 29 985 457.1 3.8 5.0 1000.207 18( 13) R(17, 7) 1301602 9P(20) ~12 869.1 29 985 780.9 ~4.2 5.0 1000.217 98( ~14) R(19, 4) 1301602 9P(20) 8 672.2 30 007 322.3 4.0 5.0 1000.936 52( 13) R(19, 8) 1301602 9P(20) 9 777.0 30 008 427.1 5.2 5.0 1000.973 38( 17) R(19, 5) 1301602 9P(20) 9 894.8 30 008 544.9 1.5 5.0 1000.977 30( 5) R(19, 6) 1301602 9P(20) 10 972.0 30 009 622.1 ~0.1 5.0 1001.013 23( 0) R(19, 7) 1301602 9P(20) 11 363.2 30 010 013.3 1.5 5.0 1001.026 29( 5) R(20, 9) 1301602 9P(20) 12 280.8 30 010 930.9 ~188.9 OMIT 1001.056 90(-630) R(22, 8) 1301602 9P(18) ~11 813.1 30 041 715.6 ~0.1 5.0 1002.083 76( 0) R(22, 0) 1301602 9P(18) ~10 504.2 30 043 024.5 ~6.1 5.0 1002.127 43( ~21) R(22, 1) 1301602 9P(18) ~10 355.1 30 043 173.7 ~1.0 5.0 1002.132 39( ~3) R(22, 4) 1301602 9P(18) ~8 519.7 30 045 009.1 1.0 5.0 1002.193 62( 3) R(22, 7) 1301602 9P(18) ~8 275.9 30 045 252.9 ~0.3 5.0 1002.201 76( ~1) R(24, 8) 1301602 9P(18) 9 666.5 30 063 195.3 2.4 10.0 1002.800 25( 8) R(24, 7) 1301602 9P(18) 14 530.0 30 068 058.7 12.5 10.0 1002.962 48( 42) R(24, 0) 1301602 9P(18) 14 530.0 30 068 058.7 0.6 10.0 1002.962 48( 2) R(24, 1) 1301602 9P(18) 14 644.2 30 068 172.9 ~0.9 5.0 1002.966 28( ~3) R(24. 2) 1301602 9P(18) 14 976.3 30 068 505.1 1.1 5.0 1002.977 36( 4) R(24, 3) 1301602 9P(18) 15 467.2 30 068 995.9 4.4 5.0 1002.993 74( 15) R(26, 9) 1301602 9P(18) 15 617.5 30 069 146.2 46.3 OMIT 1002.998 75( 154) R(24, 4) 1301602 9P(18) 15 995.6 30 069 524.4 2.6 5.0 1003.011 37( 9) R(24, 6) 1301602 9P(18) 16 131.0 30 069 659.7 ~0.8 5.0 1003.015 88( ~3) R(24, 5) 1301602 9P(18) 16 347.7 30 069 876.5 ~3.5 5.0 1003.023 10( ~12) R(26, 7) 1301602 9P(16) ~17 248.7 30 090 304.4 1.0 5.0 1003.704 52( 3) R(26, 0) 1301602 9P(16) ~14 927.1 30 092 626.0 ~4.4 5.0 1003.781 96( ~15) R(26, 2) 1301602 9P(16) ~14 597.8 30 092 955.3 1.0 5.0 1003.792 94( 3) R(26, 4) 1301602 9P(16) ~14 007.6 30 093 545.5 -8.8 5.0 1003.812 63( ~29) R(26, 5) 1301602 9P(16) ~14 007.6 30 093 545.5 9.9 5.0 1003.812 63( 33) R(27, 8) 1301602 9P(16) ~13 138.4 30 094 414.7 ~2.0 5.0 1003.841 62( ~7) R(29, 9) 1301602 9P(16) ~10 845.5 30 096 707.6 0.3 5.0 1003.918 09( l) R(28, 2) 1301602 9P(16) 9 396.3 30 116 949.4 0.3 5.0 1004.593 29( l) R(ZB, 3) 1301602 9P(16) 9 555.6 30 117 108.7 7.1 5.0 1004.598 61( 24) R(28, 4) 1301602 9P(16) 9 555.6 30 117 108.7 ~4.5 5.0 1004.598 61( ~15) R(30, 8) 1301602 9P(16) 16 990.6 30 124 543.7 ~2.2 5.0 1004.846 62( ~7) R(31, 7) 1301602 9P(14) ~16 976.5 30 143 743.4 3.1 10.0 1005.487 04( 10) R(32, 8) 1301602 9P(14) ~16 650.7 30 144 069.2 ~2.8 5.0 1005.497 92( ~9) R(31, 5) 1301602 9P(14) ~10 155.6 30 150 564.3 ~2.6 5.0 1005.714 56( ~9) R(3l. 4) 1301602 9P(14) ~9 138.2 30 151 581.7 ~0.3 5.0 1005.748 51( ~1) R(31, 3) 1301602 9P(14) ~8 734.8 30 151 985.1 1.6 5.0 1005.761 96( 5) Table 3~6 (cont’d) 108 Trans.’ Laserb v: v/MHz o—cd Unc.e v/cm 1 f R(31, 0) 1301602 9P(14) -8 618.4 30 152 101.5 -2.1 30.0 1005.765 84( ~7) R(31, 2) 1301602 99(14) ~8 618.4 30 152 101.5 2.0 30.0 1005.765 84( 7) R(3l, 1) 1301602 9P(14) -8 618.4 30 152 101.5 -8.0 30.0 1005.765 84( —27) R(33, 4) 13c1602 9P(14) 13 275.7 30 173 995.6 1.9 5.0 1006.496 14( 6) R(34, 7) 1301602 9P(14) 13 675.0 30 174 394.9 3.9 5.0 1006.509 46( 13) R(33, 3) 1301602 9P(14) 13 962.0 30 174 681.9 2.3 5.0 1006.519 04( 8) R(33, 0) 1301602 99(14) 14 383.5 30 175 103.4 -20.8 15.0 1006.533 10( ~69) R(33, 1) 1301602 9P(14) 14 383.5 30 175 103.4 7.4 15.0 1006.533 10( 25) R(35, 4) 1301602 99(12) -17 065.6 30 195 960.5 -1.1 5.0 1007.228 82( -4) R(35, 2) 1301602 9P(12) -15 590.9 30 197 435.3 6.6 20.0 1007.278 01( 22) R(35, 1) 1301602 9P(12) -15 376.3 30 197 649.9 -1.4 10.0 1007.285 l7( -5) R(35, 0) 1301602 9P(12) -15 314.5 30 197 711.6 —2.7 10.0 1007.287 23( —9) R(38, 8) 1301602 9P(12) -12 788.1 30 200 238.0 0.4 5.0 1007.371 50( 1) R(36, 6) 1301602 9P(12) -12 027.5 30 200 998.7 -2.4 5.0 1007.396 88( ~8) R(38, 5) 1301602 99(12) 12 587.3 30 225 613.4 -2.5 5.0 1008.217 93( ~8) R(38, 3) 1301602 9P(12) 16 494.9 30 229 521.1 2.4 5.0 1008.348 28( 8) R(38, 2) 1301602 99(12) 17 276.7 30 230 302.9 2.0 5.0 1008.374 36( 7) R(38, 1) 1301602 99(12) 17 679.5 30 230 705.6 16.8 0M T 1008.387 79( 56) R(38, 0) 1301602 9P(12) 17 780.7 30 230 806.8 1.2 5.0 1008.391 16( 4) R(40, 4) 1301602 9P(10) -15 472.8 30 248 996.3 -1.5 5.0 1008.997 91( -5) R(40, 3) 1301602 9P(10) —13 751.7 30 250 717.4 3.6 5.0 1009.055 32( 12) R(4l, 6) 1301602 9P(10) -13 507.3 30 250 961.8 —4.1 5.0 1009.063 47( -14) R(40, 1) 1301602 99(10) -12 276.1 30 252 193.0 -0.3 5.0 1009.104 54( -1) R(40, 0) 1301602 9P(10) -12 123.6 30 252 345.4 —1.1 5.0 1009.109 61( -4) R(46, 6) 1301602 9P( 8) ~16 605.6 30 298 440.7 2.0 10.0 1010.647 19( 7) R(45, 1) 1301602 99( 8) -10 871.0 30 304 175.2 ~6.3 10.0 1010.838 48( -21) R(45, 0) 1301602 9P( 8) -10 626.9 30 304 419.4 ~8.3 10.0 1010.846 62( ~28) R(46, 5) 1301602 9P( 8) -9 970.4 30 305 075.9 -0.3 5.0 1010.868 51( -1) R(47. 2) 1301602 9P( 8) 8 340.0 30 323 386.2 0.2 5.0 1011.479 28( 1) R(48, 5) 1301602 9P( 8) 8 917.2 30 323 963.5 -1.4 10.0 1011.498 55( -5) R(47, 1) 1301602 9P( 8) 9 239.5 30 324 285.8 ~0.6 5.0 1011.509 30( -2) R(47, 0) 1301602 99( 8) 9 522.3 30 324 568.6 —1.4 5.0 1011.518 73( —5) R(48, 4) 1301602 9P( 8) 13 507.2 30 328 553.5 1.8 5.0 1011.651 65( 6) R(48, 3) 1301602 9P( 8) 16 417.4 30 331 463.7 3.1 5.0 1011.748 72( 10) aNumbers are J and E of b Laser line used; laser the lower vibrational state. frequencies were taken from Ref. 13. cMicrowave frequency in MHz. The signed microwave frequency was added to the laser frequency to obtain the absorption frequency. d eEstimated uncertainty in the observed frequency in MHz. An ”OMIT” means that the frequency was omitted from the least squares fits. fObserved wavenumber in cm-l. The numbers in parentg minus calculated wavenumbers in units of 0.00001 cm Tses are observed Observed minus calculated frequency in MHz; the parameters for the calculation are in Table 3~8 of this work and in Table V of Ref. 7. 109 TABLE 3-7 Comparison of Observed and Calculated Frequencies in the v2 Band of 003813r Trans.a Laserb vnc v/MHz O-Cd Unc. v/cm 1 f P(45, 6) 1201602 lOR( 4) -17 835.0 28 905 211.4 9.4 5.0 964.174 07( 31) P(45, 5) 12C1602 lOR( 4) -12 239.5 28 910 807.0 -6.2 5.0 964.360 72( -21) P(45, 4) 12C1602 10R( 4) -8 825.6 28 914 220.8 -0.6 5.0 964.474 59( -2) P(44. 5) 1201602 lOR( 4) 8 365.5 28 931 411.9 -4.9 10.0 965.048 01( -16) P(44. 4) 12C1602 lOR( 4) 11 571.6 28 934 618.1 1.1 5.0 965.154 97( 4) P(44, 3) 12C1602 lOR( 4) 13 485.0 28 936 531.4 1.0 5.0 965.218 79( 3) P(44. 2) 12C1602 lOR( 4) 14 588.7 28 937 635.1 -l.9 5.0 965.255 61( -6) P(44, l) 12C1602 lOR( 4) 15 162.4 28 938 208.8 0.2 5.0 965.274 73( l) P(43, 7) 1201602 lOR( 4) 15 282.0 28 938 328.4 -2.7 5.0 965.278 72( -9) P(44. 0) 12C1602 lOR( 4) 15 336.6 28 938 383.1 -1.8 5.0 965.280 56( -6) P(39,10) 12C1602 lOR( 4) 16 336.2 28 939 382.7 374.0 OMIT 965.313 89(1248) P(43, 5) 12C1602 lOR( 6) -15 531.4 28 951 925.7 -6.9 10.0 965.732 29( -23) P(43, 3) 12C1602 lOR( 6) -10 765.0 28 956 692.1 1.8 10.0 965.891 28( 6) P(43, 2) 12C1602 lOR( 6) -9 756.6 28 957 700.4 1.4 10.0 965.924 90( 5) P(43, l) 12C1602 lOR( 6) -9 243.8 28 958 213.3 -1.4 10.0 965.942 01( -5) P(42, 3) 12C1602 lOR( 6) 9 305.8 28 976 762.8 2.2 10.0 966.560 77( 7) P(42, 2) 1261602 lOR( 6) 10 217.4 28 977 674.4 2.6 5.0 966.591 17( 9) P(42, l) 12C1602 lOR( 6) 10 676.6 28 978 133.7 2.0 5.0 966.606 49( 7) P(42. 0) 12C1602 lOR( 6) 10 814.4 28 978 271.5 -0.1 20.0 966.611 08( 0) P(39, 9) 1201602 lOR( 6) 17 944.3 28 985 401.3 -68.1 OMIT 966.848 92(-227) P(41, 4) 1201602 10R( 8) -15 867.4 28 995 265.6 -2.0 5.0 967.177 95( -7) P(4l. 3) 12C1602 lOR( 8) -14 392.1 28 996 740.9 0.8 5.0 967.227 16( 3) P(4l, 2) 1201602 lOR( 8) -13 577.9 28 997 555.1 0.9 5.0 967.254 32( 3) P(41, l) 12C1602 lOR( 8) -13 175.0 28 997 958.0 -0.6 5.0 967.267 75( -2) P(4l. 0) 12C1602 10R( 8) -13 052.4 28 998 080.6 0.1 5.0 967.271 84( 0) P(40, 7) 12C1602 lOR( 8) -9 726.2 29 001 406.8 1.0 5.0 967.382 79( 3) P(39, 7) 12C1602 lOR( 8) 11 122.1 29 022 255.1 -0.8 5.0 968.078 22( -3) P(39, 3) 12C1602 lOR(lO) -17 650.7 29 036 422.0 0.6 5.0 968.550 78( 2) P(39, 2) 1201602 lOR(lO) -17 030.5 29 037 042.2 -0.7 5.0 968.571 46( -2) P(38, 7) 12C1602 108(10) -11 059.2 29 043 013.5 -l.4 5.0 968.770 65( -5) P(37, 7) 1201602 lOR(IO) 9 608.9 29 063 681.6 1.2 5.0 969 460 05( 4) P(37, 6) 12C1602 108(10) 15 733.9 29 069 806.6 ~5.l 5.0 969 664 36( -l7) P(36, 7) 12C1602 108(12) -12 024.4 29 084 250.0 0.4 5.0 970 146 15( 1) P(35, 7) 1261602 108(12) 8 448.9 29 104 723.3 2.8 5.0 970 829 07( 9) P(35, 5) 12C1602 108(12) 16 430.7 29 112 705.1 -l.0 5.0 971 095 31( -3) P(35, 4) 1201602 108(12) 17 756.4 29 114 030.8 -1.5 5.0 971 139 53( -5) P(34, 7) 1201602 10R(14) -12 661.9 29 125 074.3 -16.0 OMIT 971 507 89( -53) P(33, 6) 12C1602 108(14) 12 065.4 29 149 801.5 -0.4 5.0 972.332 71( ~1) P(33, 5) 1201602 108(14) 14 168.3 29 151 904.4 -4.9 5.0 972.402 86( -16) P(33, 4) 1201602 108(14) 15 092.3 29 152 828.4 -0.2 5.0 972.433 67( -l) P(32, 7) 1201602 108(16) -12 987.8 29 165 517.9 1.9 5.0 972.856 95( 6) P(31. 6) 1201602 108(16) 10 706.9 29 189 162.6 -0.3 5.0 973.645 66( -l) P(3l, 5) 1201602 108(16) 12 234.5 29 190 690.1 -0.7 5.0 973.696 60( ~2) P(29, 9) 1201602 108(18) -15 798.2 29 202 632.5 -228.0 OMIT 974 094 96(-760) P(30. 7) 1201602 108(18) -12 922.0 29 205 508.7 3.5 5.0 974 190 91( 12) P(28, 3) 1201602 108(20) -10 010.6 29 247 648.0 -0.9 5.0 975 596 52( -3) P(27, 2) 1201602 108(20) 8 125.6 29 265 784.1 3.1 5.0 976 201 47( 10) P(27, 3) 1201602 108(20) 8 566.9 29 266 225.4 -4.0 5.0 976 216 19( -l3) P(27. 6) 1201602 108(20) 8 876.0 29 266 535.1 0.5 5.0 976 226 53( 2) P(27, 4) 1201602 108(20) 9 033.0 29 266 691.5 0.2 5.0 976 231 75( l) 110 Table 3-7 (cont’d) Trans.a Laserb vlc v/Mflz 0-6d Uhc. v/cm l f P(26. 8) 1261602 108(22) -16 756.9 29 279 379.5 -3.9 5.0 976.654 97( -13) P(26, 3) 1261602 10R(22) ~11 433.9 29 284 702.5 1.0 5.0 976.832 53( 3) P(26, 4) 1261602 108(22) -10 849.5 29 285 286.9 0.5 5.0 976.852 02( 2) P(25, 9) 1261602 108(22) -8 706.5 29 287 429.9 -229.0 OMIT 976.923 49(-764) P(24, 3) 1261602 108(24) -12 545.4 29 321 320.8 5.1 5.0 978 053 98( 17) P(24, 4) 1261602 108(24) -11 723.6 29 322 137.6 0.1 5.0 978 081 23( 0) P(24, 7) 1261602 108(24) -11 228.8 29 322 632.4 3.0 5.0 978 097 72( 10) P(24, 5) 1261602 108(24) -10 940.9 29 322 920.2 0.9 5.0 978 107 34( 3) P(24, 6) 1261602 108(24) -10 544.5 29 323 316.7 -0.5 5.0 978 120 55( -2) P(22. 9) 1261602 108(24) 16 078.7 29 349 939.9 -226.3 OMIT 979 008 60(-755) P(22, 2) 1261602 108(26) -14 170.6 29 356 659.0 -1.2 5.0 979.232 74( -4) P(22, 3) 1261602 108(26) -13 345.8 29 357 483.8 0.5 5.0 979.260 25( 2) P(22, 4) 1261602 108(26) -12 296.2 29 358 533.4 4.8 5.0 979.295 25( 16) P(22, 5) 1261602 108(26) -11 183.8 29 359 645.8 0.0 5.0 979.332 36( 0) P(21. 6) 1261602 108(26) 8 143.5 29 378 973.2 2.4 5.0 979.977 06( 8) P(21, 7) 1261602 10R(26) 8 623.0 29 379 452.6 4.6 5.0 979.993 05( 15) P(20, 9) 1261602 lOR(28) -16 050.7 29 390 987.5 -228.7 OMIT 980.377 82(-763) P(20, 0) 1261602 lOR(28) -15 595.8 29 391 442.5 -1.2 5.0 980.392 99( -4) P(20. 1) 1261602 lOR(28) -15 393.5 29 391 644.7 -0.4 5.0 980.399 73( ~1) P(20. 2) 1261602 lOR(28) -14 798.2 29 392 240.0 0.0 5.0 980.419 59( 0) P(20, 3) 1261602 lOR(28) -13 839.5 29 393 198.7 2.2 5.0 980.451 56( 7) P(20, 4) 1261602 lOR(28) -12 587.1 29 394 451.2 0.5 5.0 980.493 34( 2) P(20, 6) 1261602 lOR(28) -9 773.0 29 397 265.2 3.4 5.0 980.587 22( ll) P(20, 8) 1261602 lOR(28) -9 773.0 29 397 265.2 -4.5 5.0 980.587 22( -15) P(20, 7) 1261602 lOR(28) -8 926.7 29 398 111.6 1.9 5.0 980.615 45( 6) P(19, 8) 1261602 lOR(28) 9 362.8 29 416 401.1 ~4.0 5.0 981.225 51( -l3) P(18. 0) 1261602 108(30) -16 002.1 29 426 481.3 -0.1 5.0 981 561 76( 0) P(18. 1) 1261602 108(30) -15 776.9 29 426 706.4 1.5 5.0 981 569 26( 5) P(18, 2) 1261602 108(30) -15 119.7 29 427 363.6 -4.8 5.0 981 591 18( -16) P(18. 3) 1261602 108(30) -14 032.8 29 428 450.5 2.7 5.0 981 627 44( 9) P(18. 4) 1261602 108(30) -12 585.1 29 429 898.3 .3.4 5.0 981.675 74( 11) P(18, 5) 1261602 108(30) -10 865.6 29 431 617.8 -0.6 5.0 981.733 08( -2) P(18, 9) 1261602 108(30) -10 865.2 29 431 618.1 -73.1 OMIT 981 733 11(-244) P(18, 6) 1261602 108(30) -9 041.3 29 433 442.0 -0.6 5.0 981.793 94( -2) P(l7, 8) 1261602 108(30) 11 705.3 29 454 188.6 -2.9 5.0 982.485 98( -10) P(16, 1) 1261602 108(32) -15 846.0 29 461 314.9 1.3 5.0 982.723 67( 4) P(16, 2) 1261602 108(32) -15 121.4 29 462 039.5 0.2 5.0 982.747 84( 1) P(16. 3) 1261602 108(32) -13 929.3 29 463 231.1 0.8 5.0 982.787 59( 3) P(16. 4) 1261602 108(32) ~12 314.9 29 464 845.9 —7.0 5.0 982.841 46( -23) P(16, 5) 1261602 108(32) -10 317.3 29 466 843.5 0.8 5.0 982.908 09( 3) P(15, 6) 1261602 108(32) 9 524.9 29 486 685.7 2.4 5.0 983.569 96( 8) P(15, 7) 1261602 108(32) 12 043.8 29 489 204.6 -1.5 5.0 983.653 99( ~5) P(15, 8) 1261602 108(32) 14 135.5 29 491 296.3 -2.2 5.0 983.723 75( —7) P(15, 9) 1261602 108(32) 14 381.0 29 491 541.9 390.9 OMIT 983.731 94(1304) P(14, 0) 1261602 108(34) -15 861.5 29 495 205.1 1.0 5.0 983.854 14( 3) P(14, 1) 1261602 108(34) -15 593.2 29 495 473.4 7.9 5.0 983.863 09( 26) P(14, 2) 1261602 108(34) -14 817.9 29 496 248.8 2.1 5.0 983.888 95( 7) P(14, 3) 1261602 108(34) -13 523.1 29 497 543.5 6.1 5.0 983.932 14( 20) P(14, 4) 1261602 108(34) -11 750.1 29 499 316.6 -0.5 5.0 983.991 27( -2) P(14, 5) 1261602 108(34) -9 521.6 29 501 545.1 -l.0 5.0 984.065 61( ~3) 11.1 Table 3-7 (cont’d) Trans.a Laserb vnc v/Mflz O—Cd Unc v/c:m"l f P(13, 7) 12C1602 108(34) 13 523.1 29 524 589.8 28.0 OMIT 984.834 30( 94) P(12, 0) 12C1602 10R(36) ‘15 318.3 29 528 878.0 ‘1.1 5.0 984.977 35( ‘4) P(13, 9) 12C1602 108(36) ‘14 345.5 29 529 850.8 28.7 OMIT 985.009 80( 96) P(12, 2) 12C1602 108(36) ‘14 210.0 29 529 986.4 0.8 5.0 985.014 31( 3) P(12, 3) 12C1602 108(36) ‘12 833.6 29 531 362.7 ‘0.7 5.0 985.060 23( ‘2) P(12, 4) 12C1602 108(36) ‘10 942.5 29 533 253.9 ‘26.5 OMIT 985.123 30( ‘88) P(ll, 7) 12C1602 108(36) 15 071.5 29 559 267.9 ‘0.7 5.0 985.991 03( ‘2) P(10, 0) 12C1602 108(38) ‘14 455.2 29 562 089.9 ‘0.5 5.0 986.085 18( ‘2) P(10, 1) 12C1602 108(38) ‘14 156.9 29 562 388.2 7.7 5.0 986.095 13( 26) P(10, 2) 12C1602 108(38) ‘13 295.6 29 563 249.5 ‘1.5 5.0 986.123 86( ‘5) P(10, 3) 12C1602 108(38) ‘11 843.0 29 564 702.2 ‘0.5 5.0 986.172 31( ‘2) P(10, 4) 12C1602 108(38) ‘9 808.9 29 566 736.2 ‘0.2 5.0 986.240 15( ‘1) R( 3, 0) 13C1602 9P(28) 10 663.5 29 781 331.7 7.4 10.0 993.398 29( 25) R( 3, 1) 13C1602 9P(28) 10 965.2 29 781 633.4 ‘1.9 10.0 993.408 36( ‘6) R( 7, 0) 13C1602 9P(26) 10 729.8 29 839 655.3 ‘0.2 5.0 995.343 75( ‘1) R( 7, 1) 13C1602 9P(26) 11 022.5 29 839 948.0 ‘1.2 5.0 995.353 52( ‘4) R( 7, 2) 13C1602 9P(26) 11 903.5 29 840 829.1 ‘1.9 5.0 995.382 91( ‘6) R( 7, 3) 13C1602 9P(26) 13 378.7 29 842 304.3 0.6 5.0 995.432 12( 2) R( 9, 1) 13C1602 9P(24) ‘17 961.6 29 868 382.9 ‘0.8 5.0 996.302 00( ‘3) R( 9, 2) 13C1602 9P(24) ‘17 105.1 29 869 239.4 12.7 OMIT 996.330 58( 42) R( 9, 3) 13C1602 9P(24) ‘15 717.3 29 870 627.2 ‘2.7 5.0 996.376 87( ‘9) R( 9, 4) 13C1602 99(24) ‘13 757.9 29 872 586.6 ‘2.6 5.0 996.442 22( ‘9) R(10, 7) 13C1602 9P(24) 8 775.9 29 895 120.4 ‘0.7 5.0 997.193 88( ‘2) R(11, 0) 13C1602 9P(24) 9 719.0 29 896 063.5 ‘8.7 5.0 997.225 33( ‘29) R(11, 1) 13C1602 9P(24) 9 991.2 29 896 335.7 ‘2.8 5.0 997.234 42( ‘9) R(11, 3) 13C1602 9P(24) 12 089.1 29 898 433.6 ‘21.8 OMIT 997.304 39( ‘73) R(11, 4) 1301602 9P(24) 13 937.8 29 900 282.3 ‘1.6 5.0 997.366 05( ‘5) R(13, 4) 13C1602 9P(22) ‘15 470.0 29 927 450.8 ‘9.8 5.0 998 272 29( ‘33) R(13, 5) 13C1602 9P(22) ‘13 381.3 29 929 539.4 ‘0.9 10.0 998 341 96( ‘3) R(13, 6) 13C1602 9P(22) ‘10 998.9 29 931 921.9 ‘0.7 5.0 998 421 43( ‘2) R(15, 3) 13C1602 9P(22) 9 693.5 29 952 614.2 ‘1.9 10.0 999.111 67( ‘6) R(15, 4) 13C1602 9P(22) 11 203.2 29 954 124.0 0.2 5.0 999.162 02( 1) R(15, 5) 13C1602 9P(22) 13 023.3 29 955 944.0 ‘1.8 5.0 999.222 74( ‘6) R(15, 6) 13C1602 9P(22) 15 013.9 29 957 934.6 1.8 5.0 999.289 13( 6) R(17, 5) 13C1602 9P(20) ‘16 836.1 29 981 814.0 ‘2.7 5.0 1000.085 65( ‘9) R(17, 6) 13C1602 99(20) ‘15 277.4 29 983 372.7 2.2 5.0 1000 137 65( 7) R(17, 8) 13C1602 9P(20) ‘14 434.2 29 984 215.9 ‘5.5 5.0 1000 165 78( ‘18) R(17, 7) 13C1602 9P(20) ‘14 130.0 29 984 520.1 3.8 5.0 1000 175 92( 13) R(18. 1) 13C1602 9P(20) ‘8 220.0 29 990 430.1 ‘5.4 5.0 1000 373 06( ‘18) R(Zo, 0) 13C1602 9P(20) 17 434.5 30 016 084.6 ‘6.5 5.0 1001 228 80( ‘22) R(ZO, 1) 13C1602 9P(20) 17 614.8 30 016 264.9 1.8 5.0 1001 234 82( 6) R(22. 0) 13C1602 9P(18) ‘12 048.4 30 041 480.7 ‘1.5 5.0 1002 075 92( ‘5) R(22, 2) 13C1602 9P(18) ‘11 476.5 30 042 052.2 2.0 5.0 1002 095 00( 7) R(22, 3) 13C1602 9P(18) ‘10 829.5 30 042 699.3 ‘1.1 5.0 1002 116 57( ‘4) R(24, 2) 1301602 9P(18) 13 341.8 30 066 870.5 0.8 5.0 1002 922 85( 3) R(24, 3) 13C1602 9P(18) 13 839.5 30 067 368.2 3.1 5.0 1002 939 44( 10) R(24, 4) 13C1602 99(18) 14 374.9 30 067 903.6 ‘1.1 5.0 1002 957 31( ‘4) R(26, 0) 13C1602 9P(16) ‘16 656.4 30 090 896.6 ‘2.1 5.0 1003 724 27( ‘7) R(26, 1) 13C1602 9P(16) ‘16 566.2 30 090 986.9 0.1 5.0 1003.727 27( 0) R(26, 6) 13C1602 9P(16) ‘16 458.0 30 091 095.0 4.6 5.0 1003.730 89( 15) 112 Table 3-7 (cont’d) Trans. Laserb v/Mfiz v/cn 1 f R(26, 1301602 9P(16) ‘16 .0 30 091 233.1 .4 5.0 1003.735 49( 8) R(26, 13C1602 9P(16) ‘15 .7 30 091 562.4 .9 5.0 1003.746 48( ‘3) R(26, 1301602 9P(16) ‘15 .9 30 091 850.2 .4 10.0 1003.756 07( -1) R(26, 13C1602 9P(16) -15 .9 30 091 850.2 .9 10.0 1003.756 07( 13) R(29, 1301602 9P(16) 13 .1 30 120 995.2 .2 5.0 1004.728 25( 27) R(30, 1301602 9P(16) 15 .6 30 122 732.7 .4 OMIT 1004.786 20(-318) R(29, 1301602 9P(16) 17 .3 30 124 687.4 .7 5.0 1004.851 40( 6) R(31, 13C1602 9P(14) -l4 .0 30 146 475.9 .9 5.0 1005.578 18( ‘20) R(31, 1301602 9P(14) ‘12 .9 30 148 677.0 .8 5.0 1005.651 61( ‘13) R(31, 1301602 9P(14) ‘11 .8 30 149 674.1 .5 5.0 1005.684 88( ‘2) R(31, 1301602 9P(14) ‘10 .0 30 150 058.9 .6 5.0 1005.697 71( ‘5) R(31. 13C1602 9P(14) ‘10 .2 30 150 165.7 .9 10.0 1005.701 27( 3) R(3l, 13C1602 9P(14) ‘10 .2 30 150 165.7 .9 10.0 1005.701 27( ‘6) R(31, 1301602 9P(14) -10 .2 30 150 165.7 .5 10.0 1005.701 27( 22) R(33, 1301602 9P(14) ‘8 .1 30 151 863.8 .9 5.0 1005.757 92( 10) R(33, 1301602 9P(14) 9 .2 30 170 604.1 .4 5.0 1006.383 02( ‘1) R(35, 13C1602 9P(14) 9 .2 30 170 604.1 .5 OMIT 1006.383 02(-342) R(33, 13C1602 9P(14) 11 .3 30 172 011.2 .4 10.0 1006.429 96( 5) R(34. 13C1602 9P(14) 11 .4 30 172 483.3 .9 5.0 1006.445 70( 16) R(33, 1301602 9P(14) 12 .4 30 172 967.3 .2 5.0 1006.461 85( 1) R(34, 13C1602 9P(14) l7 .5 30 178 311.4 .1 .0 1006.640 12( 4) R(35, 13C1602 9P(12) ‘17 .9 30 195 553.2 .9 .0 1007 215 23( 3) R(35, 13C1602 9P(12) ‘17 .8 30 195 612.3 .3 .0 1007 217 21( ‘1) R(36, 13C1602 9P(12) ‘10 .5 30 202 652.7 .8 .0 1007 452 04( -9) R(38. 13C1602 9P(12) 10 .7 30 223 478.9 .4 .0 1008 146 74( ‘11) R(38. 1301602 9P(12) 12 .2 30 225 945.4 .5 .0 1008 229 01( 28) R(38, 13C1602 9P(12) 15 .6 30 228 102.7 .2 .0 1008 300 97( 7) R(38, 13C1602 9P(12) 15 .1 30 228 480.2 .5 .0 1008 313 56( 2) R(38, 13C1602 9P(12) 15 .9 30 228 617.0 .4 IT 1008 318 12( 78) R(40, 13C1602 9P(10) -17 .0 30 246 766.1 .5 .0 1008 923 52( ‘2) R(40. 13C1602 9P(10) ‘16 .0 30 248 461.0 .7 .0 1008.980 05( 6) R(41, 13C1602 9P(10) -15 .l 30 248 773.9 .9 .0 1008.990 49( ‘23) R(40, 13C1602 9P(10) -14 .0 30 249 914.1 .1 .0 1009 028 51( 0) R(41, 13C1602 9P(10) ‘10 .6 30 253 935.5 .8 .0 1009.162 65( ‘9) R(48, 13C1602 9P(10) ‘9 498.1 30 254 970.9 .1 T 1009.197 19(1735) R(43, 13C1602 9P(10) 9 263.4 30 273 732.5 .5 .0 1009.823 02( ‘8) R(47, 13C1602 9P(10) 12 .6 30 276 592.7 .0 1009.918 41( 540) R(45. 1301602 9P(10) 12 .6 30 276 592.7 .3 1009.918 41( 1) R(44. 1301602 9P(10) 12 .5 30 277 449.5 .3 1009.947 00( ‘44) R(43, 13C1602 9P(10) 14 .0 30 279 386.1 .3 1010.011 60( 4) R(43, 13C1602 9P(10) 16 835.9 30 281 304.9 .1 1010.075 60( ‘7) R(45, 1301602 9P( 8) ‘14 .9 30 300 961.3 .7 1010.731 27( ‘9) 113 Table 3-7 (cont'd) aNulbers are J and K of the lower vibrational state. bLaser line used; laser frequencies were taken from Ref. g5. cMicrowave frequency in MHz. The signed microwave frequency was added to the laser frequency to obtain the absorption frequency. dObserved ninus calculated frequency in MHz; the paraneters for the calculation are in Table 3-9 of this work and in Table V of Ref. 1. eEstimated uncertainty in the observed frequency in MHz. An "OMIT" leans that the frequency was omitted from the least squares fits. f0bserved wavenumber in cn—l. The nulbers in parenthfses are observed sinus calculated wavenumbers in units of 0.00001 c- 114 TABLE 3-8 79 a Molecular Constants of CD3 Br Parameterb v2 = 0C v2 = lC Ev /GHz 0.8 29 721.322 4(12) av /MHz 7 714.650 1(68) 7 690.278 7(90) (Av-8v) /MHz 70 243.4d 7o 527.91(16) DJ /kHz 5.797 8(96) 5.567 7(107) DJK /kHz 65.026(452) 69.722(558) 0K ka2 450.d 382.742 5(68497) HJ /Hz -o.002 30(303) -o.017 39(425) HJK /Rz 0.174(121) 2.462(262) HKJ /Hz -18.52(746) -27.58(924) aux /R2 0.‘3 —1410.(115) LJ./mHz o.e 0.00325(76) LJJJK /mHz o.e -o.2999(533) LJJKK /mHz o.e 18.34(218) LJKKK /mHz o.e -435.3(291) ALK /nHz o.e 6677.(633) 8Values in parentheses are one standard deviation in multiples of the last digit in the parameter. bVibration-rotation parameters. AP = P(v2=l) - P(v2=0). CObtained from a fit of the vibration-rotation frequencies listed in Table 3-6 and hypothetical unsplit rotational frequencies calculated from the experimental frequencies reported in References lg and gg. dConstrained to the value reported in Ref. 2g. eConstrained to zero. 115 TABLE 3-9 Molecular Constants of CD3alBra Parameterb v = 0C v = 1c 2 2 Ev /GHz 0.e 29 721.073 2(12) 8v /MHz 7 681.278 0(106) 7 657.050 4(121) (Av-8v) /MHz 70 276.8d 70 562.22(19) DJ /kHz 5.580 2(124) 5.595 8(153) DJK /kHz 63.030(1188) 67.955(1237) 0K /kHz 450.d 455.3(83) HJ /Hz 0.013 15(394) -0.ooo 44(579) HJK /H2 0.053(282) 2.227(384) HKJ /Hz -18.85(l790) -23.86(2144) ARK /Hz 0.8 -284.(120) LJ /mHz 0.e 0.002 40(73) LJJJK /mHz 0.e -0.416 5(518) LJJKK /mHz o.e 15.03(324) LJKKK /mHz 0.e -984.9(874) ALK /mHz 0.8 3 441.(492) 8Values in parentheses are one standard deviation in multiples of the last digit in the parameter. bVibration-rotation parameters. AP = P(v2=l) - P(v2=0). CObtained from a fit of the vibration-rotation frequencies listed in Table II and hypothetical unsplit rotational frequencies calculated from the experimental frequencies reported in References 19 and 29. dConstrained to the value reported in Ref fig. eConstrained to zero. 116 is performed, the parameters are best interpreted as constants for frequency calculation only. The parameters have been used to predict coincidences between C02 and N20 laser frequencies (§Q,§§) and the frequencies of the v2 bands of both species of CD3Br. The predicted coincidences are shown in Tables 3-10 and 3-11. The differences between the observed and calculated frequencies are shown in Tables 3~6 and 3-7, where it may be seen that the residuals are usually well within the estimated experimental uncertainties; this is confirmed by the values of the standard deviations for an observation 79 of unit weight, which were 0.86 and 0.83 for the Br and 81Br species, respectively. 11 TABLE 3-10 7 Coincidences between Calculated Frequencies for the v2 Band of CD379Br and Laser Frequencies Trans.a Frequencyb uo-vLc Laser P(38,1) 29054033.96 -38.74 1201602 BAND I R(10) P(38,0) 29054105.00 32.30 12C1602 BAND I R(10) P(32,6) 29167161.93 48.06 12C1802 BAND I R( 8) P(27,3) 29264366.87 183.54 N20 R(49) -l41.27 1301802 BAND II P(60) P(27,6) 29264630.?6 122.62 1301802 BAND II P(60) P(26,6) 29283772.83 -3l.46 N20 R(50) P(26,5) 29283920.64 116.35 N20 R(50) P(23,5) 29339816.89 3.99 13C1602 BAND II R(42) P(19,5) 29412634.09 36.19 12C1802 BAND I R(22) P(15,0) 29477350.60 189.74 1201602 BAND I R(32) P(13,7) 29523877.89 -103.50 12C160180 BAND I R(28) P(12,2) 29529373.37 21.92 1301602 BAND II R(36) P(12,5) 29535113.27 40.78 12C1802 BAND I R(30) P(ll,6) 29555157.45 90.70 13C1802 BAND II P(50) P(10,6) 29572119.06 115.97 120160180 BAND I R(3l) Q(37,2) 29638806.15 -74.04 12C1602 BAND I R(42) Q(37,l) 29639068.83 188.64 1201602 BAND I R(42) P( 5.2) 29644222.22 -l79.72 1201802 BAND I R(38) Q(35,5) 29644480.38 78.44 12C1802 BAND I R(38) P( 5.4) 29648033.64 41.04 120160180 BAND I R(36) Q(31,4) 29662655.62 76.51 12C160180 BAND I R(37) Q(27,2) 29676834.52 ~126.07 12C160180 BAND I R(38) Q(22,0) 29691147.43 10.93 12C160180 BAND I R(39) Q(23,5) 29691209.84 73.34 120160180 BAND I R(39) Q(22,l) 29691307.70 171.20 12C160180 BAND I R(39) 0(21,1) 29693916.35 -l58.96 12C1802 BAND I R(42) Q(20,3) 29697831.03 -198.32 12C1602 BAND I R(46) Q(21,6) 29698196.81 166.33 12C1602 BAND I R(46) Q(17,3) 29704927.l3 -179.16 12C160180 BAND I R(40) Q(16,0) 29705012.?2 -93.57 120160180 BAND I R(40) 0(19,7) 29705092.29 -11.00 120160180 BAND I R(40) 0(16,1) 29705243.25 136.96 120160180 BAND I R(40) Q(13,2) 29711418.23 -l58.86 1301602 BAND II P(30) Q(17,8) 29711677.82 100.75 13C1602 BAND II P(30) 0(11,4) 29717755.86 106.03 1201802 BAND I R(44) 0( 6,0) 29718790.12 -79.26 12C160180 BAND I R(4l) 0( 7,4) 29722778.40 119.92 13C1802 BAND II P(44) 118 Table 3-10 (cont’d) Trans.a Frequencyb vo-vLc Laserd 0( 9,6) 29726342.55 -52.21 1201602 BAND I R(48) Q(ll,7) 29726432.03 37.27 1201602 BAND I R(48) 0( 6,5) 29726532.18 137.42 1201602 BAND I R(48) Q(lO,8) 29732378.36 -46.81 120160180 BAND I R(42) R( 3.3) 29784647.36 84.16 120160180 BAND I R(46) R( 4,1) 29796963.69 -109.55 12C160180 BAND I R(47) R( 6,5) 29833516.22 182.26 12C160180 BAND I R(50) R( 7,4) 29845124.?6 129.35 12C160180 BAND I R(Sl) R( 8.2) 29855897.74 26.03 1261602 BAND I R(58) R(13,5) 29930628.03 107.09 120160180 BAND I R(59) R(26,3) 30093278.81 58.56 13C1802 BAND II P(30) R(31,7) 30143745.44 -10.96 1301802 BAND II P(28) 798r; J < 40. K < 8. 8Transition in the v2 band of CD3 bFrequency of the v2 band transition in MHz. CFrequency of the 0 band transition minus the laser frequency in MHz. dIdentification of the CO laser; Band II is the 9 pm band. Laser frequencies were 0 tained from Refs. 34 and 38. 119 TABLE 3-11 Coincidences between Calculated Frequencies for the 02 Band of C0381Br and Laser Frequencies Trans.a Frequencyb vo-vLC Laserd P(39,5) 29033085.68 -52.19 120160180 BAND I R( 2) P(37,3) 29075724.25 137.89 12C160180 BAND I R( 4) P(37,2) 29076156.12 151.68 13C1602 BAND II P(50) P(36,6) 29089962.67 198.43 12C1802 BAND I R( 4) P(30,8) 29198208.41 -63.44 120160180 BAND I R(10) P(27,?) 29264622.06 113.92 13C1802 BAND II P(60) P(26,0) 29283694.97 -109.32 N20 R(50) P(26,1) 29283819.06 14.77 N20 R(50) P(25,7) 29303421.?2 108.04 N20 R(51) P(24,?) 29322629.33 ~81.88 N20 R(52) P(23,6) 29341996.45 -0.ll N20 R(53) P(16,5) 29466842.77 -134.00 1301602 BAND II R(38) P(12,1) 29529159.04 -195.42 13C1602 BAND II R(36) P(10,7) 29576373.04 -l72.09 12C1602 BAND I R(38) P( 7,1) 29611334.?5 -167.81 13C1802 BAND II R(48) P( 5,2) 29644317.12 -84.83 1201802 BAND I R(38) P( 5,4) 29648123.20 130.59 12C160180 BAND I R(36) Q(34,2) 29651565.?8 -91.33 13C1602 BAND II P(32) Q(34,l) 29651660.l4 3.03 13C1602 BAND II P(32) Q(34,0) 29651681.13 24.29 1301602 BAND II P(32) Q(29,6) 29668792.27 -63.56 12C1602 BAND I R(44) Q(27,6) 29676880.16 -79.78 12C160180 BAND I R(38) Q(27,2) 29676910.92 -49.67 12C160180 BAND I R(38) Q(22,0) 29691114.52 -21.98 12C160180 BAND I R(39) Q(23,5) 29691224.34 87.83 12C160180 BAND I R(39) Q(22,1) 29691276.38 139.88 12C160180 BAND I R(39) Q(21,6) 29698177.00 147.66 12C1602 BAND I R(46) Q(19,7) 29705050.18 -56.11 120160180 BAND I R(40) 0(16,l) 29705113.37 7.08 12C160180 BAND I R(40) Q(17,8) 29711623.55 46.48 1301602 BAND II P(30) 0(12,0) 297ll761.59 184.52 13C1602 BAND II P(30) Q(11,4) 29717566.62 -83.21 12C1802 BAND I R(44) 0( 7,0) 29717722.63 72.80 12C1802 BAND I R(44) 0( 6,1) 29718863.80 -5.58 120160180 BAND I R(4l) 0( 7,2) 29718923.38 54.00 12C160180 BAND I R(41) 0(10,4) 29719007.12 137.74 12C160180 BAND I R(41) 0( 7,4) 29722552.17 -106.3l 1301802 BAND II R(44) 0( 4,3) 29722696.93 38.45 13C1802 BAND II P(44) 120 Table 3-11 (cont’d) Trans.a Frequencyb vo-vLC Laserd Q(ll,7) 29726232.07 —161.94 1201602 BAND I R(48) 0( 6,5) 29726290.57 -104.19 12C1602 BAND I R(48) R( 8,3) 29856529.51 86.61 12C160180 BAND I R(52) R(10,4) 29886501.57 157.06 13C1602 BAND II P(24) R(14,2) 29938089.58 110.22 13C1802 BAND II R(36) R(14,5) 29942810.38 -110.36 13C1602 BAND II P(22) R(18,0) 29990238.92 -89.20 13C1802 BAND II R(34) R(18,l) 29990435.49 107.38 1301802 BAND II P(34) R(22,2) 30042050.23 -26.08 1301802 BAND II P(32) R(32,4) 30160897.88 177.99 13C1602 BAND II P(14) R(37.5) 30213122.03 95.90 13C1602 BAND II P(12) 8Transition in the v2 band of CDaalBr; J < 40, K < 8. bFrequency of the v2 band transition in MHz. CFrequency of the 02 hand transition minus the laser frequency in MHz. dIdentification of the C0 laser; Band II is the 9 pm band. Laser frequencies were ogtained from Refs. 34 and 38. 121 III—5 Discussion III-5-l CD3I As seen in Table 3-1, the vibration-rotation parameters for the ground and v2 = 1 states, including the Coriolis coupling, predict the infrared frequencies for J S 43 and K s 10 to an accuracy of a few MHz. As shown in the first two numerical columns of Table 3-4, the resulting parameters are quite reasonable and convergent. In fact, ARK, ALK, and LJ were so close to zero that they could be constrained to zero in the fitting without significant effect on the standard deviation for an observation of unit weight, which was ~0.7 for both fittings. The corresponding fitting in which explicit Coriolis effects were omitted also gave calculated frequencies that were in good agreement with the experimental values (standard deviation = 1.5), but, as shown in Table 3-3, the higher-order parameters, especially those that multiply higher powers of K, are rather large. This is the typical result of an attempt to mimic the effect of substantial Coriolis coupling by means of a power series expansion in J(J+1) and K2. An important conclusion is that it is possible to predict the vibration-rotation frequencies for J $ 43 and K s 10 in the 92 hand of CD31 to within a few MHz with the parameters in Table 3—4 in a simple power series expansion without Coriolis interaction. Above K = 10 the frequencies of the P, Q, and R branch transitions for a given J, which increase in frequency as K increases for lower K, reach a maximum and begin to decrease with increasing K. small number of higher K transitions have been assigned and their frequencies agree much better with the Coriolis-corrected calculated values than with the values Obtained with the simple power series 122 expansion. It appears that many higher K transitions can be recorded and assigned, but this was judged to be beyond the scope of the present study. Combination of such frequencies with those for the v5 band given in Ref. (2) should lead to an improved set of Coriolis parameters. The parameters in Tables 3-2 and 3-4 were used to calculate the vibration-rotation frequencies of the v2 band and the rotational frequencies in the v2 = 1 state for J g 50 and K S 15 for an attempt to assign the submillimeter laser transitions reported in Ref. (21). It was possible to give a definite assignment for two of the transitions and a provisional assignment for a third. The two assigned transitions are pumped by the 10R(38) CO2 laser at 27851242 MHz (reported at 10.764 pm in Ref. (21)). This laser frequency is only 8 MHz above the calculated frequency of the P(46,10) transition in the v2 band. In addition, the two reported submillimeter wave frequencies (538347.3 MHz and 526434.4 MHz) are only 0.9 and 2.7 MHz above the calculated values for the R(44,10) and R(43,10) transitions in the v2 =1 state, respectively. Since these calculated values should be within a few MHz of the experimental frequencies, these assignments are probably definite. The provisional assignment involves a submillimeter wave laser pumped by the 10P(36) CO at 27791010 MHz (reported as 10.787 pm 2 in Ref. (21)). This frequency is ~426 MHz below the calculated frequency of the P(49,13) transition in the v2 band. The reported submillimeter wave frequency is 572772.l MHz, which is ~19 MHz below the calculated value for the R(48,13) transition in v2 = 1. This agreement is probably satisfactory considering the fact that the J and K values for the transitions is outside the range of J and K for which the parameters are known to be valid. For this reason and because of the 123 strange behavior of the levels in v2 = 1 for k > 10, this last assignment must be viewed as provisional. The ground state vibration rotation parameters obtained as a result of this study are compared to the values obtained by microwave and millimeter wave spectroscopy in Table 3-2, where it may be seen that there is good agreement between the results of our fittings and that obtained previously (12). Comparison in Table 3-3 of the parameters derived in this work with the best previous infrared values, obtained from a laser Stark study of a relatively small number of transitions, shows that a much more complete set of centrifugal distortion constants has been obtained in the present study. As mentioned above, the inclusion of the effects of Coriolis coupling to the v5 and 2v3 states improves the fit of the rotation and vibration-rotation frequencies; the standard deviation for an observation of unit weight is reduced from 1.5 to 0.75. The resulting parameters are compared to the results given by Matsuura and Shimanouchi (2) in Table 3-4, where it is seen that the agreement is very good considering the small number of experimental frequencies for the v2 band that were available to these authors. The Corilis effects on the energy are substantial for this molecule, reaching almost 30 GHz for the highest J and K studied in this work. Therefore, the calculated vibration-rotation frequencies are very sensitive to the values assumed for the Coriolis and vibration-rotation constants. It is essential that the two sets of parameters be consistent. The parameters in Table 3-3 do not include the effects of the Coriolis coupling discussed in this paper. Comparison of the B values for v2 = l in Tables 3-3 and 3-4, for example, show the large 124 contribution of this Coriolis coupling to the rotational constants. III-5-2 CD Br 3 A substantial number of frequencies in the v2 bands of CD3798r and CD381Br have been measured to an accuracy of a few MHz by the method of infrared-microwave sideband laser spectroscopy and have been used to evaluate vibration-rotation parameters for the ground and v2 = 1 states for both species. The new parameters together with previously-reported vibration—rotation constants for v5 = l and the 122-v5 Coriolis coupling are sufficiently accurate to reproduce the experimental frequencies for J S 48 and K S 8 to within ~ 5 MHz. The parameters have been used to predict coincidences between CO2 and N20 laser frequencies (25,21) and the frequencies of the v2 bands of both species of CD3Br. The predicted coincidences are shown in Tables 3-10 and 3-11. The frequencies of a number of transitions for K > 8 have been omitted from the fittings and, as can be seen in Tables 3-6 and 3-7, these show rather large residuals. We interpret this to be the result of some problem with the accuracy of the Coriolis parameters and/or the parameters for the v5 = 1 state used in the fitting. Since the Coriolis corrections are very large, relatively small changes in these parameters, perhaps even within the round-off errors, would be sufficient to cause the difficulties observed. Since we do not have any data of our own for the 95 hand, we did not pursue this problem any further. 125 III-6 References 10. ll. 12. l3. 14. 15. 16. 17. 18. . E. W. Jones, R. L. Popplewell, and H. W. Thompson, Proc. Roy. Soc. London A288, 39—49 (1965). . H. Matsuura and T. Shimanouchi, J. Mol. Spectrosc. 60, 93-110 (1976). . K. Kawaguchi, C. Yamada, T. Tanaka, and E. Hirota, J. Mol. Spectrosc. 64, 125-138 (1977). . Y. Morino and J. Nakamura, Bull. Chem. Soc. Japan 38, 443-458 (1965). .‘E. W. Jones, R. J. L. Popplewell, and H. W. Thompson, Spectrochim. Acta 22, 639-646 (1966). . C. Betrencourt-Stirnemann, R. Paso, J. Kauppinen, and R. Anttila, J. Mol. Spectrosc. 87, 506-521 (1981). . K. Harada, K. Tanaka, and T. Tanaka, J. Mol. Spectrosc. 98, 349-374 (1983). . J. W. Simmons, Phys. Rev. 76, 686 (1949). . J. W. Simmons and J. H. Goldstein, J. Chem. Phys. 20, 122-124 (1952). A. K. Garrison, J. W. Simmons, and C. Alexander, J. Chem. Phys. 45, 413-415 (1966). R. L. Kuczkowski, J. Mol. Spectrosc. 45, 261-270 (1973). J. Demaison, D. Boucher, G. Piau, and P. Glorieux, J. Mol. Spectrosc. 107, 108-118 (1984). G. Wlodarczak, D. Boucher, R. Bocquet, and J. Demaison, J. Mol. Spectrosc. 124, 53-65 (1987). Y. Merino and L. Nakamura, Bull. Chem. Soc. Jap. 38, 443-459 (1965). C. Joffrin, N. Van Thanh, and P. Bardewitz, J. Phys. Paris 27, 15-23 (1966). R. W. Peterson and T. R. Edwards, J. Mol. Spectrosc. 38, 1-15 (1971). H. Kurlat, M. Kurlat, and W. E. Blass, J. Mol. Spectrosc. 38, 197— 213 (1971). D. R. Anderson and J. Overend, Spectrochim. Acta. A28, 1231-1251 19. 20. 21. 22. 23. 24. 25. 26. 27. 28. 29. 30. 31. 32. 33. 34. 35. 36. 37. 38. 126 (1972). D. R. Anderson and J. Overend, Spectrochim. Acta. A28, 1637-1647 (1972). C. Poulsen and S. Brodersen, J. Raman Spectrosc. 14, 77-82 (1983). J. Sakai and M. Katayama, Chem. Phys. Lett. 35, 395-398 (1975). J. Sakai and M. Katayama, Appl. Phys. Lett. 28, 119-121 (1975). G. L. Caldow, G. Duxbury, and L. A. Evans, J. M01. Spectrosc. 69, 239-253 (1978). S. A. Rackley and R. J. Butcher, M01. Phys. 39, 1265-1272 (1980). Y. Langsam, S. M. Lee and A. M. Ronn, Chem. Phys. 15, 43-48 (1976). W. Schrepp and H. Dreizler, Z. Naturforsch. 36a, 654-661 (1981). S. F. Dyubko, L. D. Fesenko, 0. I. Baskakov, and V. A. Svich, Zhurnal Prikladnoi Spektroskopii 23, 317-320 (1975). T. R. Edwards and S. Brodersen, J. M01. Spectrosc. 54, 121-131 (1975). Y. Morino and C. Hirose, J. M01. Spectrosc. 24, 204-224 (1967). H. P. Benz, A. Bauder, and Rs. H. Gunthard, J. M01. Spectrosc. 21, 156-164 (1966). J. T. Hougen, J. Chem. Phys. 57, 4207-4217 (1972). M. R. Aliev and J. T. Hougen, J. M01. Spectrosc. 106, 110-123 (1984). , C. H. Townes and A. L. Schawlow, "Microwave Spectroscopy," Chap. 8, McGraw-Hill, New York, 1955. C. Freed, L. C. Bradley,and R. G. O’Donnell, IEEE J. Quantum Electron. 08-16, 1195-1206 (1980). H.-G. Cho and R. H. Schwendeman, J. M01. Spectrosc. 133, 383-405 (1989). G. Magerl, W. Schupita, and E. Bonek, IEEE J. Quantum Electron. QB- 18, 1214-1220 (1982). S. K. Lee, R. H. Schwendeman, and G. Magerl, J. M01. Spectrosc. 117, 416-434 (1986). B. G. Whitford, K. J. Siemsen, H. D. Riccius, and G. R. Hanes, Opt. Commun. 14, 70-74 (1975). CHAPTER IV INFRARED-RADIOFREQUENCY DOUBLE RESONANCE OF CD31 AND CD3Br IV-l Introduction The radiofrequency spectroscopy provides a powerful tool for investigation of various hyperfine energy structures such as nuclear quadrupole splittings, Al-A2 splittings, x-doubling, K-doubling, hyperfine rotational levels of tetrahedral molecules, and so on. However, the scope of the technique is seriously limited by the density of the spectrum, the poor signal-to-noise ratio caused by the negligible population difference, and the low photon energy due to the small energy gap between the levels. As a result, radiofrequency spectra are often too weak to record properly or too complicated to analyze. In order to overcome the limitations, the radiofrequency double resonance technique has been invented which is a combination with another radiation of much higher energy photons. By detecting a photon with much higher energy than the radiofrequency photon, sensitivity and signal-to-noise ratio are greatly enhanced; and, by requiring two near—resonant photons for signal detection, the spectra are greatly simplified. The radiofrequency-microwave (RF-MW) double-resonance method was introduced by Autler and Townes (1). In their experiment, l-type doublets in the J=l and 2 rotational levels of the v2=l vibrational 127 128 state of 008 were probed while the corresponding rotational transition J=l~2 was pumped by microwave radiation. The RF-MW double resonance technique was further developed by Wodarczyk and Wilson (2) for assignment purposes in microwave spectroscopy. When the RF double resonance method was later extended to the infrared region (IR-RF double resonance), it became possible to observe RF resonances for higher rotational quantum numbers and higher-energy vibrational states than had been possible with RF-MW spectra. Infrared-radiofrequency (IR-RF) double resonance was first used by Shimizu to observe the Stark splittings of the P(3,2) transition of the v2 excited state of PH3 by pumping the transition with the R(33) N20 laser line (2). This technique was further developed and applied to various studies, mostly by workers at the Herzberg Institute of Astrophysics. Curl and his coworkers studied hyperfine rotational energy structures of CH4 by means of the laser coincidence of the 03 hand and He-Ne 3.39 pm laser line and intracavity radiofrequency cells (4,5). The IR-RF double resonance technique is sensitive enough that they succeeded in observing two rotational transitions weakly allowed by the centrifugally induced electric dipole moment. Later, the 9P(36) C1802 laser line was used for the investigation of the rotational energy levels of CD4 by Kreiner (Q). Kreiner and Oka extended this technique to observe forbidden rotational transitions of Sifld with P(5), R(4), and R(6) N20 laser lines (1). Arimondo and his coworkers applied the technique to the observation of pure quadrupole transitions in 003I by using 002 and N20 laser coincidences (2) and later analyzed energy transfer between rotational levels by means of collision-induced resonances in the radiofrequency region (2). Dale g1 g1. and Lowe g; 21 129 used their C0 laser to study x-doublings of NO utilizing the close coincidences of VI band transitions of NO in the 5.4 pm region (19,11). They also applied the spectrometer to investigation of the spin-rotation hyperfine structure of N02 (12) and of the Stark effect of H20 (12). Recently Sakai and his coworkers observed Al-A2 splittings in the ground state (K=3) and v5 state (K1=-2) of CDF3 by pumping the ”5 band with a CO2 laser (14). Mito g1 g1. employed the coincidence of P(8,0) transition of 07 band of CH3CN and 9P(30) CO2 laser line to search for l-type doubling transitions including collisionally transferred resonances and determined the effective l-type doubling constants q,7 and q1 (1g). Ioli and his coworkers performed radiofrequency triple resonance for CH3OH in order to study the K-doubling (1Q). Some k-type doublets of the v state of CH3I were observed by Arimondo and P. 6 Glorieux (11). Man and Butcher studied pure quadrupole transitions (12- 2g) of halide compounds and K-doublings (21) of formic acid by means of CO2 laser coincidences. Their precise experiment allowed determination of quadrupole coupling constants including the centrifugal distortion parameters and the spin-rotation constants. The early IR-RF double-resonance measurements were performed with the sample cell inside the laser cavity in order to apply the highest available powers to the samples. As a result, the line broadening caused by the power of the pump laser seriously restricted the accuracy of the frequency measurement. Among the first demonstration of IReRF double resonance outside the laser cavity were studies of CF31 and CF3Br in our laboratory (22,22). The lower pumping power still provides sufficient signal-to-noise ratio and many nuclear hyperfine structures are well resolved as a result of the considerably smaller linewidth. 130 Line-tunable infrared lasers provide accurate frequency and enough radiant power for saturating vibrational transitions; however, they restrict the method to accidental coincidences between the laser frequencies and the vibration-rotation frequencies of the molecule under study; this severely limits the performance of the technique. More recently, it has been shown that tunable infrared sources could be used for IR—RF double resonance. Takami introduced IR-RF double resonance by means of diode lasers in studying forbidden rotational transitions of v3=l state of CF4 (24). The diode laser was intentionally focused inside the coaxial radiofrequency cell used in the experiment in order to overcome the low radiant power of the laser. In a series of works, he and his coworkers investigated the hyperfine rotational energy structure of CF4 (2Q), 13 CF4 (g), Sill4 (21,22), and 811114 (2g) and determined the rotational parameters. The infraredemicrowave sideband laser was first used by Oka to observe forbidden rotational transitions of OsO4 (29) and Sifld (21). A color center laser was used to observe 1- type doubling in HCN by DeLeon et a1. (22). Oka also employed a color center laser to search for Al-A2 splittings of CH3F (22). In recent studies, we discovered that our infrared microwave sideband laser system operating in the cavity mode (24) had sufficient power to saturate vibration-rotation transitions. In this thesis we describe the use of our infrared-microwave sideband laser for the measurement of pure nuclear quadrupole transitions in the ground and v2=1 vibrational states of 003I and 003Br by the method of IR—RF double resonance. Before carrying out the double resonance measurements, it was necessary to determine the frequencies of the infrared transitions in the v2 vibrational bands of these molecules. Frequencies of 131 transitions with J,K up to higher than 40,8 were measured and fit to energy expressions for symmetric top molecules with centrifugal distortion. The measured IR frequencies and spectroscopic analyses have been described in Chapter III. The tunability of the infrared- microwave-sideband laser source allows the selection of vibration- rotation transitions over a wide range of J and k, which permits the evaluation of centrifugal distortion effects on the quadrupole coupling constants and spin-rotation interaction parameters, as well as the precise measurement of the quadrupole coupling constant itself. In addition to the advantages of tunability, the spectrometer is found to have sufficient sensitivity to work at very low RF power, which together with the very low power of the infrared—microwave sideband laser source substantially increases the resolution compared to direct 002 laser- pumped double resonance. As a result, it is possible to determine the spin rotation constants as well as the centrifugal distortion constants for the quadrupole coupling in these molecules. IV-l-l CD31 In a series of microwave studies of the ground vibrational state of CD3I Simmons and co-workers (25-21) resolved quadrupole components and determed the primary quadrupole coupling constant as well as rotational constants. Kuczkowski (22) extended this microwave work to transitions in the low-lying vibrational states 02, v3, ”5’ v6, 203, and 03+ve. More recently, higher J transitions have been recorded in the millimeter wave region and more accurate quadrupole constants were reported for low—lying vibrational states by Demaison 41 Q1. (22) and by 132 Wlodarczak g1 g1. (49). Infrared radio frequency double resonance at 1— MHz resolution was reported by Rackley and Butcher (41) as part of a study of Stark-tuned non-linear spectroscopy. Demaison g1 g1. (22) used infrared radio frequency double resonance to measure the frequencies of pure quadrupole transitions in the ground state of this molecule with 100 kHz accuracy. The influence of nuclear quadrupole coupling on rotational relaxation has been investigated by means of microwave double resonance (42). In the present study, about 150 radio frequency resonances, half each in the ground and v2 = 1 states, have been recorded at 70 kHz resolution and few kHz accuracy by using the infrared microwave sideband system as a pumping source for infrared radio frequency double resonance. In addition to demonstrating the usefulness of this technique for systematic infrared radio frequency double resonance, the radio frequencies have been combined with previous measurements of microwave, millimeter wave, and infrared radio frequency double resonance spectra to determine nuclear quadrupole coupling parameters, including centrifugal distortion effects, and spin rotation parameters for the iodine nucleus. IVrl-Z CD38r The splittings caused by Br quadrupole coupling in CD3798r and 381Br have been studied in the microwave region for the ground state CD by Garrison 91 Q1. (42) and in low-lying vibrational states by Morino and Hirose (44). Consequently, values of the quadrupole coupling constants for the ground and v2 = 1 states of the two species have been 133 reported. However, we are not aware of any previous measurements that are sufficiently precise to include the effects of the centrifugal distortion of the quadrupole coupling or of the spin-rotation interaction. An infrared microwave sideband laser source operating in the 10 pm region has been used with the method of infrared radiofrequency double resonance to record radiofrequency spectra in the ground and v2 = l vibrational states of CD3Br. The frequencies of ~ 200 and ~ 160 pure 81 3 3 Br, respectively, approximately half in the ground state and half in the v2 quadrupole transitions have been observed for CD 798r and CD = l vibrational state of each species. The frequencies have been used to determine the quadrupole coupling constants, including centrifugal distortion parameters, and spin-rotation constants for the bromine nucleus in each species. During the fitting of the frequencies of the pure quadrupole spectra, it became apparent that some effect was causing an apparent shift in frequency for each of a pair of closely spaced double resonance transitions that occur at low RF frequencies. This shift has been traced to a double-resonance effect that appears in calculations when four interacting levels are taken into account, but is not evident in calculations based on the usual three-level system employed for double- resonance theory. The nature of the shifts, a description of the theory used to interpret them, and a comparison of observed and calculated lineshapes is described separately in Chapter V. The theory of vibration-rotation-quadrupole interaction is outlined in the next section, whereas the experimental details of this study are presented in the subsequent section. The last two sections 134 include a description of the spectra and a discussion of the results of this work, respectively. 135 IV-2 Theory IV-2-l IRrRF Double Resonance The mechanism of IR—RF double resonance is easily understood by considering a three-level system excited by laser and radiofrequency fields. We assume that two levels in the excited state form the hyperfine structure and that the laser frequency is much larger than kT/h. An example of a three—level system is shown in Fig. 4-1, where state ll) is a rotational level in the ground vibrational state and states [2) and [3) are rotational levels in an excited vibrational state. The laser radiation will interact with a group of molecules with velocity v, which satisfies the Doppler shifted resonance condition 012 = ”IR (l-v/c). If the infrared radiation is strong and the gas pressure low, molecules with the correct velocity will be "pumped" from state II) to |2>. This occurs when the infrared Rabi frequency, xRabi(IR) = pleIR/h, is comparable to or larger than the collisional frequency, = (Av)p-p. Here ”12 is the transition dipole moment matrix v 0 O collision element, E is the laser electric field, (Av)p is the pressure IR broadening parameter, and p is the gas pressure. Due to the pumping, "holes" are burned in the Maxwellian velocity profile of state II) and transferred to state l2) as "spikes." When the radiofrequency radiation with sufficient power for saturation comes into resonance with the transition between levels, the "spikes" in level I2) are transferred to level [3). This causes an increase in infrared absorption and is detected as a decrease in the infrared radiation reaching the detector. The condition for saturation by the 136 I3) -———-—— _1...— RF _/_/_\__ A IR PUMPING IR and RF PUMPING l1) —--- Figure 4~l. Three level system showing double resonance technique. The infrared radiation pumps molecules from ll) to |2> according to the Doppler shift resonance condition v12 = vIR(ltv/c) which appears as "holes" in the Maxwellian velocity profile of ll) and "spikes" in |2>. The radiofrequency will then transfer the "spikes" from |2> t0 l3) creating deeper "holes" in II). This causes an increase in the molecular absorption. The radiofrequency transition from [2) to |3> can thus be observed by detecting the infrared radiation. 137 radiofrequency is that its Rabi frequency, xRabi(RF) = ”23'ERF/h’ needs to be comparable to or larger than the collisional frequency, where p23 is the transition dipole moment matrix element in the excited state, and ERF is the radiofrequency electric field. In terms of the absorption coefficient, the maximum value is obtained when the saturation parameter pE/hv ~ 1 (2). collision According to Shimizu, the maximum attainable rf—induced absorption coefficient in this technique is 13* of the linear absorption coefficient for a Doppler-limited three-level system (2). The linewidth increases with increasing field intensities. The best operating condition is usually obtained when the saturation parameters of both fields are around one. In case the saturation parameter of the rf field is larger than that of the laser, the resonance line splits into a doublet. IV—2-2 Nuclear Quadrupole Coupling 12 Atomic nuclei have radii near 10_ cm, and hence are very small compared with the size of electron orbits, which are approximately -8 cm in diameter. Nuclei are also some 104 times heavier than 10 electrons. To a good approximation, therefore, electronic energies can be obtained by considering nuclei to be positive point charges of infinite mass. However, effects on electronic energy levels due to the finite size and mass of nuclei, although small, often appear on observation of atomic and molecular spectra. These effects are called "hyperfine structure" because they produce a very small splitting of spectral lines. 138 If a nucleus is to be considered other than a point charge, it must be recognized that the nuclear particles may be in motion, producing a magnetic field and giving the nucleus an angular momentum. The interaction energy between a nuclear charge distribution pi(xi, yi, 21) and an electron charge distribution pe(xe,ye,ze) is p.p d£.dg _ I 1 e R 1 e (4_1) where /2 :U u (r?+r2-2r.r cosm)1 1 e 1 e Here, ri=vector from the origin of the coordinates of the nuclear center of mass to the volume element dri, 5e the vector from the origin to the volume element dge and m the angle between Ei and Ee' Only s electrons have non-negligible charge distribution inside the nucleus. However, the contribution of s electrons to the quadrupole coupling energy vanishes because of the spherical symmetry of the electron orbital. We therefore expand l/R in powers of ri/re to obtain as r. 9. _1- = Fl 2 [Fl] P (cosm) . (4-2) e i=0 e 1 Where P1(cosm) is the Legendre polynomial of order 1. It is convenient to use the spherical harmonic addition theorem in the form, 139 2 P1(cosu) = z (-1)"(§§ETJ Y1m(e£, ¢£)Yi,-m(°i’¢i) . (4—3) m=-1 Substitution of Eq. (4-2) in Eq. (4-1) gives W as a series of integrals, as follows: Then, 9.0 p - 1 e - .9 _ wo _ [I ;;——d§idre 2e] re dr (4 5) where Z ' atomic number. This is the Coulomb interaction between the nucleus and the electrons, which is independent of the nuclear orientation and would be included in the determination of the electronic energy. The second term in the series of W is ”i "I: II_;2 C080 pipedsidge e pe Ee [I ”i EidEi] dEe ° (4'6) =1 3 r e The quantity in square bracket is the nuclear electric dipole moment; hence W1 is the nuclear dipole interaction energy. However, if the 140 nucleus has a dipole moment in one direction with respect to its angular momentum, there must be a degenerate nuclear state, or one of the same energy, with an oppositely directed dipole. Normally, such identical or degenerate states of the nucleus are not encountered. Hence the nucleus has no inherent dipole moment, and no effects from nuclear dipole moments have been observed, so that we can assume that this term vanishes. The rule is rather more general as all electronic multipole moments of odd order are zero for a nucleus. The third term in the series for W is the quadrupole interaction, r . = n -;;- WM =22 (- —1)‘“(4—5") [p33 r 72.3“ (e. .0. )dr [0° 3 72 m(°e .0 )dr <4-7) m=-2 re e +2 m or HQ: 2 (-l) va—m m--2 _ g]1/2 where vm_&1%r3h2,m( e’¢i) dz:i re fll/Z ' (4 ‘2'] 1°11 13y2’_m(ei,¢i) d5i VIII and Q_m are components of second-rank irreducible spherical tensors since they are integrals of a spherical factor (~rn) times a spherical harmonic (ref. (45), P. 115). They are characterized by 1 in the nuclear space and g in the molecular space. The quadrupole moment may be considered as a measure of the 141 deviation of the nuclear charge from the spherical shape. If the charge distribution is somewhat elongated along the nuclear axis 2n, then 0 is positive; if it is flattened along the nuclear axis, 0 is negative. IV—2-3 Irreducible Tensor Method If the interaction energy of two parts of any quantum mechanical system is invariant under arbitrary rotations of the space-fixed axes, then it can be written most generally as a contraction of two irreducible tensors (gfi). Usually, the system may be divided into two distinct parts, characterized by their angular momenta J1 and J2, so that one tensor depends exclusively on one set of variables and the other tensor on a set of variables in a different space. The matrix elements of such a contraction of two commuting irreducible tensors A and B of rank K are given in the irreducible representation where the angular momenta of the two parts are coupled to form the resultant J=J1+J2 as (J1,J2,J,MIA:BIJ',Jé,J',M'> J J J _ _ J +J'+J 2 l , . _ -( 1) 2 l SJJ'SMM' {k Ji Jék . (4 8) The symbol in curly brackets is the Wigner 6j symbol. Eq.(4-8) expresses the fact that each matrix element is proportional to constants (JlflAflJl) and (JZHBHJZ) called reduced matrix elements which may be determined by using the Wigner-Eckart theorem, as follows; 142 1; g) . <4-9) ° (1) H I _ _ aj-m .j (J,m|Tq IJ ,m >-( 1) (—m If any one of the matrix elements of an irreducible set of spherical tensors Téi) of rank i is known in the representation with the angular momentum quantum number j and the projection quantum number m, the remaining elements can be determined. The symbol in parenthesis is the Wigner 35 symbol, which contains the entire dependence of the matrix elements on the projection quantum number. The relation of a quantity, which refers to only one of the interacting systems, between its reduced matrix element in the coupled representation and in the original uncoupled representation is expressed as (i) J1+J2+J' +i (J1,J2,JHT HJ',J2,J'> = (-1) J1 J J '[(2J+1)(2J'+1)]1/2 { . J. 12} (4—10) 1 where the tensor operator T(1) acts only in the J1 space. It is therefore possible to calculate the matrix elements of any observable in the coupled representation using Eq. (4—9) and (4-10). IV-2—4 Quadrupole Interaction Energy As shown above, the quadrupole interaction energy can be expressed as a contraction of two irreducible tensors of rank 2: the electric field gradient tensor V and the nuclear quadrupole moment tensor 0. 143 2 - _ m _ The quantity Q-m is the -m component of the nuclear quadrupole tensor, 9. The nuclear quadrupole moment, Q, is defined conventionally to be the I, mI=i diagonal matrix element of the m=0 component of Q i.e.; eQ = 2 (4-11) where e is the electric charge. The matrix elements of HQ in the coupled representation F = J+I are given according to Eq. (4-8). It turns out that H6 may be factorized into blocks for the different quantum numbers of the total angular momentum F and is independent of the projection quantum number M From the Wigner-Eckart theorem F. o I -I 0 or [(21+3)(21+2)(21+1)(2I)(ZI-l)]1/299 2[3IZ—I(I+1)] 2 ' = (4‘12) The symbol in parenthesis is the Wigner 3j symbol, and called the reduced matrix elements. The electric field gradient tensor V has constant components VA in the molecular frame. Hence it is necessary to transform one component of V to the principal inertial axes 144 2 (2) v0 = Z 2noq (or,B,r)V_'_q (4-13) q=- ’ ( where 00:)(u,8,r) is a matrix element of the five-dimensional irreducible representation of the three-dimensional rotation group, which depends on the Eulerian angles a, B, Y locating the molecular frame in the space-fixed axes system. The matrix elements of 032) in the symmetric rotor basis mé§)(a,8,r) c (2J+1)1/20é§)(a,8,r) are given as = <—1)"“"“”q [(2J+l)(2J'+1)]1/2 J 2 J' J 2 J' ”(m o m)(-k -q 1..) (4-14) using k for the projection quantum number in the molecular frame and m for the same in the space-fixed system. Then, the reduced matrix element of the V tensor is calculated with the aid of Rqs. (4-10), (4- 13), and (4—14) to yield J 2 J = (-1)J+k[(2J+1)(2J'+1)]1/2(-k —q k;)v;q/2 . (4—15) The matrix elements of the quadrupole Hamiltonian can be expressed in the specified representation by introducing the reduced matrix elements (4-12) and (4—15) into Eq. (4-8) for each F block 145 = (_1)J+J +k+I+F+1 ( J 2 a) :E_:a__5_ x_q/4 (4-16) .[(2J+1)(2J'+1)]1/2 iF I J] I 2 I {—1 o I) 2 J' I with the abbreviation xq = eQVé for the quadrupole coupling tensor. The irreducible quadrupole coupling tensor may also be expressed in the Cartesian axes x0 - xzz’ xfl = $(2/3)1/2(sz x ixyz). (4-17) _ 1/2 . X12 - (1/5) (xxx - xyy : 21xxy). The explicit expressions for the matrix elements of the quadrupole interaction have been derived by Benz et a1. (gfi). The matrix elements used in this study are listed in the Appendix of this chapter. I and CD Br IV—2-5 Quadrupole Coupling of C03 3 The interaction between a nuclear quadrupole and an electric field gradient splits the rotational level into 21+l hyperfine levels if J 2 I, where I is the nuclear spin number. The complete Hamiltonian for quadrupole interaction includes the rotation of the molecules since J is no longer a good quantum number. Especially the quadrupole couplings of Iodine (qu[CDaI] = ~-1930 MHz) and Bromine (qu[CD3Br79] = ~576 MHz, 81 qu[CD3Br ] = ~481 MHz) are large enough that calculation to the accuracy of 1 kHz requires inclusion of the effect of centrifugal 146 distortion on the quadrupole interaction and the spin-rotation interaction and diagonalization of the appropriate energy matrices. The method used to calculate the quadrupole interaction energy has been described in Chapter III in the discussion of the effect on the vibration-rotation energies of the molecules. As mentioned, the matrix H, as defined, is diagonal in F, I, and k; therefore, submatrices indexed by the possible J’s (usually 6x6 for CD I and 4x4 for CD3Br) 3 were set up and diagonalized to obtain the energy levels; the eigenvalues were indexed by the J value of the closest diagonal element. For 0031, all of the microwave(§§-§Q) and radio frequency data for the ground vibrational state(§g) were combined and used in a least squares adjustment of the rotational, centrifugal distortion, quadrupole coupling, distortion quadrupole, and spin rotation constants for the ground state (21 parameters). In this calculation the unresolved microwave data were included, but were assumed to have no quadrupole or spin rotation contribution. In the corresponding fitting for the v2 = 1 state the centrifugal distortion constants and the rotational constants, except the B value, were constrained to the values obtained from the fitting of the vibration-rotation spectra because only a small number of rotational frequencies in the v2 = 1 state have been measured. For CD3Br, the least squares fitting was performed by adjusting only the six quadrupole and spin-rotation parameters qu, xJ, XK’ xD, and C C the vibration-rotation parameters were constrained to the N’ K‘ values determined in the analysis of the infrared spectra (Chapter III). This was done because of a limited number of reported microwave frequencies. The experimental data for the fitting included the previously-reported microwave frequencies (fl§,flfl), in addition to all of 147 the measured IR—RF double resonance spectra. The calculated frequencies of the IR—RF double-resonance spectra were obtained from the computed energy levels by using the selection rules AJ = 0, Ak = 0, and.AF = t1. 148 IV-3 Experimental Fig. 4-2 is a block diagram of the infrared radiofrequency double resonance spectrometer used in the present study. The infrared microwave sidebands are generated in a CdTe electrooptic crystal that is irradiated simultaneously with the output of a frequency-controlled CO2 laser and the output of a ZO-W traveling wave tube amplifier. For IR-RF double resonance, the sideband generator was operated in the "cavity mode" (g3), in which the electrooptic crystal is made part of a tunable microwave cavity. In order to provide a cavity resonance, a tunable short was used which is adjustable anywhere in the 8-18 GHz range. In this mode the sideband output was ~l mW per W of infrared power. Since we normally used 2 W of 002 laser power, the typical sideband power was 2 mw, which is sufficient to saturate partially an infrared transition in the molecules. In order to maintain highest power, the beam splitter and reference detector used in traveling mode operation (g5), are not employed in the cavity mode of operation. Also, the PIN diode is set for maximum transmission. The sidebands were directed through a radiofrequency cell which is made of a l-meter piece of X-band waveguide with a centered septum in a stripline design (31). The RF cell was matched to a 50 9 transmission line impedance and has Ban windows. The infrared power was detected by a liquid-N2 cooled Hg-Cd-Te photoconductive detector (Santa Barbara Research Center Model 40742), whose signal was processed at the modulation frequency by means of a lock-in amplifier and recorded by a computer. The frequency of the infrared source was set at the center frequency of the Doppler-limited infrared transition, especially for CD3Br. Because of the relatively 149 PZT L I 4 1TH” X D“ cu LASER STAB 8 Vac : , ~ ' Fluorescence Cell Polorlzer Strlpllne Cell + s e u————$ ATT. 53355 lam" .9 ower ATT. Meter RF RF DET' I SYN. AMP. q, A/D DBM TVTA PRC»? 1 \l/ l DB" 33.344 W SYN. CDMPUTER °°""°‘ non. I 5 PSD. (— A/D Figure 4—2. Block diagram of the infrared radiofrequency double- resonance spectrometer used to record the pure quadrupole transitions in this work. An infrared microwave sideband laser in the cavity mode serves as the infrared pumping source. A radiofrequency synthesizer whose output is chopped by a double-balanced mixer and amplified serves as the radiofrequency source. 150 small hyperfine splitting of the vibration-rotation transitions, all of the expected double resonances could be recorded without retuning the infrared frequency. However, when the frequency difference between the component and the hypothetical unsplit frequency was calculated to be more than 10 MHz, the frequency of the infrared sideband laser was fixed at the frequency of the desired hyperfine component. we estimate the accuracy of the time averaged infrared pump frequency to be 1150 kHz. The frequency jitter of this source is also ~150 kHz, which is mostly the intentional laser modulation for the frequency stabilization. The radiofrequency was generated by an RF-synthesizer (Programmed Test Sources Model PTS 500) operating in the range 1-500 MHz with +3 to +13 dBm output. The frequency and the power of the radiowaves were controlled by the computer through an interface built at MSU. The radiowave was 100 X amplitude modulated at 33 kHz (Hewlett Packard 8428 C Modulator Control) by means of a double balanced mixer (DBM, Mini- Circuit Laboratory Model ZAD-lSH) at the output of the synthesizer. The switched RF output from the DBM was amplified by broadband power amplifier (Electronic and Navigation Industries, Inc. Model 525 LA). The amplified radiofrequency power from the computer-controlled synthesizer was applied to the central electrode of the cell. The power of the radiowave was monitored at the exit of the cell by a thermister detector (Hewlett Packard 8478 Thermister Mount) and a power meter (Hewlett Packard Model 432) after 30 dB attenuation. The signal of the power meter was fed into the computer, which in turn sent a correction voltage to the synthesizer in order to maintain constant power of the radiowave. The computer increased the radiofrequency in steps of 20 kHz within the range 1-500 MHz and recorded the output of the lock-in 151 amplifier, which consisted entirely of double-resonance effects. The RF power at the sample cell was kept as low as is consistent with reasonably good signal to noise ratio, because the spectra are easily RF power broadened at the low sample pressures used. Typical RF powers were of the order of a few milliwatts for CD31 and 5-50 milliwatts for CD3Br. An example of an infrared radio frequency double resonance spectrum of CD31 is shown in Fig. 4-3, where it is seen that the half width at half maximum for the transitions is about 70 kHz. Figs. 4-4 and 4-5 show typical IR-RF double resonance spectra for CD379Br and CD381Br, respectively, where it may be seen that the half width at half- maximum for the transitions is about 100 kHz. The center frequencies of the RF transitions were determined by fitting the observed lineshapes to a Lorentz function or to a sum of Lorentz functions for overlapped transitions; we estimate the RF accuracy of well-resolved transitions to be 1-5 kHz. The methyl iodide and the methyl bromide were fully-deuterated samples obtained from Merck & Co. and used as received except for the usual freeze-pump-thaw cycling. Sample pressures were 3-5 mTorr for the double resonance measurements. All spectra were recorded at room temperature (~297 K). 152 35 I ' I T I I T T 25 “'- d A P(22,5) 3 . 15 15.. 3 .d 5 - .1 s. 3 a -5 _ 4 '77) C 3 ~15 - - E -25 L- Upper F - 45/2 - 43/2 Lower F I- 47/2 - 45/2 -I _3 . 1 . 1 . L a 1 . L . ?05 106 107 108 109 110 111 Radio Frequency (MHz) Figure 4—3. A portion of the infrared radiofrequency double resonance spectrum obtained by pumping the P(22,5) transition in the 02 band of CD31. The F quantum numbers of the transitions in the upper and lower states of the vibration-rotation transition are shown. The horizontal axis is the absolute radiofrequency. the sample pressure was 3 mTorr and l-m path length was used. 153 35 t j t I u r fi— I ' j -I 7. '4 25 CD3 Br P(22,6) A 4 l 9? 15-1 J c :3 .o' L o V >. 3: 0‘) c a) 'E - r-n/z-os/z F-41/2-39/2 r-4s/2-47/2 r-u/z-u/z * I l -35 V l I r T I I F r I f 109 110 111 112 113 114 115 Radio Frequency (MHz) Figure 4~4. Example of infrared radiofrequency double resonance spectra obtained in the present study for CDs7gBr. For these transitions, the infrared sideband laser source was tuned to the center frequency of the Doppler-limited lineshape of the P(22,6) transition in the ”2 band. For the infrared microwave sideband laser source, the 10R(26) 1201302 laser was used with a microwave frequency of 11726 MHz; the lower frequency sideband was used. 154 35 1 T f I F I r 4 I ll 25- CD3 Br P(30,6) .. A d d :2 15 'E - q 3 1 .d 5— a L 3 ‘i 'i > -5-J _q «H '6 ‘ ‘ c 3 -15-' -I E , F-57/2-55/2 r-59/2-57/2 . _25_1 F-59/2-6l/2 F-51/2“63/2 _. . V2=1 V2=O . —35 . r . , . , . 125 126 127 128 Radio Frequency (MHz) Figure 4—5. spectra obtained in the present study for CD3818r. Example of infrared radiofrequency double resonance For these transitions, the infrared sideband laser source was tuned to the center frequency of the Doppler-limited lineshape of the P(30,6) transition in the v2 band. For the infrared microwave sideband laser source, the 10R(18) 1201602 laser was used with a microwave frequency of 9747 MHz; the lower frequency sideband was used. 155 IV-4 Results and Discussion IV-4-l CD31 About 150 radio-frequency resonances in CD31 were recorded by the IR—RF double resonance technique; 19 vibration-rotation transitions with J’s between 4 and 31 and K’s between 1 and 9 were pumped. In many cases all 10 of the possible RF resonances were measured. It was often possible to observe all of the RF resonances with a single infrared pumping frequency. This can be explained by the fact that each quadrupole component is in resonance for some velocity group within the Doppler profile for the transition frequency (Fig. 4-6), though the intensities of the transitions vary because they depend on the Maxwellian (Gaussian) weight. The results show that the IR—RF double resonance method is very powerful for studying pure quadrupole transitions, especially for high J transitions. For these transitions, the quadrupole hyperfine splittings in the infrared spectrum are usually very small (a few MHz), because the hyperfine shifts in the energies of the upper and lower states are almost the same. However, the shifts in energy for the hyperfine components of a single vibration-rotation level are still very large for high J (up to 300 MHz). The AF = :1 selection rules for the RF resonances allows the differences in these large shifts to be observed directly. An example of RF transitions observed by IR-RF double resonance is shown in Fig. 4-3. Previously reported microwave and radiofrequency transitions are also included in the least squares fittings with their estimated uncertainties. The frequencies of the radiofrequency transitions measured in this work are shown in Table 4-1 with their estimated 156 T JI+I-1 J’-I+8 v -1 J"K i "NH 3 ‘ I J’-I+1 J’+I .J’-I RF F d In rare " Tronsltlans Tronsl‘tlons K - Whuh F: ‘1' J+I‘1 J-I-l-E J)K J+I-1 G'S' J-I+1 J+I J-I Figure 4-6. Typical energy level pattern far the infrared radiofrequency double resonances Observed for CD31. In most cases, a single infrared frequency pumps all of the allowed infrared transitions by interacting with molecules in different velocity groups. 157’ Table 4-1 Pure Quadrupole Frequencies of CD31 v = 0 v2 = l J zr’ 2F” v/MHz o—ca nob J 2F’ 2?" 0/882 o—cc nob Pumpd 5 15 13 300.357 4 5 4 13 11 290.458 —17 5 1 13 11 57.337 -3 5 11 9 34.853 38 20 1 7 9 180.203 -29 20 5 7 179.019 18 5 2 3 5 175.589 0 5 2 5 15 13 199.185 2 5 3 13 11 38.939 -2 5 4 11 9 17.739 33 20 3 9 11 85.409 4 5 7 9 54.518 10 5 3 7 9 120.597 -1 5 5 7 85.115 20 5 4 3 5 82.945 -8 20 4 7 19 17 308.174 -29 20 8 17 15 304.872 20 20 5 17 15 83.897 -3 5 15 13 72.909 8 5 5 13 15 74.580 0 5 11 13 85.015 -1 5 8 11 13 177.185 12 5 9 11 179.245 -2 5 8 9 21 19 98.493 -8 5 8 19 17 92.248 8 5 7 15 17 173.113 7 20 13 15 175.258 —4 5 7 10 25 23 99.388 0 5 9 23 21 51.889 -17 5 8 23 21 34.354 -4 5 21 19 17.830 3 5 8 17 19 9.922 8 20 9 17 19 58.233 -1 5 15 17 30.194 -3 5 9 12 29 27 181.095 -8 5 11 27 25 134.888 0 5 10 27 25 59.083 0 5 25 23 48.010 0 5 10 23 25 23.980 -18 20 21 23 21.898 21 20 11 21 23 89.114 3 5 19 21 75.192 -7 5 11 19 21 137.522 -7 5 17 19 113.882 -2 5 11 14 33 31 149.473 -8 5 13 31 29 125.888 -2 5 12 31 29 57.578 —12 5 29 27 47.495 1 5 12 27 29 19.208 -21 5 25 27 17.297 21 20 13 25 27 81.852 -5 5 23 25 89.150 -8 5 13 23 25 130.498 -2 5 21 23 108.844 ~17 5 13 14 31 33 48.795 5 5 14 29 31 17.907 -33 20 14 27 25 28.241 35 20 15 25 23 41.181 5 5 15 17 39 37 257.732 -5 5 18 18 39 37 108.818 3 5 37 35 103.820 4 5 18 35 37 28.871 33 20 33 35 27.888 -12 20 18 33 35 140.217 -8 5 31 33 138.558 12 5 18 31 33 234.447 2 5 29 31 229.373 -2 5 18 1583 Table 4-1 (cont’d) - 0 v2 - 1 J ZF’ 2F" v/MHz o—c‘ ucb J 2r' 2F” v/an o—c° ucb Pumpd 18 41 39 237.778 4 5 17 39 37 230.748 ~10 5 17 39 37 97.078 7 5 37 35 93.033 2 5 17 35 37 24.388 42 20 33 35 24.890 -20 20 17 33 35 127.383 0 5 31 33 124.079 4 5 17 31 33 213.015 5 5 29 31 205.491 -5 5 17 19 43 41 109.599 0 5 18 41 39 88.375 10 5 18 41 39 45.591 0 5 39 37 38.483 12 5 18 37 39 10.393 -8 20 35 37 8.788 22 20 18 35 37 58.573 7 5 33 35 47.445 7 5 19 33 35 99.173 4 5 31 33 79.738 8 5 19 22 49 47 273.529 8 5 21 47 45 271.587 -8 5 20 47 45 118.014 2 5 45 43 114.244 8 5 20 43 45 23.187 25 20 41 43 24.018 —8 20 20 41 43 144.731 -8 5 39 41 144.098 17 20 20 39 41 249.583 4 5 37 39 248.788 -2 5 20 22 49 47 257.427 10 5 21 47 45 253.879 -14 5 21 47 45 109.225 4 5 45 43 108.848 1 5 21 43 45 21.780 33 20 41 43 22.412 -14 20 21 41 43 138.217 —4 5 39 41 134.718 8 5 21 39 41 234.937 3 5 37 39 230.775 -10 5 21 23 51 49 189.077 -1 5 22 49 47 157.529 3 5 22 49 47 72.494 4 5 47 45 87.079 5 5 23 43 45 89.245 3 5 41 43 83.373 8 5 23 41 43 155.101 1 5 39 41 144.034 -7 20 22 28 57 55 288.894 —22 20 25 55 53 288.899 17 5 24 55 53 125.810 —10 5 53 51 125.002 10 5 24 51 53 20.818 22 20 49 51 21.588 -14 20 24 49 51 151.591 37 20 47 49 151.891 -24 5 24 45 47 288.084 8 5 24 28 57 55 279.957 3 5 25 55 53 278.978 —10 5 25 55 53 121.934 -4 5 53 51 120.819 3 5 25 51 53 20.155 25 20 49 51 20.821 -17 20 25 49 51 148.817 —32 20 47 49 148.847 28 20 25 47 49 258.814 -2 5 45 47 257.182 -5 5 25 27 57 55 89.484 —2 5 28 55 53 88.024 8 5 28 51 53 108.722 -10 5 49 51 103.352 12 5 28 49 51 189.181 -2 5 47 49 182.348 -3 5 27 1553 Table 4-1 (cont’d) v = 0 v2 = 1 I O! a b g u C b d J K 2F 2F v/bflz O-C 00 J K 2F 2F 1.7/m: 0-0 00 Pump 30 4 65 63 283.814 -4 5 29 4 63 61 283.358 -4 5 28 63 61 126.027 -5 5 61 59 125.297 5 5 28 59 61 17.743 34 20 57 59 18.261 -17 20 28 31 9 67 65 226.064 4 5 30 9 65 63 221.747 -8 5 29 65 63 100.904 -2 5 63 61 98.602 2 5 29 59 61 117.536 -10 20 57 59 115.485 10 5 29 57 59 211.477 2 5 55 57 207.037 -7 5 29 aObserved minus calculated frequency in kHz. The parameters for the calculation are in the second column of Table 3-2 and in the first column of Table 4-3. bEstimated uncertainty in the observed frequency in kHz. cObserved minus calculated frequency in kHz. The parameters for the calculation are in the first column of Table 3-3 and the third column of Table 4-2. dPump transitions and frequencies are listed in Table 4-2. 160 uncertainties. Also shown in Table 4-1 are the observed minus calculated frequencies for the parameters derived in this work. Table 4-2 lists the infrared transitions that were pumped for the RF double resonances listed in Table 4—1. The quadrupole and spin rotation parameters obtained from the radio frequencies and the resolved microwave frequencies for both vibrational states are in Table 4-3. As shown in the table, the centrifugal distortion parameters for the quadrupole coupling and the spin—rotation parameters are well determined in the present work although the previous microwave and radiofrequency data could not determine all of these constants. This is a result of the accuracy of the present radiofrequency data as well as the tunability of our pump source which allowed selection of a wide range of J and K for the double resonances. Comparison of the observed and calculated radio frequencies in Table 4-1 shows that the quadrupole and spin-rotation parameters in Table 4-3 predict the combined quadrupole-spin-rotation splittings to a few kHz. A comparison of the predicted uncertainties of the microwave and radio frequencies with the observed residuals indicates that the predicted uncertainties are approximately equal to the expected accuracies for resolved transitions by each technique; the standard deviations for an observation of unit weight are all within a factor of 2 of unity. Also, although the previous microwave and radiofrequency data could not determine all of the centrifugal distortion parameters for the quadrupole coupling, these parameters are all well determined in the present work. 161 Table 4-2 Infrared Pumping Frequencies for IR-RF Double Resonance 27 P(27,9) -11 130. 28 P(30,4) -10 167. 29 P(31,9) -11 463. 10P(26) 28 130 035. 10P(28) 28 074 502. 10P(28) 28 073 206. Index8 Transitionb v/Ml-IzC Laserd vP/MHze 1 P(5,1) -12 289.2 10P(16) 28 400 300.5 2 P(5,1) -12 249.3 10P(16) 28 400 340.4 3 P(5,2) -11 466.0 10P(16) 28 401 123.7 4 P(5,2) -11 444.0 10P(16) 28 401 144.9 5 P(7,1) 15 655.5 10P(18) 28 375 429.3 6 P(7,1) 15 678.9 10P(18) 28 375 452.7 7 P(9,1) -9 458.0 10P(18) 28 350 315.8 8 P(10,5) -15 861.2 10P(18) 28 343 912.6 9 P(10,5) -15 878.1 10P(18) 28 343 895.7 10 P(12,5) 12 111.0 10P(20) 28 318 335.9 11 P(12,5) 12 105.8 10P(20) 28 318 330.7 12 P(14,6) -10 919.4 10P(20) 28 295 305.5 13 P(14,6) -10 923.9 10P(20) 28 295 301.0 14 P(15,9) -12 582.9 10P(20) 28 293 642.0 15 P(15,9) -12 596.1 10P(20) 28 293 628.8 16 P(18,4) -14 138.4 10P(22) 28 237 803.3 17 P(18,5) -11 905.3 10P(22) 28 240 036.4 18 P(19,9) -11 659.0 10P(22) 28 240 282.9 19 P(19,9) -11 662.8 10P(22) 28 240 278.9 20 P(22,4) -12 539.3 10P(24) 28 184 383.3 21 P(22,5) -10 395.9 10P(24) 28 186 526.7 22 P(23,9) -11 191.1 10P(24) 28 185 731.5 23 P(23,9) -11 180.3 10P(24) 28 185 742.3 24 R(26,3) -12 825.8 10P(26) 28 128 340.2 25 P(26,4) -11 220.7 10P(26) 28 129 945.3 26 P(27,9) -11 123.1 10P(26) 28 130 042.9 1 9 5 3 8 0 aIndex number in Table 4-1. bVibration-rotation transition pumped for IR-RF double resonance. cMicrowave frequency in MHz; the signed microwave frequency was added to the laser frequency to obtain the pumping frequency. dCO2 laser line used; laser frequencies taken from Ref. 51. ePumping frequency in MHz. 1152 Table 4-3 Quadrupole and Spin-Rotation Interaction Parameters of CD318 v = 0 v2 = 1 Parameter . b c . d .e This Work Wlodarczak This Work Kuczkowski qu/MHz -1 929.008(14) -1 928.918(86) -1 930.886(3l) -l 930.30(26) xJ/KHz -1.098(33) -1.615(19) -1.342(72) xK/KHz -32.86 (40) -8.16(184) -45.81 (88) xD/KHz 19.27 (27) 26.58 (35) CN/KHz -13.64 (6) -14.94 (42) -l4.03 (ll) CK/KHz -9.57 (52) -ll.3 (63) -7.09 (87) 8Values in parentheses are one standard deviation in multiples of the last digit in the parameter. bObtained from a fit of the rotational frequencies of the ground state from the references shown in Table 4-1 and pure quadrupole frequencies in Table III and in Table V of Ref. 39. cObtained from Table VI in Ref. 49. dObtained from a fit of the rotational frequencies of the v2 = 1 state from Table II in Ref. 38 and pure quadrupole frequencies in Table IV. eObtained from Table VIII in Ref. 38. 163 IV-4-2 CD3Br More than 160 IR—RF double resonances have been observed for each of the two naturally-occurring isotopic species of CD Br; it has been 3 possible to measure pure quadrupole frequencies for 10 S J $ 38 and 3 S K S 8. The experimental values of the pure quadrupole frequencies measured in this work are given in Tables 4-4 and 4-5. In each table the v2 = 0 transitions are given on the left side and the v2 = 1 transitions are given on the right side. The pumped vibration-rotation transition is identified by the J,K quantum numbers in the two vibrational states. Since most of the quadrupole splittings in the infrared spectra of CD3Br are within 5 MHz and the Doppler width is ~18.5 MHz, it was not necessary to adjust pump frequencies to observe all of the pure quadrupole transitions for a given infrared transition. Hence, the infrared frequency was set at the center frequency of the Doppler-limited vibration-rotation transition. The infrared frequencies were calculated from the parameters given in Chapter III and the appropriate CO2 laser transition and microwave frequency for the IMSL source were determined from the calculated frequency. The experimental frequencies in Tables 4-4 and 4-5 were fit separately by least squares to differences in energies calculated by diagonalization of Hamiltonian matrices with different parameters for the two isotopic species. The resulting parameters are shown in Tables 4-6 and 4—7 for C0379Br and CD38lBr, respectively. Also shown in Tables 4-6 and 4-7 are the values of qu determined by Marina and Hirose (44). It is seen that the newer values are in good agreement with the less accurate values previously reported. The observed minus calculated frequencies for the parameters 164 Table 4-4 Pure Quadrupole Frequencies of CD3793ra v = 0 v2 = 1 2!“ 2r" v/MHz o—cb 00° J x 21“ 21'" v/MHz o—ob 00c 10 19 17 108.683 9 50 9 17 15 100.987 108 100 21 23 108.517 -62 50 19 21 100.807 -35 100 10 19 17 81.161 -6 50 9 17 15 67.508 170 200 21 23 81.161 10 50 19 21 67.272 ~12? 200 12 23 21 99.742 -10 40 11 21 19 91.853 31 50 25 27 99.568 -55 40 23 25 91.674 -69 50 14 27 25 125.543 -37 50 13 25 23 122.841 35 50 29 31 125.326 -9 40 27 29 122.629 36 50 14 27 25 111.183 -4 20 13 25 23 106.224 -22 30 29 31 110.979 2 20 27 29 106.056 -17 30 14 27 25 92.688 8 30 13 25 23 84.932 -51 30 29 31 92.515 4 30 27 29 84.788 -70 30 15 29 27 55.883 -63 OMIT 31 33 55.888 68 OMIT 15 29 27 28.928 -19 OMIT 31 33 28.928 73 OMIT 16 31 29 118.728 4 20 15 29 27 115.457 -3 20 33 35 118.451 2 20 31 33 115.214 -2 20 16 31 29 104.449 5 20 15 29 27 99.298 -51 30 33 35 104.201 3 20 31 33 99.092 -48 30 18 35 33 123.958 2 10 17 33 31 121.722 15 10 37 39 123.628 3 10 35 37 121.420 16 10 18 35 33 112.606 0 10 17 33 31 109.059 -25 20 37 39 112.297 0 10 35 37 108.784 -22 20 18 35 33 98.737 7 20 17 33 31 98.618 -63 50 37 39 98.453 6 20 35 37 93.372 -59 50 20 39 37 127.736 -2 10 19 37 35 126.154 11 10 41 43 127.355 —2 10 39 41 125.803 15 10 20 39 37 118.501 -0 10 19 37 35 115.977 -12 10 41 43 118.135 -3 10 39 41 115.641 -11 10 20 39 37 107.212 1 20 41 43 106.866 0 20 165 Tdfle 4-4 (cont’d) = 0 v2 = 1 J 21" 21*" mm: o—ch 00° J 21" 21'" was: o-cb 00° 20 39 37 93.888 3 20 19 37 35 88.982 —21 20 41 43 93.542 2 20 39 41 88.873 -19 20 20 39 37 78.458 0 10 41 43 78.152 -5 10 22 43 41 122.907 5 10 21 41 39 121.082 -6 10 45 47 122.489 2 10 43 45 120.874 -4 10 22 43 41 113.537 0 10 21 41 39 110.874 -15 10 45 47 113.138 0 10 43 45 110.503 -13 1o 24 47 45 137.747 -3 20 23 45 43 137.310 -10 50 49 51 137.310 43 20 47 49 138.893 32 30 24 47 45 128.277 2 10 23 45 43 124.912 -5 10 49 51 125.814 2 10 47 49 124.474 —4 10 24 47 45 118.384 0 10 23 45 43 118.397 -11 1o 49 51 117.932 0 10 47 49 115.978 —8 10 24 47 45 109.052 -2 10 23 45 43 108.410 39 10 49 51 108.616 -1 10 47 49 105.995 34 10 28 51 49 138.717 -0 5 25 49 47 138.449 24 10 53 55 138.190 -3 5 51 53 137.947 23 10 26 51 49 134.434 3 10 25 49 47 133.815 -5 20 53 55 133.930 18 20 51 53 133.327 1 10 28 51 49 128.928 9 10 25 49 47 127.892 -14 20 53 55 128.419 9 10 51 53 127.424 3 20 28 51 49 122.180 0 10 25 49 47 120.889 -1 10 53 55 121.875 -6 10 51 53 120.215 0 10 28 51 49 114.210 2 10 25 49 47 112.220 42 30 53 55 113.722 -3 1o 51 53 111.758 42 20 28 55 53 139.483 -12 20 27 53 51 139.325 17 30 57 59 138.923 -6 20 55 57 138.783 17 30 28 55 53 135.773 -20 30 27 53 51 135.347 -8 50 57 59 135.229 -3 30 55 57 134.848 28 30 28 55 53 131.029 -2 10 27 53 51 130.255 -23 1o 57 59 130.485 7 10 55 57 129.745 -3 10 30 59 57 138.910 10 30 29 57 55 138.809 10 10 81 83 138.291 -6 3o 59 81 138.011 -9 10 166 Table 4-4 (cont'd) v = 0 v2 = 1 J 8 2r' 2F" v/MHz o—cb 00° J x 27' 2t" v/an o—cb 00 30 59 57 132.724 ~23 3o 29 57 55 132.221 28 20 81 83 132.128 ~24 20 59 81 131.837 18 40 30 59 57 127.870 0 10 29 57 55 128.811 ~9 10 81 83 127.078 ~2 10 59 81 128.240 ~14 10 32 83 81 129.888 ~28 3o 31 81 59 129.097 35 50 85 87 128.984 ~78 80 83 85 128.455 3 40 34 8 87 85 131.389 ~13 20 33 8 85 83 130.883 ~42 50 89 71 130.721 18 40 87 89 130.259 ~13 30 35 8 89 87 132.128 5 20 34 8 87 85 131.719 ~23 4o 71 73 131.432 8 30 89 71 131.040 ~27 20 .Obtsined by infrared radiofrequency double resonance. The infrared transition was between the J and K values across from each other in the left and right halves of the table. For example, the infrared transition for the first four double resonances was from (J,K) = (10.3) in v = 0 to (J,K) = (9,3) in V: = 1. The infrared frequency used was the center frequency of the Doppler-limited transition, as calculated from the parameters in Table 3-8. bObserved minus calculated frequency in kHz. The parameters for the calculation are in Tables 4-6 and 3-8. cEstimated uncertainty in the observed frequency in kHz. An ”OMIT” means that the frequency was omitted from the least squares fits. Pure Quadrupole Frequencies of 003 Br 167 Table 4-5 81 = 0 v2 = 1 J 21" 21'” v/MHz o-cb 00° J 21" 21m o/mz o-cb 00° 12 23 21 111.089 ~28 4o 11 21 19 109.548 33 40 25 27 110.854 ~13 30 23 25 109.322 28 40 12 23 21 99.547 ~8 20 11 21 19 95.872 18 30 25 27 99.323 ~9 20 23 25 95.887 0 30 14 27 25 104.945 9 20 13 25 23 102.833 ~25 20 29 31 104.889 14 20 27 29 102.395 ~10 20 14 27 25 92.890 ~27 30 13 25 23 88.839 40 40 29 31 92.822 ~38 30 27 29 88.579 12 40 14 27 25 77.488 9 30 13 25 23 71.005 44 40 29 31 77.221 -4 30 27 29 70.787 35 40 18 31 29 108.499 11 20 15 29 27 108.992 ~18 30 33 35 108.181 7 30 31 33 108.892 ~9 20 18 31 29 99.228 13 50 15 29 27 98.518 4 20 33 35 98.913 18 50 31 33 98.239 19 20 18 31 29 87.274 ~14 30 15 29 27 83.029 22 30 33 35 88.988 ~3 30 31 33 82.750 22 30 18 35 33 110.959 2 10 17 33 31 109.977 18 10 37 39 110.572 ~2 10 35 37 109.810 4 10 18 35 33 103.585 ~3 20 17 33 31 101.718 ~28 30 37 39 103.223 7 30 35 37 101.381 ~18 10 18 35 33 94.123 14 3o 17 33 31 91.120 ~48 50 37 39 93.788 17 30 35 37 90.818 ~12 20 20 39 37 112.742 ~2 10 19 37 35 112.089 8 20 41 43 112.322 8 10 39 41 111.889 9 10 20 39 37 108.755 8 10 19 37 35 105.444 ~13 20 41 43 108.329 1 10 39 41 105.047 ~14 10 22 43 41 117.840 8 5o 21 41 39 117.514 34 50 45 47 117.187 15 40 43 45 117.054 22 30 22 43 41 114.087 ~15 10 21 41 39 113.881 50 20 45 47 113.570 ~37 10 43 45 113.192 28 20 22 43 41 109.118 5 10 21 41 39 108.175 ~15 10 45 47 108.848 8 10 43 45 107.735 ~12 10 168 Table 4-5 (cont’d) :0 V231 J 2r' 2F” v/an o-cb 00° J 2F' 2F” v/an o—cb 00° 22 43 41 102.715 0 20 21 41 39 101.190 ~22 3o 45 47 102.225 ~30 20 43 45 100.750 ~23 20 24 47 45 115.118 8 10 23 45 43 114.799 9 10 49 51 114.591 0 1o 47 49 114.307 8 10 24 47 45 110.923 0 10 23 45 43 110.237 ~28 10 49 51 110.427 19 10 47 49 109.771 ~5 10 24 47 45 105.539 4 1o 23 45 43 104.419 ~17 10 49 51 105.032 8 10 47 49 103.931 ~20 10 24 47 45 98.948 1 1o 23 45 43 97.310 7 20 49 51 98.443 ~1 10 47 49 98.830 10 10 28 51 49 115.932 10 20 25 49 47 115.727 18 20 53 55 115.373 18 20 51 53 115.191 12 20 28 51 49 112.354 8 30 25 49 47 111.878 0 20 53 55 111.805 20 30 51 53 111.327 ~18 20 28 55 53 118.588 14 40 27 53 51 118.457 11 20 57 59 115.970 7 50 55 57 115.884 ~8 20 31 81 59 111.578 11 20 30 59 57 111.211 ~3 20 83 85 110.885 ~11 20 81 83 110.558 ~19 20 31 81 59 107.548 ~48 50 30 59 57 107.003 -16 20 83 85 108.883 ~47 50 81 83 108.398 17 20 33 85 83 109.122 ~17 20 32 83 81 108.720 -7 20 87 89 108.424 -4 20 85 57 108.041 ~3 20 34 87 85 105.895 ~13 30 33 65 83 105.400 28 20 89 71 105.170 ~8 30 87 89 104.714 48 20 38 71 89 107.508 ~13 20 35 89 87 107.188 21 20 73 75 108.738 -8 20 71 73 108.418 21 20 38 75 73 108.888 0 3o 37 73 71 108.835 ~11 20 77 79 108.089 20 20 75 77 107.854 0 20 169 Table 4—5 (cont’d) IObtained by infrared radiofrequency double resonance. The infrared transition was between the J and K values across from each other in the left and right halves of the table. bObserved minus calculated frequency in kHz. The parameters for the calculation are in Tables 4-7 and 3-9. cBatimated uncertainty in the observed frequency in kHz. An "OMIT” means that the frequency was omitted from the least squares fits. 1370 Table 4-6 Quadrupole and Spin-Rotation Interaction Parameters of CD37gBr v = 0 v2 = 1 Parameter This Harka Morino & Hiroseb This Workc Merino & Hiroseb qu/MHz 575.718(35)‘l 575.4(10) 575.811(41) 578.2(10) xJ/kHz 0.224(53) 0.946(74) xK/kHz 14.75(l32) 26.01(243) xD/kHz 4.19(154) -52.76(402) CN/kflz -10.02(15) -10.00(22) Cx/kHz -9.12(259) -9.04(391) .Obtained from a fit of the pure quadrupole frequencies in Table 4-4 and the rotational frequencies for the ground state reported in Refs. 43 and 44. bRef. g. cbbtained from a fit of the pure quadrupole frequencies in Table 4-4 and the rotational frequencies for the v2 = 1 state reported in Ref. 44. dValues in parentheses are one standard deviation in multiples of the last digit in the parameter. 171. Table 4-7 Quadrupole and Spin-Rotation Interaction Parameters of CD3alBr v = 0 v2 = 1 Parameter This Worka Morino & Hiroseb This Workc Morino & Hiroseb can/1012 480.922(24)d 479.5(10) 481.206(25) 478.5(10) xJ/kHz 0.064(56) 0.480(64) xK/kHz 14.73(127) 35.15(153) xD/sz 0.e 0.° CN/kHz -10.75(22) -10.45(25) Cx/kHz -11.12(588) -17.61(612) .Obtained from a fit of the pure quadrupole frequencies in Table 4-5 and the rotational frequencies for the ground state reported in Ref. 44. bRef. 44 cObtained from a fit of the pure quadrupole frequencies in Table 4-5 and the rotational frequencies for the v2 = 1 state reported in Ref. 44. dValues in parentheses are one standard deviation in multiples of the last digit in the parameter. eConstrained to zero. 172 in Tables 4-6 and 4-7 are shown in Tables 4-4 and 4-5, respectively, where it is seen that the theoretical frequencies agree with the experimental values for well—resolved transitions to within the experimental uncertainty. Examination of the centrifugal distortion terms for the quadrupole coupling (Tables 4-6 and 4-7) shows that both xJ and XD are quite small in the ground state. The residual for xD for CD381Br was larger than the value obtained, and it was therefore constrained to zero. The centrifugal distortion terms for the quadrupole coupling in v2 = l are larger than in the ground state for both species. This may be the result of the Coriolis interaction between the v2 = l and v5 = 1 states (48), which should lead to some sharing of quadrupole effects between the two vibrational states. Since this is a Coriolis interaction involving states of A and E symmetry, the coupled levels differ by 11 in k. Therefore, even if the quadrupole coupling is very similar in the two vibrational states, an effect of the mixing is expected. The result is that caution should be used in interpretation of the vibrational dependence of the quadrupole parameters. Since the values of qu obtained are quite precise, it is expected that the ratio of these values should be nearly equal to the ratio of the quadrupole moments of the two bromine isotopes. The experimental 7 81Br) obtained in the present work for the value of qu(CD3 9Br)/qu(CD3 ground vibrational state is 1.197ll(9), which is the same within our experimental error as the molecular beam values of 1.1971005(24) for LiBr (49) and 1.1970568(15) for atomic bromine (59). The corresponding ratio obtained by us for v2 = l in CD3Br is 1.19660(9). The difference 173 between this value and that for the ground vibrational state may result from the effect of the Coriolis coupling. As stated before, it has been found that some effect was causing an apparent shift of the transitions especially at low RF frequencies. In contrast to the residuals shown in Tables 4-4 and 4-5, the observed- minus- calculated frequencies for the low radiofrequency transitions shown in Tables 4-8 and 4-9 are often greater than the experimental uncertainty and nearly always the same sign for a given vibrational state; the residuals for v2 = 0 are positive while the residuals for v2 = l are negative. The reason has been traced to the result of a four— interacting-level double—resonance effect that causes the lower frequency transition of a pair to be shifted to higher frequency while the higher frequency component is shifted to lower frequency. In fact, the same effect has been observed in low frequency quadrupole transitions of CD31, however, it is much more serious in CD3Br since the transitions are located much closer (within 1 MHz). The details are discussed in the next chapter. Since the low frequency transitions were most strongly affected by the four-interacting-level double resonance effect, they have been omitted from the least squares fittings. V-4-3 Other Aspects This is the first systematic application of an infrared microwave sideband laser system to the use of IR-RF double resonance for studying quadrupole transitions; previous studies of a few rotational transitions in 0804 and SiH4 have been reported (39,31). Some unresolved questions 174 Table 4-8 - _ . . 79 a F~J+l/2 ~ F-J-1/2 transitions of CD3 Br v = 0 v2 = l J x 21" 21'" v/MHz 0—0b 00° J 11 21" 2F” mm: 0-0" 00° 10 3 21 19 15.834 95 50 9 3 19 17 16.110 -76 50 14 3 29 27 13.225 81 60 13 3 27 25 13.741 -62 60 16 4 33 31 11.047 89 100 15 4 31 29 11.283 -55 100 18 4 37 35 10.292 71 30 17 4 35 33 10.545 -53 30 18 5 37 35 9 362 51 60 17 5 35 33 9.512 -17 60 20 5 41 39 8.915 54 60 19 5 39 37 9.067 ~40 60 20 6 41 39 8.036 -8 100 19 6 39 37 8.142 -23 100 19 8 39 37 5.744 -26 30 22 5 45 43 8.446 49 40 21 5 43 41 8.608 -35 40 22 6 45 43 7.820 41 20 21 6 43 41 7.922 -19 20 24 3 49 47 8.686 42 30 23 3 47 45 8.984 -31 30 24 6 49 47 7.513 40 40 23 6 47 45 7.625 -22 40 24 7 49 47 6.930 22 160 23 7 47 45 7.019 5 160 26 2 53 51 8.294 41 30 25 2 51 49 8.524 -28 30 26 3 53 51 8.129 39 30 25 3 51 49 8.331 -20 30 26 4 53 51 7.889 47 30 25 4 51 49 8.060 -34 30 26 5 53 51 7 587 53 60 25 5 51 49 7.722 -29 60 26 6 53 51 7.175 18 80 25 6 51 49 7.292 -40 80 28 2 57 55 7.768 37 20 27 2 55 53 7.954 -34 20 28 3 57 55 7.630 39 30 27 3 55 53 7.797 -39 30 28 4 57 55 7.445 46 60 27 4 55 53 7.588 -36 60 28 5 57 55 7.188 37 40 27 5 55 53 7.325 -25 40 30 4 61 59 7.039 35 50 29 4 59 57 7.172 -34 50 30 5 61 59 6.847 45 50 29 5 59 57 6.973 -12 50 30 6 61 59 6.590 35 50 29 6 59 57 6.704 -11 50 34 6 69 67 6.047 20 70 33 6 67 65 ' 6.153 -13 70 35 6 71 69 5.943 35 50 .Obtained by infrared radiofrequency double resonance. The infrared transition was between the J and K values across from each other in the left and right halves of the table. bObserved minus calculated frequency in kHz. The parameters for the calculation are in Tables 4-6 and 3-8. cEstimated uncertainty in the observed frequency in kHz. 175 Table 4-9 F=J+l/2 . F=J-1/2 transitions of CD Br J K 2F' 2F" v/MHz 0—0 00 J K 2F' 2F" v/Mflz O-Cb DC 12 2 25 23 13.591 94 50 11 2 23 21 14.383 -75 50 12 3 25 23 12.212 93 40 11 3 23 21 12.607 -82 40 16 3 33 31 10.147 114 100 15 3 31 29 10.437 -84 100 16 4 33 31 9.282 84 60 15 4 31 29 9.506 -11 60 18 3 37 35 9.272 93 40 17 3 35 33 9.537 -62 40 20 3 41 39 8.523 76 30 19 3 39 37 8.755 -52 30 20 4 41 39 8.062 48 50 19 4 39 37 8.248 -59 50 22 3 45 43 7.878 57 50 21 3 43 41 8.082 -47 50 22 4 45 43 7.569 75 50 21 4 43 41 7.708 -49 50 22 5 45 43 7.147 75 50 21 5 43 41 7.259 -20 50 24 3 49 47 7.333 50 50 23 3 47 45 7.510 -38 50 24 4 49 47 7.074 44 50 23 4 47 45 7.218 -46 50 24 5 49 47 6.753 49 50 23 5 47 45 6.888 -11 50 24 6 49 47 6.341 36 50 23 6 47 45 6.480 28 50 26 3 53 51 6.872 55 30 25 3 51 49 7.026 -21 30 26 4 53 51 6.665 48 50 25 4 51 49 6.798 -28 50 28 3 57 55 6.472 60 50 27 3 55 53 6.606 -6 50 30 7 61 59 5.349 40 50 31 5 63 61 5.647 22 60 30 5 61 59 5.792 25 60 31 6 63 61 5.456 18 100 30 -6 61 59 5.616 50 100 33 6 67 65 5.248 26 50 32 6 65 63 5.405 65 50 .Obtained by infrared radiofrequency double resonance. The infrared transition was between the J and K values across from each other in the left and right halves of the table. bObserved minus calculated frequency in kHz. The parameters for the calculation are in Tables 4-7 and 3~9. cEstimated uncertainty in the observed frequency in kHz. 176 have arisen as a result of this work. For example, the narrowest lines that we have obtained have a half width at half height of ~70 kHz for CD31 and ~100 kHz for CD3Br. We have not yet analyzed sources of the broadening, although the most likely candidates are some combination of RF power broadening, beam transit time broadening, and pressure broadening. It is also necessary to investigate the effect of the nuclear quadrupole coupling of the deuterium nuclei in these molecules, which could give additional linebroadening; however, further study may require more theoretical development for the effect of interaction of quadrupoles between different nuclei. In order to analyze the source of line-broadening, CH3I is a very good candidate since the molecule provides a strong vibrational band (02) in 002 laser region (3), and is free from the perturbation of deuterium nuclei. A second unresolved question is the source of the many weak satellite lines that accompany the RF transitions. These could be the result of collisional double resonance (3,43), but have not yet been assigned. Probing the intensity and the frequencies of the satellite lines may also shed additional light on energy transfer between rotational levels as well as uusual double resonance effects. _An additional interesting subject for future work is observation of Al-A2 splittings in the v5 doubly-degenerate vibrational bands of CD3I and CD3Br. Pure quadrupole transitions of k = 1 = :1 states are not allowed due to the single parity of the hyperfine levels, however, Al-A2 transitions are allowed for all of the quadrupole components by the opposite parity and may provide further information about the Coriolis interaction between the v2 and the 05 vibrational states. 177 IV-5 Appendix For a symmetric top molecule the principal axes of the quadrupole coupling tensor x lie along the principal inertial axes of the molecule. Also, x Therefore, for xq, only x020, and the only non-zero xx-xyy' matrix elements of the quadrupole interaction are as follows: = 3- _ e1[3k J(J+l)]xzz (4 Al) —3e2k[(J+l)2-k2]1/2x 22 (4—A2) = 3e3[(J+l)2-k2)((J+2)2-k2)]1/2xzz (4—13) The abbreviations are e1: [3G(G+l)/4-I(I+1)J(J+l)]/2I(21-1)J(J+l)(2J-1)(2J+l), (4-A4) G = F(F+l)—I(I+1)—J(J+1), (4—A5) [F(F+1)-I(I+1)—J(J+2)][(F+I+J+2) -(J+I-F+l)(F+J—I+l)(F+I-J)/(2J+l)(2J+3)]1/2 e = 2 8I(2I-1)J(J+1)(J+2) ’ (4‘A6) [(F+I+J+2)(F+I+J+3)(I—F+J+1)(I-F+J+2) e3 = -(F—I+J+l)(F-I+J+2)(F+I-J-1)(F+I—J)]1/2 (4-47) 16I(2I-1)(J+1)(J+2)(2J+3)[(2J+1)(2J+5)]1/2 ’ xzz is equal to qu for a symmetric-top molecule. 178 IV-6 References M 10. ll. 12. l3. 14. 15. 16. 17. 18. 19. . S. H. Autler and C. H. Townes, Phys. Rev. 100, 703-722 (1955). . F. J. Wodarczyk and E. B. Wilson, J. Mol. Spectrosc. 37, 445-463 (1971). . F. Shimizu, Chem. Phys. Lett. 17, 620-622 (1972). . R. F. Curl, Jr., T. Oka, and D. S. Smith, J. Mol. Spectrosc. 46, 518-520 (1973). . R. F. 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Joerissen, W. A. Kreiner, Y. T. Chen, and T. Oka, J. Mol. Spectrosc. 120, 233-235 (1986). R. L. DeLeon, P. H. Jones, and J. S. Muenter, Appl. Opt. 20, 525-527 (1981). C. Pursell, W. C. Ho, F. Scappini, and T. Oka, J. Mol. Spectrosc., 131, 241-249 (1988). G. Magerl, W. Schupita, and E. Bonek, IEEE J. Quantum Electron. QB- 18, 1214—1220 (1982). J. W. Simona, Phys. Rev. 76, 686 (1949). J. W. Simmons and J. H. Goldstein, J. Chem. Phys. 20, 122-124 (1952). A. K. Garrison, J. W. Simmons, and C. Alexander, J. Chem. Phys. 45, 413-415 (1966). R. L. Kuczkowski, J. Mol. Spectrosc. 45, 261-270 (1973). J. Demaison, D. Boucher, G. Piau, and P. Glorieux, J. Mol. Spectrosc. 107, 108-118 (1984). G. Wlodarczak, D. Boucher, R. Bocquet, and J. Demaison, J. Mol. Spectrosc. 124, 53-65 (1987). 41. 42. 43. 44. 45. 46. 47. 48. 49. 50. 51. 180 S. A. Rackley and R. J. Butcher, Mol. Phys. 39, 1265-1272 (1980). W. Schrepp and H. Dreizler, Z. Naturforsch. 36a, 654-661 (1981). A. K. Garrison, J. W. Simmons, and C. Alexander, J. Chem. Phys. 45, 413-415 (1966). Y. Morino and C. Hirose, J. Mol. Spectrosc. 24, 204-224 (1967). A. R. Edmonds, "Angular Momentum in Quantum Mechnics," McGrawrflill, New York, 1955. H. P. Benz, A. Bauder, and Hs. H. Gunthard, J. Mol. Spectrosc. 21, 156-164 (1966). H. Dreizler, W. Schrepp, and R. Schwarz, Z. Naturforsch. A34, 571- 574 (1979). K. Harada, K. Tanaka, and T. Tanaka, J. Mol. Spectrosc. 98, 349—374 (1983). R. C. Hilborn, T. F. Gallagher, Jr., and N. F. Ramsey, J. Chem. Phys. 56, 855-81 (1972). H. H. Brown and J. G. King, Phys. Rev. 142, 53-59 (1966). C. Freed, L. C. Bradley, and R. G. O’Donnell, IEEE J. Quantum Electron. QE-16, 1195-1206 (1980). CHAPTER V FOUR-INTERACTING-LEVEL DOUBLE RESONANCE V-l Introduction As mentioned in the previous chapter, the preliminary fittings of the pure quadrupole transitions of CD3Br revealed some problem with the low-frequency RF spectra. The nature of the problem may be seen by reference to the energy-level diagram in Fig. 5-1, which shows a typical hyperfine pattern for a single J and k in the ground vibrational state coupled by the infrared radiation to a typical hyperfine pattern for J' and k' in the v2 = 1 state. It may be seen that the allowed RF transitions include two transitions of relatively high frequency and one transition of relatively low frequency for each of the two vibrational states. Because the hyperfine splittings in the upper state are not greatly different from those in the lower state for the double resonances in this work and because of the near symmetry of the patterns, the four upper frequencies are comparable and the two lower frequencies are comparable. Generally, the two lower frequencies are more severely overlapped than the higher frequencies. Finally, each pair of comparable frequencies has an energy level pattern similar to that shown in Fig. 5-2, in which it may be seen that both the upper and lower states of both RF transitions are pumped by the infrared radiation. The least squares adjustment of the hyperfine constants to fit the experimental frequencies showed that the experimental values for 181 182 Rodlof‘requency Tronsltlons J’+1/2 TI; J’-1/2 L.“ J’+3/2 *3 J’-3/2 )F Infrared 4+ Transltlons .. f J+1/2 / W: J-1/2 J,K 6.8. 4"- J-3/2 Figure 5-1. Typical energy level pattern for the infrared radiofrequency double resonance observed for CD3Br. A single infrared frequency pumps all of the allowed infrared transitions by interacting with molecules in different velocity groups. In general, four high- frequency and two low-frequency double resonances were observed for each infrared transition. 183 Figure 5—2. Energy level diagram for the four-interacting~level double resonance system. 184 the two lowest radiofrequency transitions were too close together; the lower frequency of the pair almost always showed a positive residual (observed - calculated) while the upper frequency showed a negative residual. This was finally traced to a double-resonance effect that appears to be unique to an energy-level pattern like that in Fig. 5-2, a pattern that we refer to as a "four-interacting-level double resonance". Double resonance for the four-level system in Fig. 5-2 has been treated by Small gt El. (1), but in their case the millimeter wave frequency (corresponding in our case to the IR frequency) was scanned while the RF was fixed. In our study, it has been found that the magnitude of the shift in frequencies depends on the difference in frequency of the two overlapped lines, the Rabi frequencies for the IR and RF radiation, and the pressure broadening. 185 V—2 Theory The purpose of this section is to describe the density matrix treatment used to calculate the lineshape of the double-resonance spectra obtained for the case of four interacting levels. The energy levels and allowed transitions for the four levels are shown in Fig. 5- 2. The procedure followed is to set up and solve numerically the density matrix equations for the four levels in the presence of two radiation fields. The equations are solved for a sequence of values for the component of the velocity in the direction of the two beams and the resulting lineshapes are weighted by the appropriate Boltzmann factor and summed. Only the infrared frequencies are assumed to be affected by the Doppler averaging, since the Doppler shifts at the radiofrequencies involved are much smaller than the Lorentz widths of the double resonances. The density matrix equation is as follows: $3; = -% [H.p] - K (p - 0°) . (5-1) Here, 9 is the density matrix, p0 is the density matrix at thermal equilibrium, and K is a supermatrix of relaxation coefficients. The Hamiltonian H is in two parts, H = 11(0) + 11(1) , (5-2) in which R(o) is the Hamiltonian for the rovibrational energy including the quadrupole coupling, and R(l) describes the interaction with the two 186 (1) radiation fields. A matrix element of H is 3(1) = R(1)= — p (2 cos 2wv t + 2 cos 2nv t) (5—3) ij kj Jk l l 2 2 ' In this expression, £1 and £2 are the peak electric fields and v1 and v2 are the frequencies of the laser and radiofrequency fields, respectively; 1t 18 assumed that v1 = vL-kv1 ~ EC-Ea ~ Ed-Eb and v2 ~ v1 u Eb—Ea ~ Ed—EC in which the E3 are eigenvalues of R(o) for the energy levels shown in Fig. 5—2, v the infrared laser frequency, k = (vL/c) L and v is the component of molecular velocity in the direction of the beam; Doppler effects are assumed to be negligible at the radiofrequency v 0f the dipole transition moments, we assume that ”ba’ pea, ”db’ and R' “dc are all real and are the only non-zero elements. For the four levels in Fig. 5-2, the density matrix contains 4 real diagonal elements and 6 complex elements above the diagonal that are complex conjugates of the elements below the diagonal as follows; +22>+..+..+22 +..+22 -+..++.. 5bb=‘(i/m(“t(aWpab+fltg+11)°db‘°bang)‘°bd db)) kbbApbb (5’5) .. ++22+..+..+22 ++.. +—22> +..++.. pdd i_(1/fi)(R(1)pbd+ndi)pcd_pdbubd ‘pch Héd))-kddApdd (5‘7) _- (1)H(1)(1) _ a(i/m(fiba)p aa +1'lbd pda_pbcH ca -pbeba ) (ivba+ kba)pba (5 8) ' -_ + (1)‘J H(1) ”(1) (1) pca- (l/h)(ncap aa+ Hcd pda_pccH ca chnba ) (ivca+ kca)pca (5-9) +11(1)p Ha) __ . (1) <1) __ _ pda- (I/fi)(Hdb 0be do pHca-pdc ca _pdeba ) (ivda+ kda)pda (5 10) 187 __ (1)p (1) (1)1(1) . _ (i/fi)(Hc pab +Had pdb-pcanab Tcdndb ) (lvcb+kcb)pcb (5 11) _ (1) M(1) (1) H(1) _ pdb (1/H)(H& ”be dc ”cb’pdaHab pddH db ) (lvdb+kdb)pdb (5 12) __ - (1) (1) (1) (1) _ ”dc‘ (l/H)(Hdb pbc Hdc pcc ”daHac pddec ) (1”d ckdc)pdc ' (5 13) To write Eq. (5-4) to (5-13), the relaxation supermatrix K has been assumed to have a particularly simple form. In preparation for using the rotating-wave approximation, which assumes that the oscillating electric field of the radiation is too fast to be detected by experimental apparatus, we make the following substitution for the off-diagonal elements of p: pjk Ejkexp(-2nivnt) . (5—14) Here, ”n is v2, v1, v1+v2, vl-vz, v1, and v2 for jk 3 ba, cs, da, cb, db, and dc, respectively. After this substitution and elimination of common factors of exp(-2nivnt) , all terms that oscillate at radiofrequencies or higher are eliminated. The resulting equations are; paa:(i/z)[x2(dba_dab)+xl(dca-dac)1—kaaApaa (5‘15) pbb=(i/2)[x2(dab- dba )+x3(ddb- dbd)]k bbApbb (5-16) pmin/2)["1(dac‘dca)+"4(ddc‘d cd)] kccAp cc (5‘17) Hdd:(i/z)[x3(dbd-ddb)+x4(dcd-ddc)]_kddApdd (5'18) pba:(isba-kba)dba+(i/2)[x2(pas-pbb)+x3dda_xldbc)1 (5-19) 188 Sca:(isca-kca)dca+(i/2)[x1(pas—pcc)+x4dda—x2dcb)] (5-20) gda:(isda_kda)dda+(i/2)[x3pba+x4pca)_xlddc-xzddb)1 (5‘21) Hdb:(isdb‘kdb)ddb+(i/2)[x3(pbb‘pdd)+x4dcb'x2dda)1 (5‘22) Sdc:(isdc—kdc)dba+(i/z)[x3dbc+x4(pcc_pdd)—xldda)1 (5'23) Scb:(iscb-kcb)dcb+(i/2)[leab+x4pdb_x2dca—x3dcd)1 ° (5‘24) In these equations, the non-oscillating part of each off-diagonal element (Ejk) has been represented by pjk: d. Jk + 1 d3 (5-25) k 9 where dsk’ and dgk are real numbers that account the real and imaginary parts of the off-diagonal element. There are, therefore, 16 real numbers that must be specified to define the density matrix. It is possible to write the 4 diagonal elements and the 6 real and 6 imaginary parts of the off-diagonal elements as a column matrix, in which case the supermatrix K in Eq. (5-1) becomes an ordinary two-dimensional matrix, which is diagonal for the form of the relaxation elements in Eq. (5-15) - (5-24). For simplicity, we have made the further assumption that the diagonal elements are kd and k0 for the relaxation rates for the diagonal and off-diagonal elements of p, respectively. For the calculations here, it was further assumed that kd = k0. The next step is to make the steady-state approximation in which the time derivatives of the pjj’s and the djk’s are set equal to zero. The result is a 189 linear system, as follows: A D = B (5-26) in which D is a vector of the diagonal elements of the density matrix and the real and imaginary parts of the pjk' The order of the elements in D is such that the transposes of D and B are “muumuuuuumumuuuuw 0 O c O 0 Odd 0 0 0 0 0 0 ) . (5-28) __ 0 O ' Hd (pan 0 ° pbb ° ° ”c Finally, the matrix A is the following: r-kd 0 -x2 0 0 -x1 0 o o o o o o o o o 7 2 0 -ko -s o o o o o o o o o o -x1/2 o -x3/2' x2/2 52 -k -x2/2 o o o o o o o o -x1/2 o x3/2 o f 3 o 0 x2 -kd o o o 0 -x3 0 o o o o o o i i o o o 0 -ko ‘51 o o o o o o o xz/Z o - 4/22 éxl/z o o o 51 -k -x1/2 o o o o o -x2/2 o x4/2 o i i o o o o 0 x1 -kd o o o 0 -x4 0 o o o t A = g o o o o o o 0 -ko -53 o o o o -x4/2 o xz/zg o o o x3/2 o o o 53 -k -x3/2 o o x4/2 o -x2/2 o f o o o o o o o 0 x3 -kd 0 x4 0 o o o E o o o o o o o o o 0 -ko -s4 0 x3/2 o xl/Zé . 0 0 0 0 0 0 x4/2 0 0 -x4/2 64 -k0 x3/2 0 -x1/2 0 i i o o x1/2 o o x2/2 o o -x4/2 o o -x3/2 ~20 ‘2'51 0 o I 2 o x1/2 o o -x /2 o o x4/2 o o -x3/2 0 51“2 -k° o o i o o -x3/2 o o -x4/2 o o x2/2 o o xl/Z o 0 -ko ‘52'53 \o x3/2 o o x4/2 o o -x2/2 o o -xl/2 o o o 52+53 -k° J (5-29) 190 In the matrix, x1 = ucafil/h, x2 = ubaSZ/h, x3 = udbEI/h, and x4 = “chZ/h' Also, 61 = v1(l—v/c) - vca’ 62 = v2 — vba’ 63 = v1(1-v/c) - vdb’ and 64 = 02 - vdc' In these equations v is the component of the molecular velocity in the direction of the laser beam, c is the speed of light, and vjk = (Ej - Ek)/h' In order to calculate the spectrum, the linear system is solved for a fixed value of the laser frequency, v1, and sequences of values of the velocity component v and the RF frequency v2. For each of these solutions, the contribution to a quantity a, which is proportional to the absorption of the laser radiation, is calculated as a = x1 dga + x d . (5-30) 3 db This equation is set by the fact that the infrared absorption is proportional to the product of the Rabi—frequency (xi) and the imaginary part of the corresponding off-diagonal element of the density matrix. The calculation is repeated for x2 = x4 = 0 in which case Eq. (5-26) becomes a 6x6 linear system since the hyperfine levels are not connected any more. It is then possible to derive an analytical expression for a, as follows: 191 .. no ”0 “o- xldca + x3d'db k k l o 2 2 2 2 o 2 2 2 E E; { x1D1[(53+Ho)+"3 E'] + X1D3(53+Ho) k 2 2 2 2 o 2 2 2 +x393[(51+ko)+x1 kd] + X3D1(61+ko)} : k k 9 (5-31) 2 2 2 o 2 2 2 o 2 2 2 2 {[(61+k0)+x1 E;][(63+k0)+x3 EEJ-(63+k0)(61+k0) where D1 3 p28 - 02c and D3 = pgb - p§d° The intensities of the double- resonance spectra are then proportional to the differences, An = a — do. The values of Am for the v values for a given v2 are multiplied by the Boltzmann weight factor exp(-v2/uz) and summed. Here, u2 = 2kBT/m where RE is the Boltzmann constant and m is the molecular mass. For the numerical integration, it is necessary to insure that the interval in v is sufficiently small and that the range of v includes the important contributions to the integral. It has been found that the interval in vlv/c must be smaller than the smaller of kd or ko and that the range of vlv/c must include at least several times the larger of kd or R0 on either side of the v values for the resonant velocity groups (there are in general two resonant values of v in the four-interacting-level case). 192 V-3 Results and Discussion The effect of the four-interacting—level double-resonance was discovered by calculating the lineshape for a selected doublet by means of Eq. (5-9) under conditions as close as could be estimated to the experimental conditions. An example of the comparison of observed and calculated lineshapes is shown in Fig. 5-3. The conditions used for the calculation are given in the caption for the figure. We have no value for the transition moment for the infrared transition and could only estimate the Rabi frequency to be about 20 kHz by assuming 0.01 Debye as the transition dipole moment (2,§). The Rabi frequency for the radiofrequency transition was calculated from the measured value of the amplitude of the RF field and the known permanent dipole moment for CD38r (1.83 D (4)) by using the dipole moment matrix elements given by Benz gt g1. (Q). The only questionable point in this calculation is the method used to average over the spatial degeneracy. We used an average over the m states weighted by the expected intensity of the double resonance and obtained values of 5-80 kHz for the various transitions. Also needed for the double resonance calculation are the effective relaxation parameters; we used the halfwidth at half-maximum for the double resonances, 100 kHz. The observed and calculated lineshapes in Fig. 5—3 were each fit by least squares to a sum of two Lorentz functions and the resulting residuals are plotted below each line. The agreement between the two plots of the residuals in both appearance and magnitude provides strong confirmation of the proposed four-interacting-level double resonance effect. If conventional 3—level double resonance equations (3,6) are 193 Figure 5-3. Comparison of observed and calculated infrared radiofrequency double resonance spectra for a four-interacting-level double resonance system. The upper trace is the calculated spectrum and the lower trace is the observed spectrum. The points below each trace are the residuals obtained when the lineshape is fitted by least squares to a sum of two Lorentz lineshapes. The experimental spectrum was observed with a sample pressure of 4 mTorr, infrared power ~2 mW, and radiofrequency power ~20 mW. The theoretical spectrum was calculated by means of Equation (5-26) with all xi = 20 kHz and with kd 3 k0 = 100 kHz. For the experimental spectrum, the infrared frequency was set at the center frequency of the Doppler-limited lineshape of the P(26,4) transition in the v2 band of CD37QBr; the 10R(22) 1201502 laser was used with the lower frequency sideband generated by a microwave frequency of 12632 MHz. Intensity (orb. units) 194 95 r l ' 79P(26.4) 75- l 55- " Wfiffififlw 35- " 154 H -5- " -25- r-53/2-51/2 F-51/2-49/2 _ —45 I I ' 7.0 7.5 8.0 8.5 9.0 Frequency (MHz) 195 used to calculate the spectra, it is found for the conditions in this work that the lineshapes are almost perfect Lorentz functions centered at the predicted frequency. The two Lorentz functions obtained from the fitting of the calculated lineshape in Fig. 5—3 are each shifted by 40 kHz from their expected value; the lower frequency transition is shifted to higher frequency and vice-versa. Examination of the residuals in Tables 4-8 and 4-9 shows that 40 kHz is of the correct order of magnitude to explain the observed frequency shifts. After discovering this effect, the next question was whether there was a corresponding shift in frequency for the other double resonances, because, as mentioned above, both the upper and lower levels of every RF transition are pumped. Such a difficulty did not seem probable because the residuals for the high-frequency double resonances were much smaller than for the low-frequency transitions, even when the low-frequency transitions were included in the fit. Nevertheless, a series of lineshape calculations have been carried out with 20 kHz for Rabi frequencies, with 100 kHz for the Lorentz widths, and with varying values of the separation in frequency of the two double-resonance transitions. The computed lineshapes were fit to a sum of two Lorentz functions and the difference between the center frequency of the lower frequency Lorentz component and the expected value is plotted in Fig. 5- 4 as a function of the separation of the two peaks. It may be seen that the shift ranges from about 45 kHz for a separation of 0.3 MHz to less than 5 kHz for separations greater than 4 MHz. These values were surprising to us in view of the rather small Rabi frequencies involved. A final point is that examination of the radiofrequencies obtained for a single pumping frequency shown in Tables 4-4 and 4-5 will reveal a 196 50- 30- 20-+ Frequency Shift (kHz) 10- ‘ ”T o ' i 4 ' 5 ' a ' 10 Frequency Split (MHz) Figure 5-4. Plot of the frequency shift caused by the four- interactingelevel double resonance effect against the assumed frequency splitting between the two lower frequency hyperfine transitions fer the conditions described in Fig. 5~3. The vertical axis is the difference in frequency between the center of the best Lorentz line approximation to the calculated lineshape and the assumed hyperfine frequency for the lower-frequency component of the infrared radiofrequency double resonance doublet. All of the conditions for the calculated lineshape in Fig. 5-3 apply, except that the difference between the hyperfine frequency in the upper vibrational state (vcd) and that in the lower vibrational state (”ba) is varied. This difference is plotted on the horizontal axis. 197 number of strongly overlapped lines, which might be expected to be shifted. In these cases, however, the overlapped lines do not involve four interacting levels, as shown in Fig. 5-1. We believe, and the residuals in Tables 4-4 and 4-5 seem to confirm our belief, that the shifts occur only when the two transitions occur between four interacting levels. The calculation should probably be done for the eight-level system, but the necessary algebra and computer time are both formidable. As has been shown, the frequency shifts of RF-transitions in low frequency region have been traced to a result of a four-interacting- level double—resonance. The amount of frequency shift and the distorted lineshape were calculated numerically by the use of density matrix; the calculated frequency shift and lineshape with the estimated input parameters show good agreements with the experimentally obtained values. Considering the amount of shift in frequency, the four-interacting-level double-resonance effect must be taken into account in the assessment of measured frequencies, especially for overlapped transitions in the low frequency region. 198' V-4 References l. C. E. Small, J. G. 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