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I??2_ MSU is an Affirmative Action/Equal Opportunity Institution 0-12771 ”WM? Mm? *c’i” "“ Universsi iv 3' _l . u. .-.--._ -.__ ., P‘s—vi 0.. “-... PLACE IN RETURN BOX to remove this checkout from your record. TO AVOID FINES return on or before date due. DATE DUE DATE DUE DATE DUE 1mg .3 2" “ ll “AL-CM; __ _____l c‘v- _ l N . ' ‘ _ “I MSU to An Affirmative Action/Equal Opportunity Institution chnS-DJ ELECTRICAL PROPERTIES AND PHYSICAL CHARACTERISTICS OF POLYCRYSTALLINE DIAMOND FILMS DEPOSITED IN A MICROWAVE PLASMA DISK REACTOR By Bohr-ran Huang A DISSERTATION Submitted to Michigan State University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Department of Electrical Engineering 1992 672' 373/ Copyright by Bohr-ran Huang 1992 ABSTRACT ELECTRICAL PROPERTIES AND PHYSICAL CHARACTERISTICS OF POLYCRYSTALLINE DIAMOND FILMS DEPOSITED IN A MICROWAVE PLASMA DISK REACTOR By Bohr-ran Huang Diamond possesses many excellent properties which motivate investigations of the potential of diamond for a wide range of electronic, mechanical, and optical applications. This work experimentally investigates techniques for high quality dia- mond synthesis and develops means for electrical and physical characterization of the films. The films are deposited by plasma assisted chemical vapor deposition using a methane/ hydrogen plasma in a microwave plasma disk reactor system. Both a diamond paste nucleation method and a diamond powder nucleation method are studied in this research. Although as indicated by Raman spectroscopy both methods produced similar quality diamond films, the powder nucleation method produced fine grain, sub-micron sized crystallite, films whereas the paste nucleation method produced large grain, several-micrometer size crystallite, films. This differ- ence is due to a higher density of surface nucleation sites in the powder polished films. Grain size could also be varied by using microwave power, pressure, and the methane/ hydrogen ratio as processing variables, however, the effect is smaller than the differences caused by the two nucleation methods. For electrical characterization, a new sample preparation method was developed in cooperation with the University of Wuppertal which allows metallic access to both sides of the diamond film. Using this technique, the properties of a variety of metal/ diamond contacts were investigated. Although films were not intention- ally doped, thermo-power measurements show all films to be p-type with activation energies between 0.1 and 0.5 eV. For powder polished films, all metallic contacts were ohmic. These samples were used to explore the high electric field properties of diamond. It was discovered that for fields larger than approximately 1x105 V / cm the electrical properties are dominated by defects, where defect is used generically for either an impurity or a structural defect. For low electric fields, the electrical conductivity was constant which resulted in ohmic behavior. But for high fields, the conductivity was field activated according to Poole’s law. This behavior was modeled as being due to ionizable defects and indicates that there is approximately one ionizable defect per 10,000 host atoms. As a result of such defects, the breakdown field for these films was somewhat less than 1x106 V/cm. A large concentration of defects is compatible with the observation of ohmic contact behavior regardless of metallic work function since contact space charge layers would be sufficiently thin to allow tunneling. N on-ohmic, Schottky barrier contacts were achievable on the paste polished films. For Al/diamond/silicon structures diode characteristics were observed. These I-V characteristics were modeled as an ideal Schottky barrier diode in series with bulk diamond, for which the property of the bulk diamond follows an I ocV'" relation- ship, indicative of space charge limited current in an insulating material. The rec- tifying behavior was determined to be at the Al / diamond surface rather than the diamond/ silicon surface. The best rectification ratios were 2x105. To my parents Chien-Ching, Tsui-Kuan C. Huang and my wife Pey—Nan C. Huang ACKNOWLEDGEMENTS The author would like to thank Dr. Donnie K. Reinhard for his guidance , support, and encouragement. Special thanks is extended to Dr. Jes Asmussen Jr. and Dr. Timothy Grotjohn for their valuable discussions, and Dr. Peter A. Schroeder for his comments. Additional thanks is given to Dr. Engemann and Mr. Hans Keller in Wuppertal University (Germany) for their help on fabricating back-etched diamond samples, Dr. Kevin Gray of Norton Company and Dr. Mark Holtz in the Physics department of Michigan State University for providing the Raman spectra, and Dr. Kevin Hook in the Composite and Structural Materials Center of Michigan State University for performing the XPS analysis. This work was supported in part by grants from Wavemat, Corp. and the Michigan Research Excellence Fund. vi TABLE OF CONTENTS LIST OF TABLES x LIST OF FIGURES xi 1 Introduction 1 1.1 Motivation for Diamond Research .................... 1 1.2 Research Objectives ............................ 3 1.3 Dissertation Outline ........................... 4 2 Synthetic Diamond : Background Review 5 2.1 Introduction ................................ 5 2.2 Brief History of Diamond Synthesis ................... 6 2.2.1 Historical Background ...................... 6 2.2.2 Growth Mechanism of Diamond Films ............. 13 2.3 Review of Diamond Film Technologies ................. 17 2.3.1 Hot Filament Chemical Vapor Deposition Techniques ..... 18 2.3.2 Plasma Assisted Chemical Vapor Deposition Techniques . . . 20 2.3.3 Other Deposition Methods .................... 24 2.3.4 Nucleation Methods. ....................... 24 2.4 Physical Attributes of Diamond ..................... 27 2.4.1 Comparison of Bulk and Film Material Properties ....... 27 2.4.2 Comparison of Semiconductor Properties ............ 30 2.5 Review of Diamond Diodes and Transistors ............... 33 3 Film Deposition and Sample Preparation 38 3.1 Introduction ................................ 38 3.2 The MPDR System ............................ 38 3.2.1 The Microwave Cavity ...................... 38 3.2.2 The Deposition System ...................... 41 3.3 The Nucleation Methods .................. . ...... 45 vii 3.4 Diamond Film Deposition ........................ 3.4.1 Operation of The System ..................... 3.4.2 Experimental Parameters .................... 3.4.3 Substrate Temperature ...................... 3.5 Fabrication of Electrical Samples .................... 3.5.1 Four-Point Probe Samples .................... 3.5.2 The Metal / Diamond/ Silicon Samples .............. 3.5.3 Back-Etched Samples ....................... Physical Characterization 4.1 Introduction ................................ 4.2 Raman Spectroscopy ........................... 4.3 X-ray Photoelectron Spectroscopy .................... 4.4 Dek-Tak Analysis ............................. 4.5 Scanning Electron. Microscope Analysis ................. 4.6 Film Uniformity Analysis ......................... Electrical Characterization 5.1 Introduction ................................ 5.2 Four Point Probe Characterization ................... 5.2.1 Experimental Method ...................... 5.2.2 Theory of Conductivity vs. Temperature ............ 5.2.3 Comparison with Physical Characterization .......... 5.2.4 Experimental Results and Match with Theory ......... 5.3 Back-Etched Samples. .......................... 5.3.1 The Back-Etched Samples and IV Measurement Set-Up . . . 5.3.2 Contact Effects on Back-Etched Samples ............ 5.3.3 High Field Effect ......................... 5.3.4 Photo Efiect ............................ 5.4 The Metal/ Diamond/ Silicon Samples .................. 5.4.1 The I-V Measurement Set-up .................. 5.4.2 Contact Effects on Metal/ Diamond/ Silicon Samples ...... 5.4.3 Photo Effect ............................ 5.4.4 Diamond Schottky Barrier Diode ................ Summary and Future Research 6.1 Summary of Important Results ..................... 6.1.1 NucleationMethod ...... viii 48 48 53 54 61 61 65 65 72 72 73 79 89 94 107 113 113 113 113 116 118 122 130 130 132 132 145 147 147 151 158 165 183 184 6.1.2 Quality of Diamond Films .................... 6.1.3 Back-Etching Technique ..................... 6.1.4 Diamond/ Silicon Interface .................... 6.1.5 Activation Energy of Diamond Films .............. 6.1.6 Electric Field Dependent Conductivity of Diamond Films . . . 6.1.7 Diamond Schottky Barrier Diode ................ 6.2 Future Research .............................. 6.2.1 Improvement for Diamond Deposition .............. 6.2.2 The Techniques for Physical Characterization ......... 6.2.3 The Role of SiC at the Diamond/ Silicon Interface ....... 6.2.4 Defects States in Diamond Films 6.2.5 Diamond Devices ......................... A Deposited Diamond Films B Electrical Samples BIBLIOGRAPHY ix 185 185 186 186 187 188 188 189 189 190 191 191 193 198 202 2.1 2.2 2.3 2.4 2.5 4.1 4.2 4.3 4.4 LIST OF TABLES Physical properties of bulk natural diamond.[68] ............ 28 Properties of bulk natural diamond and synthetic diamond films.[13] . 29 Properties of diamond, i-C, and graphite.[21] .............. 31 Working definition for different carbon coatings.[69] .......... 32 Comparison of semiconductor properties for diamond, Si, GaAs, ,BSic.[70] 34 Relation of average grain size vs. methane concentration, microwave power and plasma pressure by the paste-polished method. ...... 105 Relation of average grain size vs. microwave power and plasma pressure by the powder-polished method ...................... 106 Relation of deposition rate vs. methane concentration, microwave power and plasma pressure by the paste-polished method. ...... 108 Relation of deposition rate vs. methane concentration, microwave power and plasma pressure by the powder-polished method. ..... 109 2.1 2.2 2.3 2.4 2.5 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 3.9 3.10 3.11 3.12 3.13 LIST OF FIGURES The atomic structure of (a) diamond (b) graphite ............ 7 Phase diagram of carbon.[12] ....................... 8 Illustration of free energy difference between diamond and graphite. . 10 Low pressure CVD diamond synthesis in the phase diagram of carbon.[13] 12 Relationship between diamond properties and engineering applica- tions.[70] .................................. 35 The cross section of the MPDR and processing chamber, and a schematic display of the electric (E) and magnetic (H) field patterns Of the TMou mode. ........................... 39 The microwave power source, circuit, and cavity applicator ....... 42 The diagram of the MPDR CVD system ................. 44 SEM pictures of the silicon substrate prepared by diamond paste method. 47 SEM pictures of the silicon surface prepared by diamond powder method. 49 The MPDR CVD system during the diamond film deposition. . . . . 52 Top view of the MPDR processing chamber. .............. 56 (a) Typical temperature profile and (b) better temperature uniformity of the silicon substrate ........................... 58 Si substrate temperature vs. microwave input power for 1 ‘70 and 0.5 % methane concentration at 50 Torr. .................. 59 Si substrate temperature vs. microwave input power for 1 % and 0.5 % methane concentration at 60 Torr. .................. 60 Si substrate temperature vs. microwave input power for 50 and 60 Torr at 0.5 % methane concentration ...................... 62 Si substrate temperature vs. microwave input power for 50 and 60 Torr at l % methane concentration ....................... 63 Temperature difference between silicon and silicon nitride for 0.5 ‘70 methane concentration at 50 Torr ..................... 64 xi 3.14 3.15 3.16 3.17 4.1 4.2 4.3 4.4 Fabrication of the four-point probe samples. The actual surface was more uneven than is indicated here. (a) The starting point is a silicon nitride substrate which has received a nucleation procedure. (b) Since the substrate is insulating, the sample is ready for the 4 point probe measurement. ............................... Fabrication of the metal/ diamond/ silicon samples. (a) The surface is nucleated by diamond powder or diamond paste, (b) the diamond film is deposited, and (c) top contacts are evaporated through a shadow mask. Aluminum is shown here as an example .............. Fabrication of back-etched diamond samples for surface analysis. (a) Silicon is coated with diamond using conventional method. (b) The sample is secured to an epoxy substrate. (c) The silicon is removed by chemical etching. ............................. Fabrication of dual-sided metal contacts on isolated diamond films. (a) The silicon is coated with diamond and (b) a metallic contact is evaporated on the first diamond surface. (c) A wire lead is attached to the evaporated metal and (d) the substrate is placed face down in epoxy. (e) The silicon is removed by etching and (f) metal contacts are evaporated on the second diamond surface .............. Raman spectroscopy is based on a process of inelastic scattering of photons by phonons. ............ . .............. Raman spectra for diamond and silicon on (a) absolute wave number scale and (b) relative wave number scale ................. Raman Spectroscopy set-up for the Raman spectrum analysis.(From Dr. Gray) ................................. Raman spectra of 0.5% methane samples at (a) 936 °C (b) 1040 °C' - and (c) 1090 °C. (From Dr. Gray) ................... 4.5 4.6 4.7 Raman spectra of samples with conditions : (a) 0.5% methane, 1000 °C’ (b) 0.5% methane, 1040 °C (c) 1% methane, 1000 °C and (d) 1% methane, 1040 °C. (From Dr. Gray) .................. Raman spectra of samples of 0.5% methane at 1000 °C’ for (a) 10 hours’ deposition and (b) 6 hours’ deposition. (From Dr. Gray) ....... Raman spectra of samples with 0.5% methane at 1040 °C’ by (a) powder-polished method and (b) paste-polished method. (From Dr. Gray) ................................... xii 66 67 69 70 74 76 78 80 81 82 4.8 Raman spectra of (a) the as-deposited film and (b) the free standing film of the sample with 1.5% methane at about 1040 °C. (From Dr. Gray) ................................... 4.9 Principle of X-ray Photoelectron Spectroscopy. When a core level elec- tron absorbs a photon of energy (hu) greater than its binding energy (E3), the electron is ejected from the atom with kinetic energy (K.E.) 4.10 ESCA spectra of samples exposed to air for (a) a long time and (b) no time before the analysis. (From Dr. Hook) ............... 4.111 (a) Elemental survey scan of the sample before the Ar sputtering (b) higher resolution narrow scan of (a) in the carbon region. (From Dr. Hook) ................................... 4.12 (a) Elemental survey scan of the sample after the Ar sputtering (b) higher resolution narrow scan of (a) in the carbon region. (From Dr. Hook) ................................... 4.13 SEM view of the paste-polished produced diamond film on a cleaved sample showing the silicon substrate, the interface, and the side view and top surface of the diamond film. .................. 4.14 The surface profile on (a) the top surface of an as-deposited paste- polished produced diamond film and (b) the back surface of the film after transfer to the epoxy substrate. .................. 4.15 SEM view of the powder-polished produced diamond film on a cleaved sample showing the silicon substrate, the interface, and the side view and top surface of the diamond film. .................. 4.16 The surface profile on (a) the top surface of an as-deposited powder- polished produced diamond film and (b) the back surface of the film after transfer to the epoxy substrate. .................. 4.17 The extreme top surface profiles of (a) large-grain-size and (b) small- grain-size diamond films .......................... 4.18 Typical SEM photo of the top view of the diamond film prepared by the paste—polished method. The triangular shapes indicate [111] crys- tallite faces. (MW power: 600 W, plasma pressure: 60 Torr, methane concentration: 0.5%.) ........................... 4.19 Typical SEM photo of the top view of the diamond film prepared by the powder-polished method. (MW power: 600 W, plasma pressure: 60 Torr, methane concentration: 0.5%.) ................. xiii 84 86 88 90 91 93 95 98 101 102 4.20 Growth mechanism of diamond film prepared by (a) paste-polished and (b) powder-polished method. The latter has a higher nucleation density and therefore a finer grain film .................. 103 4.21 This SEM photo shows large and small grain size diamond growth on the same substrate ............................. 104 4.22 (a) Cross section view of laser scan from plane A to D. (b) Thickness (pm) uniformity analysis on an area of 1 cm X 2 cm of a sample. . . 112 5.1 The set-up of the four point probe method ................ 115 5.2 Raman spectra of (a) NDF-S3, (b) NDF—S4, and (c) NDF—S6. (From Dr. Holtz) ........................ ' ......... 120 5.3 Raman spectrum of N DF-Sl. (From Dr. Gray) ............ 121 5.4 Conductivity vs. 1000/ T of N DF -Sl .................. 125 5.5 Conductivity vs. 1000/ T of N DF—S3 .................. 126 5.6 Conductivity vs. 1000/ T of N DF—S4 .................. 127 5.7 Conductivity vs. 1000/ T of N DF-S6 .................. 128 5.8 Raman spectrum of the diamond film as deposited on the silicon sub— strate with substrate temperature at 1000 °C. (From Dr. Gray) . . . 131 5.9 The I-V measurement set-up of the back-etched samples. ....... 133 5.10 I-V characteristics of a small grain size sample with gold contacts top and bottom. It shows linear and symmetric behavior at low voltages. (Electrical sample : P47-Tl) ....................... 134 5.11 I-V characteristics of a small grain size sample with gold contacts top and bottom. It shows nonlinear behavior at high voltages. (Electrical sample : P47-T1) ............................. 136 5.12 The I — V3/2 characteristic and (b) the I - V2 characteristic of Figure 5.11. (Electrical sample : P47-Tl) .................... 137 5.13 I-V characteristic of diamond film with gold contacts top and bot- tom. Experimental data is shown by data points. The solid line represents the model results of Eq. (5.12) with (27¢)o=2.6x10'10 It“, Go = 2.1x10‘11 0“, and a = 0.042 V". (Electrical sample : P47-T1) 139 5.14 I-V characteristic of diamond film with top indium contacts and bottom gold contact. Experimental data is shown by data points. The solid line represents the model results of Eq. (5.12) with Goo=2.1><10‘1° fl“, Go = 2.0x10‘11 9“, and a = 0.045 V“. (Elec- trical sample : P47-T3) .......................... 140 xiv 5.15 5.16 5.17 5.18 5.19 5.20 5.21 5.22 5.23 5.24 5.25 5.26 5.27 I-V characteristic of diamond film with silver contacts top and bot- tom. Experimental data is shown by data points. The solid line represents the model results of Eq. (5.12) with Goo=2.9x10'1° Q“, Go = 4.0> P' P’ Waveguide Dummy Load Reflected Power Figure 3.2. The microwave power source. circuit, and cavity applicator. The fit respect aslnglt A la in some not use it perio: stainless I'aruum It’ll] a mun, [01 Ton region [1 the rang, CODdlIlox Same 0P! pump {Ir The 5 Pump is 355%. In bfl'li’epn l 339- nit 43 The flow controllers have maximum operating flows of 10,000, 500, 100, and 10 sccm respectively. The gas output of each mass flow controller is mixed simultaneously into a single gas channel which feeds the quartz processing chamber through the baseplate. A large stainless steel vacuum chamber is below the baseplate and quartz chamber. In some cases, this could be used as a downstream processing chamber, although it was not used as such in this research. [6] Pressure measurement within the vacuum system is performed through four vacuum gauges. There are three gauges connected to the stainless steel vacuum chamber; a baratron pressure gauge, a thermal conductivity vacuum gauge, and an ion pressure gauge. The baratron pressure gauge (model MKS 122A) can determine pressure from 0.1 Torr to 1000 Torr. The thermal conductivity vacuum gauge (TC2) (model MKS 286) can accurately measure pressure from 1 mTorr to 1 Torr, and the ion gauge (model MKS 290) is able to measure in the high vacuum [region (10"3 to 10‘9 Torr). These three different pressure gauges can therefore cover the range from very good vacuum to above an atmosphere depending on the operating conditions. In addition, a second thermal conductivity vacuum gauge (TCl) with the same operating pressure range is located between the roughing valve and roughing pump (mechanical pump). The system is pumped down by a Alcatel 2033 roughing pump. The mechanical pump is filled with Alcatel 200 oil which is safe for pumping hydrogen and methane gases. In order to minimize the backstream oil from the pump, a baffle trap is placed between the pump and the chamber. Because the hydrogen and methane are explosive gases, nitrogen gas is also used to purge the gas exhaust for safety reasons. Flow Controller (“:8KD "DA; Valve fl-IIL‘ Melon mm mm IonPresaureGaupe run-nun tau (mutual .l, C m N, WV“ 8. T02 TC1 (FWM) (Oriana-r) Thannd Doom Thermal 6mm Vaaum Vaaium Guac- Gm (us-name-) (hi-Hurts-) em Figure 3.3. The diagram of the MPDR CVD system. 3.3 Ti A wide variei appwacbes‘ mfhesis. I] mond p0WC in detail as l The dial 1. 0.25 W- IEXMEI P lletadi luhnI diamond pas rubbing hack 2. Step 1 pro ishing. :1 him substrate suri 3. Next the s hnsdimmedl water for ahof l. The subst: IHIOI I l.\'H nation left ore Iiii 1', °- The substr. ”202: IHCI Hints. Again, i‘ 826“ and 5 fro 45 3.3 The Nucleation Methods A wide variety of nucleation methods are described in chapter 2. In this research, two approaches were used to do the sample polishing and cleaning before the diamond synthesis. They are l. the diamond paste nucleation method, and 2. the dia- mond powder nucleation method. The two nucleation methods will be described in detail as follows. The diamond paste nucleation method : 1. 0.25 pm Buehler Metadi synthetic diamond paste was placed on a Buehler TEXMET polishing cloth sheet, which is water and oil resistant. Then Buehler Metadi lubricant oil was sprayed onto the paste. The substrate was placed onto the diamond paste position and was gently polished by hand for about 20 min by using rubbing back and forth motions. 2. Step 1 produces a substrate surface which has a dirty appearance. After the pol- ishing, a kimwipe with some acetone was used to get rid of the dirty stain on the substrate surface as much as possible. 3. Next the substrate was placed in a boiling TCE solution for 3 min. Then it was rinsed immediately in running acetone, running methanol, and running de-ionized(DI) water for about 60 sec each. Finally it was dried with nitrogen gas (N2). 4. The substrate was then immersed in a freshly prepared degrease etch (5H20 : 1H202 : 1NH4OH) for 10 min at about 70 °C’ to remove residual organic contami- nation left over from the solvent cleaning. Then it was rinsed in DI water and dried with N2. 5. The substrate was next immersed in a freshly prepared de-metal etch (8H20 : 2H202 : 1H CI) for 10 min at about 70 °C' to remove ionic and metallic contami- nants. Again, it was rinsed in DI water and dried with N2. Step 4 and 5 from the RCA cleaning procedure are widely used in the silicon industry. «I; (l) U-JJ 101 4- Dir. 46 [91] 6. After the RCA clean, the substrate was placed in a 9:1 H20:H F diluted solution in order to get rid of the thin oxide layer. This was again followed by a rinse in DI water and a dry with N2. The substrate at this point was ready for the diamond film deposition. If the substrate was a silicon wafer polished to a mirror finish, then after step 6 one cannot see scratches easily on the shining surface by eye unless it is observed under a strong light. No diamond particle residue was found either by the optical microscope or by the scanning electron microscope as shown in Figure 3.4. The diamond powder nucleation method : l. The substrate was cleaned by following step 3 to step 6 of the diamond paste method. 2. Dry 1 pm natural diamond powder was spread on a 3-inch diameter sacrificial silicon wafer which was used as a lapping surface. The substrate surface was then prepared by gentle polishing by hand on the sacrificial wafer for about 2 min. 3. Following the polishing process, the substrate receives an ultrasonic ace- tone/ methanol cleaning for 5 min respectively. 4. The substrate also received a diluted H F solution treatment, DI water rinse and blow dry with nitrogen. At this point the substrate was ready for the diamond film deposition. If the substrate was originally mirror-polished silicon, after step 4 one can easily see a marked difference of the surface. The surface is filled with a lot of scratches and is now hazy compared to the previous mirror-like surface. Under the optical microscope and the scanning electron microscope, the surface is seen to be rough and full of scratches as compared to the diamond paste nucleation method. In Figure 3.5 one can easily see the difference of the surface prepared by the powder nucleation method. 47 Figure 3.4. SEM pictures of the silicon substrate prepared by diamond paste method. Inot treat) 3.4 3.4.] In the are 50‘ a givel by \‘irt Single C have be mOde “ PFPSSuye fined tt Ton. b}. the (War Operatjn! TM,“ m 48 What are the effects of the nucleation mechanism on the diamond film growth? In other words, is there any difference on the film growth after different surface treatments? The answer is yes! It will be described in the next section. 3.4 Diamond Film Deposition 3.4.1 Operation of The System In the MPDR, a microwave (MW) plasma is generated within a resonant cavity. There are several advantages over radio-frequency (rf) and direct current (dc) plasma. For a given power input and plasma size, the electron density is higher in a MW plasma by virtue of the higher frequency, so its reactivity is expected to be very high. Since MW plasma can be electrodeless, electrode contamination can be eliminated. Although the electromagnetic modes of a perfect cylindrical cavity are well known [92], the introduction of a plasma into the cavity can significantly alter the field geometry. However, the MPDR can create a microwave discharge when excited in a single cavity electromagnetic mode. For example, in the past experimental discharges have been sustained in the TEm {93], TE211 [3], TMou and TMou modes [94]. Each mode was experimentally evaluated for its potential to deposit films at discharge pressures of 30 - 90 Torr. The cavity applicator was first length (L,) and probe (LP) tuned to a specific mode. Then a discharge was started at a gas pressure of 5 - 10 Torr, by applying microwave power which then ignited a discharge that entirely filled the quartz processing chamber. The discharge pressure was then increased to an operating condition of 30 - 90 Torr by manually adjusting the roughing valve while length and probe tuning the cavity to a matched condition. It was found that the TMou mode is superior to the others in this pressure range and set-up. [10] 49 \. ' 15KU X18888 8813 l.8U CEU91 Figure 3.5. SEM pictures of the silicon surface prepared by diamond powder method. 50 The experimental parameter space is large, since the microwave power, CH4/H2 ratio, substrate material, shape of the substrate, position of the substrate, discharge pressure (plasma pressure) all may contribute to the quality of the diamond depo- sition. A systematical operation procedures should be conducted in order not to inadvertently introduce new parameters. Consequently, a well defined procedure of operation for ”turning on” and ”shutting off” the MPDR CVD diamond system was developed as follows. The procedures of turning on the system : l. The substrate received the surface treatment either by diamond powder nucleation method or diamond paste nucleation method before putting it into the quartz pro- cessing chamber. The size of the substrate was always 2 cm x 2cm for silicon and 1.2 cm x 1.2 cm for silicon nitride. 2. The system stand-by condition is under vacuum. So the first step was to close the baratron valve, open the system vent valve, and allow the nitrogen gas to flow into the quartz chamber until the chamber pressure reaches atmosphere. Then the quartz disk and the sliding short are removed from the system. 3. Silicon substrates were typically mounted on a 0.1 inch thick graphite holder with a 2 cm x 2 cm recessed area. The graphite holder was placed on a quartz tube, typi- cally 3.25 cm high, which stands on the perforated stainless steel sheet, contained in the quartz processing chamber. The silicon nitride substrates were mounted directly on the quartz tube without a graphite susceptor. In both cases, the substrates were in a position along the cavity axis. 4. The quartz disk was positioned such that it smoothly fit the viton O-ring. The system vent valve was closed and the processing chamber was evacuated by the rough- ing pump with an ultimate pressure of 10" Torr. The baratron readout was then adjusted to zero. 4.. 5D! PM 11:5 51 5. The sliding short was placed in the cavity, then the cavity length L. was set to approximately 7 cm which is the position for the TMon mode. The probe position L, was set at about 1.8 cm which corresponds to maximum absorbed power and min- imum reflected power. 6. After the reading in both of the thermal conductivity vacuum gauges (TC 1, TC2) was almost zero, gas was introduced into the discharge chamber. 99.999 % H2 and 99.99 % CH4 Airco gases are used in this research. The flow rate and ratio of the gases were monitored through the 4-channel gas flow controller. The nitrogen purge and water cooling were on from this point throughout the whole process . 7. The roughing valve was ”throttled” to increase the chamber pressure up to 5 to 10 Torr as measured by the baratron gauge, then MW power was applied. At ignition the discharge completely filled the quartz chamber, but as the pressure increased to 30 - 90 Torr (It takes about 5 - 15 min), the discharge contracted and separated from the surrounding quartz walls and formed a roughly semi-spherical shape when the TMou mode was used. During the plasma pressure increase, cavity length and probe tuning are still necessary to minimize the reflected power. Visual inspection showed that the discharge uniformly covered the whole substrate under this particular mode. Typically, the microwave input power and plasma pressure are in the range of 400 - 900 watts and 50 - 80 Torr respectively. 8. Typically the system ran for 5 - 10 hours in order to get the desired thickness of the diamond films. For the duration of the run, the roughing valve was monitored to provide the desired plasma pressure. Operation of the MPDR CVD system during the film growth is shown in Fig- ure 3.6. One can see the discharge glowing inside the cavity through a transparent metal-screened side window. The procedures of shutting off the system : Figure 3.6. The MPDR CVD system during the diamond film deposition. 53 1. The MW power was reduced from several hundred watts down to 0 immediately and the gas flow of both hydrogen and methane gases were turned off. Also the roughing valve was fully open to rapidly eliminate the gases from the discharge chamber. At this point, the T01, T02, and baratron pressure gauges all read almost zero. 2. A 20 min period was allowed to let the system cool down. Then the water cooling was turned off and the system was vented to nitrogen and the sample was removed. Unless otherwise noted, these were the procedures for starting and ending a de- position process. The procedure to terminate the deposition process is crucial to the question of formation of a surface conducting layer on top of the diamond film. For example, if reactive gases continue to flow while the substrate is cooling, a graphite layer may be formed. Early in the research, another approach was used to turn off the system. First, the methane flow was turned off to prevent graphite formation on the surface of the diamond film but the hydrogen was left on. Second, the hydrogen flow was gradually reduced,a.nd then the microwave power was turned down immediately. However, Raman characterization showed. a graphite peak instead of the diamond peak on one of the samples under this procedure. The energy of the hydrogen plasma is high enough to convert diamond into carbonaceous conducting layer. [32, 79] 3.4.2 Experimental Parameters The experimental deposition parameters varied in this research are summarized as follows. Methane Concentration : The percentage of methane in the methane/ hydrogen mixture was varied from 0.5% to 1.5%. Microwave Power : The microwave input power was varied from 400 W to 900 W. Plasma Pressure : The plasma pressure range investigated was from 50 to 80 Torr. 54 Gas Flow : Total gas flow was varied from 100 seem to 250 sccm. Substrate Position : The quartz pedestal length was varied from 2.5 cm to 3.5 cm. Additional deposition parameters, as described elsewhere in this chapter, are the choice of substrates (silicon or silicon nitride) and the nucleation procedures (dia- mond paste method or diamond powder method). It should be noted that there is a big difference between the deposited diamond films which are prepared by diamond powder method and diamond paste method. Large grain (greater than 1 pm) size diamond films were obtained by the diamond paste prepared method, and small grain (sub-micron) size films were achieved by the diamond powder prepared method. A more detailed study of the grain size difference will be discussed in chapter 4. 3.4.3 Substrate Temperature In the last subsection, it was noted that during the film growth the position of the substrate, flow rate, CH4/H2 concentration, microwave power, and plasma pressure are all experimental parameters. Each of these may contribute to the film proper- ties either directly or indirectly in that they affect the substrate temperature. In this research, the substrate was self-heated by the plasma and microwave power. Consequently, changing the deposition conditions generally changed the substrate temperature. Temperature is a very important parameter in any CVD process, including dia- mond film deposition. Most often, good quality diamond films are deposited with a substrate temperature between 800 °C and 1100 °C [10-60]. Usually, there are two ways to determine the substrate temperature. One way is to determine the sub- strate temperature by direct contact as for example by a thermocouple through the substrate holder, which is on the down side of the substrate. However, microwave coupling to the thermocouple wire is a potential problem in this approach. Another 55 way is to determine the temperature without direct contact as for example with an optical or infrared pyrometer. For a microwave applicator one means of optical access is through the system window, which is on the top side of the substrate. Generally the windows are shielded by a metal screen which provides microwave power leakage protection. In this case the measurement goes through the metal screen, transparent window quartz wall, and discharge to the substrate. Pyrometer calibration is always a questionable matter in such a situation. The temperatures reported for good quality diamond films by direct contact with a thermocouple (800 °C to 950 °C) are often lower than those reported by the pyrometer methods (900 °C to 1050 °C). In our design, the original sliding short on the MPDR can be replaced with a short constructed with an axial opening to allow vertical optical access to the substrate as shown in Figure 3.7. A brass collar is used for shielding the MW leaks. The advantage of this set-up is that one can measure the temperature through only quartz and plasma to the substrate. Without a metal screen, calibration for the measuring device is much easier and temperature measurement accuracy improved. Generally these vertical pyrometer measurements produced higher (100 °C - 150 °C) readings than pyrometer readings through the metal screened window. An Ircon Ultimax optical pyrometer (model UX-20), with working temperatures between 600 to 3000 °C, was used for measuring the substrate temperature. This is a small spot size instrument which has a spot size approximately equal to D/ 100 mm where D is the focusing distance. This device has a focal range from 500 mm to infinity, but close focus lenses can be used to reduce the focal range. There are four different close focus lens with focal ranges of 100 - 130 mm, 130 - 180 mm, 180 - 290 mm, and 250 - 540 mm respectively. The unit was generally used with a 370 mm focus distance, which corresponds to a spot size of 3.7 mm. This makes it possible to measure the temperature distributions across the substrates. 56 tical gyprometer Plasma Quartz Tube ______ Substrate and Perforated Graphite Holder Stainless Steel Sheet [III to Vacuum Chamber Figure 3.7. Top view of the MPDR processing chamber. Eat thu de 09‘! is comes respect tempei for on eat] min frc Howev Insom higher : Shfinks Sllppbl 57 Each material has different emissivity, which is the main calibration factor for this device. When the silicon emissivity of 0.89 and the silicon nitride emissivity of 0.92 is multiplied by the quartz correction factor of 0.95, the corrected emissivity comes to 0.85 and 0.88 for measuring the temperatures of silicon and silicon nitride respectively. Then the calibration is also confirmed using silicon wafers at comparable temperatures in thermal diffusion furnaces. For several runs at various deposition conditions, 9 spot measurements were made on each substrate. The corner and side measurement points were approximately 2 mm from the edge of the substrate. Figure 3.8 (a) shows a typical temperature profile. However the uniformity is quite dependent on substrate position and cavity tuning. In some cases much better profiles were observed. A better uniformity case is shown in Figure 3.8 (b). Generally, all points showed temperatures within plus/ minus 5 % of the center temperature. However, better uniformity was sometime achieved within less than 1 %. Figure 3.9 and Figure 3.10 show the substrate temperature dependence on power for 1 % and 0.5 % CH4/H2 concentrations for two different plasma pressures, 50 Torr and 60 Torr. At both cases, a 2 cm x 2 cm silicon wafer was placed on a 0.1 inch thick graphite holder which is supported by a 3.25 cm high quartz pedestal. There is no obvious temperature difference for the 1 % and 0.5 % concentration depositions. The temperature increases with increasing microwave power in a nearly linear fashion. Figure 3.11 and Figure 3.12 show the the same data plotted so as to demonstrate the pressure dependence of substrate temperature. With higher plasma pressure, higher substrate temperatures, were observed. At higher pressures, the plasma ball shrinks and the energy is concentrated nearer the substrate. In all the above cases, the microwave input powers listed are shown as measured by the Cheung microwave power supply. The actual power delivered into the cavity is about 75 % of the microwave (a “fire 3 lhe Sill“ 58 (a) 905°C 930°C 960°C Microwave 910°C 950°C 980°C Probe 915°C 950°C 985°C Screened Window ( b ) 1070°C 1070°C 1060°C 1 075. C 1 076° C 1 080° C Microwave Probe 1080°C 1085°C 1090°C Screened Window Figure 3.8. (a) Typical temperature profile and (b) better temperature uniformity of the silicon substrate. 59 1080 l l l I 1 T : 0. 0- . . 8395: : 1.8% o— A Substrate matenal : Si O 4 106° ' Plasma pressure : 50 Torr ‘ L 2 1040 - d 3 :3 q.) 1020 - r 2‘ E3 1000 e - 8 66 H 980 *- 'i 4.: a: .0 fl U) 960 F . 940 I L l I l L 450 500 550 600 650 700 750 800 Microwave Input Power (W) Figure 3.9. Si substrate temperature vs. microwave input power for 1 % and 0.5 ‘70 methane concentration at 50 Torr. AO°~ ¢L~F€.quhcfih ~tn¥rr n\.‘ at! .‘..rua.n IIHU 60 1120 l T j r r l l 1100 - Substrate material : Si , . O . Plasma pressure : 60 Torr 1080 - 1060 h 1040 - 1020 - 1000 - 980 P Substrate Temperature (°C) 960 - 940 L 1 l 1 l l L L J 350 400 450 500 550 600 650 700 750 800 850 Microwave Input Power (W) Figure 3.10. Si substrate temperature vs. microwave input power for l % and 0.5 ‘70 methane concentration at 60 Torr. 61 powers from the Cheung microwave source. When silicon nitride substrates were used, a 1.2 cm x 1.2 cm x 0.5 cm substrate was supported on a 2.75 cm high quartz pedestal without a graphite holder. F ig- ure 3.13 shows the temperature difference between silicon and silicon nitride for 0.5 % methane concentration at 50 Torr. The substrate temperature of silicon nitride increases almost linearly with microwave power and is higher than that of silicon at the same deposition conditions. The reason for the higher temperature with silicon nitride is that the surface area is smaller than the silicon. The plasma will then con- tribute more energy per unit area on the silicon nitride samples as compared to the silicon samples. 3.5 Fabrication of Electrical Samples 3.5.1 Four-Point Probe Samples Silicon nitride, which is an insulating composite ceramic material, was used as the substrate for fabricating four-point probe samples. As described in chapter 3 (section 4), a 1.2 cm x 1.2 cm x 0.5 cm silicon nitride sample was placed directly on a 2.75 cm high quartz pedestal for deposition. Both diamond powder and diamond paste nucleation methods were used to prepare the substrate. The as-received silicon nitride substrates showed an uneven surface upon microscope examination, with multiple trenches and ridges which were on the order of a few micrometers wide and deep. However, the deposited diamond film followed the surface topography and successfully covered this uneven surface. As shown in Figure 3.14, as-deposited diamond films were ready for the four-point probe measurements which determines the sheet resistance of the diamond films. Results of the 4 point probe resistivity measurements will be discussed in chapter 5 1"- ‘i‘f‘llil'hk /C°\ < .1 62 1120 T I I T l T T T l 1100 Substrate material : S i - CH4/H2 concentration : 0.5% 1080 ~ 1060 - 1040 - 1020 r 1000 - 980 P Substrate Temperature (°C) 960 - 940 L l l l l l L J 4 350 400 450 500 550 600 650 700 750 800 850 Microwave Input Power (W) Figure 3.11. Si substrate temperature vs. microwave input power for 50 and 60 Torr at 0.5 ‘70 methane concentration. 63 11m T j T T l T T T 6 on 4“- 58 Torr ‘- A 1080 - Substrate material : Si - 9 CH4/H2 concentration : 1% v q) 1060 .. “ H 3 “3 _ _ S-r 1040 Q) Q. a 1020 L ~ Q . El 3 1000 - ‘* :6 1'3 m 980 i- a ..Q :3 U) 960 L - 350 400 450 500 550 600 650 700 750 800 Microwave Input Power (W) Figure 3.12. Si substrate temperature vs. microwave input power for 50 and 60 Torr at 1 7o methane concentration. 64 11m T T I I T T I T I 5i3N4 A- S: 0- A CH4/H2 concentration : 0.5% 0 Plasma pressure : 50 Torr 8.x 4 Q) 1050 r- H 3 :6 i- Q) Q. a 1000 - . Q3 E-l 3 c6 33 m 950 i- " .0 fi U) . 900 l l L 1 l L 1 J l 250 300 350 400 450 500 550 600 650 700 750 Microwave Input Power (W) Figure 3.13. Temperature difference between silicon and silicon nitride for 0.5 % methane concentration at 50 Torr. 65 (section 2). 3.5.2 The Metal/ Diamond/ Silicon Samples For the metal/diamond/silicon samples, both It and p—type silicon substrates with (100) orientation and resistivity of 1-2 Q-m were used, with a area of 4 cm2. Some samples were prepared with the diamond paste nucleation method and some by the diamond powder nucleation method. After deposition, a shadow mask with 900 pm diameter openings was used to form metal contacts on the top of the diamond films. Typically, Al contacts were most often used in the diamond paste prepared samples as shown in Figure 3.15. But on the diamond powder prepared samples, a shadow mask with smaller openings (400 pm) was used. An, Ag, and In were used as the top metal contacts in this case. The electrical properties will be described in chapter 5 (section 4). 3.5.3 Back-Etched Samples For film characterization, it is useful to have access to both sides of the film. Towards this purpose, a procedure suggested by Dr. J. Engemann from the University of Wuppertal was used. Some of the preparation details were developed by H. Keller at the University of Wuppertal. Specifically, after the diamond deposition on the silicon substrate, a back-etched process was performed to transfer the diamond film from the silicon substrate to an epoxy substrate. For samples intended for back surface analysis, the coated silicon was cleaved into approximately 5 mm x 5 mm samples which were placed diamond film down into a Torr - SeaITM [96] mixture formed by 1 part of hardener and 2 parts of resin on an aluminum oxide substrate. After a 70 °C' anneal for 30 min, the silicon was removed by etching. Both NaOH (25 ‘70 by weight to water) and KOH (44 ‘70 by 66 -(a) O. O . ...... Silicon Nitride AAAAAAAAAAAA AAAAAAAAAAA AAAAAAAAAAAAAAAA o . AAAAAAAAAAAAAAAAA AAAAAAA AAAAAAAAAAAAAAAA KAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA.— [amon 'm ..__ Silicon Nitride ( S'aN 4) Figure 3.14. Fabrication of the four-point probe samples. The actual surface was more uneven than is indicated here. (a) The starting point is a silicon nitride substrate which has received a nucleation procedure. (b) Since the substrate is insulating, the sample is ready for the 4 point probe measurement. 67 8". ‘— IICOTI AAAA“AKAAAnAKAAAAAAAAAKKKAAAAA“KI AA AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA AAA . AAAAAAAAAAAAAA AAAAAAAA AAAAAA AAAAAAAAAA O O AAAA AAAAAAAAAAAAAAAAAAAAAAAAAAAAAA AAN.‘ “AAA AAAAAAAAAAAAAAAAAAAAAAAA AAAAAAAAA‘ lm AAAAAAAAAAAA‘AAA‘AAAA‘AAAAAAAAAAAAAAA 8.. IllCOTI (c) . . . W W W —A' Dot AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA C . RAAA AAAAAAAAAAAAAAAAAAAAAAAAAAAAA “Aflfllb‘ m m AA AAAAAAAAAAAAAAAAAAAAAA “AAA AAAAA AAAA la on I AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA ~—Si|icon Figure 3.15. Fabrication of the metal/diamond/silicon samples. (a) The surface is nucleated by diamond powder or diamond paste, (b) the diamond film is deposited, and (c) top contacts are evaporated through a shadow mask. Aluminum is shown here as an example. 68 weight to water) were successfully used with a bath temperature of 58 °C. For a substrate thickness of 15 mils, it takes about 25 hours to etch the silicon. With lower temperature, longer time is needed to finish the etching process. There is sufficient adhesion between the top polycrystalline surface of the diamond film and the epoxy that the intact film remains, attached to the hardened epoxy substrate, thereby providing the back surface for analysis as shown in Figure 3.16. In some cases, however, film peeling and wrinkling were observed from the epoxy, indicating either films with higher internal strain or poor film-epoxy adhesion [95]. Some of the diamond/ silicon interface (back-etched diamond surface) characterization results will be discussed in chapter 4. For electrical access to both sides of the film, the sample preparation procedure was modified as follows. After diamond deposition on the silicon substrate, the first (bottom) metal contact was evaporated onto the diamond surface through a shadow mask. Then a wire lead is attached to the evaporated metal with Epo — TekTM polymide silver conducting epoxy [97] which is cured first for 30 min at 50 °C and then 60 min at 150 °C. The sample is placed top down in the Torr — SeaITM epoxy and the silicon is removed by back etching. At this point, the evaporated metal contact is visible through the transparent diamond film, and the second diamond surface is available for electrical contacts as shown in Figure 3.17. The second (top) metal contacts then can be evaporated onto the back-etched surface through another shadow mask with much smaller openings. A careful study of diamond film samples prepared by this method will be discussed in chapter 5 (section 3). 69 ( a) «— Diamond Film ‘\ Silicon ( P 0' N W99 ) ( b ) Silicon Diamond Film °—Al203 (6) T0" 393' Diamond Film Figure 3.16. Fabrication of back-etched diamond samples for surface analysis. (a) Silicon is coated with diamond using conventional method. (b) The sample is secured to an epoxy substrate. (c) The silicon is removed by chemical etching. 70 (a) .— —- Diamond Film “~Sillcon (PorNtype) (b) , , First Metal Contact ., .— -— Diamond Film ‘- ~ Silicon ’ ,- First Metal Contact _. .— — Diamond Film ' ‘— ~'Sillcon / Contact Wire (d) ..... _. Contact Vlfire ,- -’ ' T 2;, .._)- Diamond Film §,‘ _______ _ First Metal Contact A9 EPOXY / ( Bottom Metal Contact) Torr Seal 3. , Silicon Figure 3.17. Fabrication of dual-sided metal contacts on isolated diamond films. (a) The silicon is coated with diamond and (b) a metallic contact is evaporated on the first diamond surface. (c) A wire lead is attached to the evaporated metal and (d) the substrate is placed face down in epoxy. (see also Engemann, et' al. [95]) 71 Torr Seal (f) Second Metal Contact .,....—-—...N_ /’ (Top Metal Contact) Contact Wire ,-’ /V\_ \ W ..i _ Diamond Film / >4 """" "’i 5“ ‘ First Metal Contact Ag Epoxy / 3' ' (Bottom Metal Contact) Torr Seal \ \ Contact Wire \. - Diamond Film Figure 3.17 (cont’d): Fabrication of dual-sided metal contacts on isolated diamond films. (e) The silicon is removed by etching and (f) metal contacts are evaporated on the second diamond surface. CHAPTER 4 Physical Characterization 4.1 Introduction Physical characterization of the deposited film is very important to determine whether the film is in fact diamond and if it is indeed diamond, the film quality. There are several methods which may be used for film characterization, such as Raman spectroscopy, X-ray diffraction, reflection high-energy electron diffraction (RHEED), scanning electron microscope (SEM), X-ray photoelectron spectroscopy (XPS), Auger analysis, and others. In this chapter, we will use Raman spectroscopy to study the film quality in terms of sp3 bonding, XPS to perform surface analysis, SEM to examine the surface morphology, a Dektak profiler to evaluate the surface profile, and laser scanning microscopy to observe the film uniformity. Detailed descriptions of these methods are in the following sections. 72 73 4.2 Raman Spectroscopy Raman spectroscopy is based on an inelastic light scattering process. The incident photons, which are monochromatic, interact with the material either by creating or annihilating one or several phonons and then emerge with energies different from the incident photons. As in Figure 4.1, the strong line centered at hu is due to elastic scattering of photons and is known as Rayleigh scattering. The weak lines at 111/th originate from inelastic scattering of photons by phonons and constitutes the Raman spectrum. The Raman bands at frequencies V — 6 are called Stokes lines, corresponding to phonon generation, and those at frequencies V + 6 are known as anti-Stokes lines, corresponding to phonon absorption. The intensity of the anti- Stokes lines are usually considerably weaker than those of the Stokes lines [98] and the Raman spectra reported in this chapter are based on the Stokes-line signals. Figure 4.2 shows the Raman spectra for diamond and silicon on the absolute wave number scale and on the relative wave number scale. Most traditionally Raman spec- tra on the relative wave number scale were presented. For example, in this research, a wavelength of 488 nm laser was used by the Raman operators. It corresponds to the photon energy of 2.541 eV and wave number at 20492 cm‘l. Since only the first-order Raman scattering, which involves the optical phonons with wave vector k 2 0, is considered, for diamond the energy of optical phonon involved is 0.165 eV. Considering only the Stokes signal, the photon energy becomes 2.376 eV after the phonon generation. Photon energy of 2.376 eV corresponds to wavelength of 522 nm and wave number of 19160 cm“. A strong peak of diamond is then observed at 19160 cm"1 if an absolute wave number scale is used. It is 1332 cm“, which is called the Roman shift for diamond, between 19160 cm‘1 and 20492 cm“. The reported natural diamond peak at 1332 cm"1 is on the relative wave number scale [99]. Similarly, for silicon the optical phonon energy is 0.063, eV. After calculation, the silicon peak will 74 Raman Spectroscopy ' (a) m, Elastic Scattering Argm h” / ...___’ ___) . Laser , \ m, + ms >lnelastic Scattering Sample h" - his no : Optical phonon energy (b) Rayleig'i Spectrum . Raman Spectrun Raman Specmm ( Stokes line ) ( Natl-Stokes line ) hi! " h6 ‘ hi! bi! + 116 Figure 4.1. Raman spectroscopy is based on a process of inelastic scattering of photons by phonons. 75 1 on the relative be at 19984 cm‘1 on the absolute wave number scale and 508 cm” wave number scale. It is also known that graphite shows broad peaks at about 1360 cm‘1 , 1590 cm'1 [100] and amorphous carbon at about 1600 cm"1 [41]. Diamond-like carbon, which is amorphous but has properties close to those of diamond, is reported to have a broad peak at about 1500 - 1550 cm“. [101, 102, 103] The larger the Raman signal at 1332 cm"1 and the smaller the other peaks, the higher quality of the diamond films in that the results indicate a preponderance of sp3 bonding (diamond) rather than sp2 bonding (graphite). At the present time, Raman spectroscopy is considered to be the best technique to distinguish between the diamond, diamond-like carbon and graphite. Dr. Kevin Gray in Norton Company (Northboro, Massachusetts) performed most of the measurements for the Raman spectrum analysis. The principle set-up of the instrumentation is illustrated in Figure 4.3 [104]. The monochromatic and polarized light of the laser passes through an interference filter that rejects spurious lines and background from the laser source. The light beam then enters the beam-splitter and is focused by the lens to the samples. If micro-Raman analysis is performed, the microscope shown in Figure 4.3 is added to reduce the beam size. Light scattered from the sample through a variable beam-splitter then is focused by the lens onto the entrance slit of the 1/8 meter double-grating monochromator. Before entering the monochromator, a notch filter was used to reduce the laser light. The double-grating monochromator acts as a tunable filter of extremely high contrast; its purpose is to prevent the internally scattered intense Rayleigh light from overpowering the weak Raman lines. Light leaving the final slit of the double-grating monochromator is collected by a 1024 element silicon-array detector, whose output is processed with a ”photon counting” electronics. It includes a programmable detector controller and 76 (a) Laser Diamond Silicon h 1 9160 1 9984 20492 Intensity Absolute Wave Number( cm’1 ) 0)) Diamond - .é‘ in § Silicon E A 508 1 332 Relative Wave Number( cm") Figure 4.2. Raman spectra for diamond and silicon on (a) absolute wave number scale and (b) relative wave number scale. 77 an oscilloscope, which is used for monitoring the real time signal synchronously with the spectrometer. Finally, the data processing and data acquisition were collected and processed with the personal computer. In this work, typically a wavelength of 488 nm from an Argon laser and a laser power of 400 mW was used to excite the Raman signals. In Figure 4.4 Raman spectra of 0.5 % C H; / H2 powder-polished samples are compared at different substrate deposition temperatures. All spectra show the characterization peak at 1332 cm“. At 936 °C’ the 1332 cm‘1 peak is quite small and a broad shoulder around 1500 cm‘1 indicates amorphous diamond—like component in the film. Around 1040 °C' a better defined diamond peak shows up. Then at 1090 °C a graphite peak at 1600 cm”1 becomes obvious. In all cases the peak at 508 cm“1 is the silicon Raman signal. For depositing good quality diamond films, the depositing temperature must be in a certain range. If the temperature is too low, an amorphous diamond-like component is dominant in the film. If the temperature is too high, graphitic component will play a major role in the film. It is observed that the preferential temperature range for good quality diamond films is between 1030 °C and 1060 °C. The Raman spectrum is also dependent on gas flow composition. In Figure 4.5 the Raman spectra for 0.5 ‘70 and 1 % gas mixture powder-polished samples are compared at a fixed substrate temperature of 1000 °C and 1040 °C. It shows that the 1 % samples have a larger graphitic component than the 0.5 % samples for both substrate temperatures. It indicates that for the same temperature, a smaller methane concentration of the gas flow produces better quality diamond fihns than a higher methane concentration does. Figure 4.6 shows that at the same growth condition a 10 hours deposition sample has a similar Raman spectrum to a 6 hours deposition sample, but the sample with longer deposition time has a stronger diamond signal and weaker silicon signal because 78 Optical Silicon Notch Filter Array ( ,\ a 433 nm ) Detector , l 1:30 -1 Microscope \\ Aperture Aperture 1/8 Meter eyepiece l \Van'able Monochromator AT '0" Laser Beamsplitter ( Spam Physics 2on ) Detector I ] Controller A .488 nm :C Beamsplitter Tunable Laser Line Filter Oscilloscope 32 X Microscope Objective Lens [] Computer Figure 4.3. Raman Spectroscopy set-up for the Raman spectrum analysis.(From Dr. Gray) 79 of the thicker diamond film. In Figure 4.4 to Figure 4.6, only powder-polished samples were analyzed. In Figure 4.7 Raman spectra of samples with the same deposition conditions but with different nucleation methods were examined. It showed that the Raman spectra were similar for samples with 0.5% methane at 1040 °C by both paste—polished and powder- polished methods. Consequently, the quality of diamond films shows no obvious difference between different kinds of preparation methods under the same deposition conditions. Raman spectra are based on bulk properties of the sample rather than on surface or interface characteristics. However, the method was used to indirectly identify the location of the graphite signal in one case. Figure 4.8 shows a good Raman spectrum with a small graphitic peak for a sample prepared with 1.5% methane at about 1040 °C. The temperature was not measured from the pyrometer directly but by estimation from the temperature measurement on the similar deposition conditions. A part of the film peeled off when the sample cleavage was performed. Absence of the graphitic peak was observed on the Raman spectrum of the free standing film. This suggests that some graphitic component exist in the diamond / silicon interface during the film deposition. When the diamond film peeled off, most of that graphitic component stayed on the silicon surface. Generally, Raman analysis is essential for characterizing the deposited diamond films. However, it is not appropriate to do the surface or interface analysis. Another characterization technique, X-ray photoelectron spectroscopy, is then introduced for the chemical analysis in the surface and interface layers. 4.3 X-ray Photoelectron Spectroscopy X-ray Photoelectron Spectroscopy (XPS) is also known as Electron Spectroscopy for Chemical Analysis (ESCA). This technique is able to analyze a wide of variety of (a) (b) (C) ”Half" 80 M "01’“ m "-000 1110.0 0N.” " 4 5‘4,” W-VOU-w-‘r-w-w—v—v—f—v—F-r v—r—w v-s-v-rP-v-w—m 4”.” 700.00 000.00 1100.0 1300.0 1010.0 7“.” not,” W-c,c--e,---f,c--e v ' ' ' ' l “.00 700.00 use.” 1~.0 1340.0 1010.0 l”... -e---. -'-' Q-s-o-w—rm-' -Q-e~ o-v -r>v-v-o-v- «0.00 700.00 ”.00 1200.0 1500.0 1010.0 mm CI Figure 4.4. Raman spectra of 0.5% methane samples at (a) 936 °C (b) 1040 ac and (C) 1090 °C. (From Dr. Gray) . 81 INIWIVV 451.00 I—' v v 1 v v u no... 700.00 0“.“ 10..0 10‘.0 1010.0 “m0” V a Y ' v v j 4”.“ 700-” ”a“ 10..0 1010.0 1010.0 (c) A (d) 8'10“ 1 I V V v V ‘ v V v ' j ' V V V as... 700.00 000.. 1000.0 1000.0 1010.0 400.00 700.“ ”o” 10..0 10‘.0 1010.0 Figure 4.5. Raman spectra of samples with conditions : (a) 0.5% methane, 1000 °C (b) 0.5% methane, 1040 °C (c) 1% methane, 1000 °C and (d) 1% methane, 1040 °C. (From Dr. Gray) 82 (3) ”AN 900m SAMPLE: HOP-047 000.00 . - T v ' v v—V v—j V v j v I V T W i I V Yfi V 700.00 702000 000.00 'V'WT'V'VY'WIYVU' INTENSITY 010.00 I j’ v v’ v I fffi v v V V V V ‘ 430.00 700.00 000.00 1200.0 1040.0 1010.0 0)) RANAN SPECTRUM IANPLE: NDF-PJI 001.00 var v - . j—fi 731.00 001.00 001.00 INIENBIIY flan-A 001.00 0000 45:.20.--v-.-- ----f---- 430.00 700.00 000.00 sumo sumo tame Home. on Figure 4.6. Raman spectra of samples of 0.5% methane at 1000 °C for (a) 10 hours’ deposition and (b) 6 hours’ deposition. (From Dr. Gray) 83 ( ) mm was: III-P30 ”a” fi V v ‘ v v v v I v v v v ' v I v v w v r . «l I 4 . F 1 0..00 .. u i- . D 1 D G D 1 "‘.oo - - D I f- » . N D d b 003.00 .- I on p 000.00 “t‘” [#7 v V ‘ V V W v ' v v v v ' v v v v ' v v v w 430.00 700.00 000.00 1200.0 1040.0 1010.0 (13) RANAN SPECTRUM SANPLE: NDF-N10 2100.0 ' 1040.0 1030.0 1220.0 INTENSITY 010.00 YVIUTYVITYT'IVYYVIVTTY U 430.00 700.00 000.00 1200.0 1040.0 ‘ 1010.0 Figure 4. 7. Raman spectra of samples with 0. 5% methane at 1040 °C' by (a) powder- polished method and (b) paste-polished method. (From Dr. Gray) 84 RAMAN SPECTM SAME: ”-05 01300111 SIDE 2w.o V V V V fl V v v ‘r v v v ‘fiv v v f I v v v P 1 t 4 r 2410.0 L. l : 1 L 4 19‘0-0 — d > 4 >- . \\ 4 .- H r- ‘ . 2 1470.0 .. .. 0- _ -‘ 2 H > 4 1000.0 .— p v- 4 r 1 533.00 f---,.---,fi--.j--.-,-..- 430.00 ' 700.00 900.00 1200.0 1540.0 1010.0 mum». CI! mm SPEC?” ME: FIT-05 FKE STAN)!“ FILM 2‘”.o ' V ‘ 1“ V ' V V ' W v V V ' v v v v I v v v v 0 d ’ 1 h c1 1050.0 .. ... D- d " 4 ’ 1 1510.0 _. _ >- " : h b H k d 2 L . m 1170.0 ,. _. p— Z " < 04 L 4 y b 030.00 ... " < ‘93-” f fifi Yfifi ' ' I Y ' ' ' I ' ' ‘ fifi ' V V ' 430.00 700.00 9”.00 1200.0 1540.0 1010.0 Figure 4.8. Raman spectra of (a) the as-deposited film and (b) the free standing film of the sample with 1.5% methane at about 1040 °C. (From Dr. Gray) 85 samples in terms of elemental and chemical composition on the surface layer of a sample, typically 5 to 50 )1 in depth. XP S involves the energy analysis of electrons ejected from a surface under energetic bombardment by X-rays as shown in Figure 4.9. The photoelectric process occurs when a core level electron absorbs a photon of energy greater than its binding energy. When this occurs, the electron is ejected from the atom with kinetic energy (K..E) expressed by the following equation: K.E. = hV—EB (4.1) where hu is the X-ray photon energy and E3 is the photoelectron binding energy. E3 provides both elemental information as well as chemical bonding information. Far example it is possible to distinguish carbon bonded as diamond from carbon bonded to silicon as SiC. Typically, KO, X-ray emission from the light metals is the photon source used by most XPS [105]. XPS characterization of the samples was performed in a Perkin-Elmer PHI 5400 X-ray Photoelectron Spectrometer in this research. Dr. Kevin Hook of MSU’s Com- posite and Structural Materials Center performed the XPS analysis. Samples were attached directly to the instrument analysis stubs and placed in the system pre- pumping chamber. System pressure during XPS analysis was approximately 10'9 mbar. The spectrometer is equipped with both a M 9 KO, standard source and a Al K a, monochromatic source. The Al K a monochromatic source was used mostly in this study and was operated at 600 W (15 KV, 40 mA). A continuously variable stage was used and set to 65° with respect to the sample surface. The portion of the sample was analyzed through an initial lens system in this instrument. For all analyses, the lens system was set in the large area, small solid angle mode. The size of the electron beam was 3.3 mm diameter circle. Data points were collected 'in the fixed analyzer 86 H 3‘ _.____ 2p H /e 25}L — 15 K A + hr ——> A“ + e' (ESCA) Figure 4.9. Principle of X-ray Photoelectron Spectroscopy. When a core level electron absorbs a photon of energy (hu) greater than its binding energy (E3), the electron is ejected from the atom with kinetic energy (KME) 87 transmission mode utilizing a position sensitive detector and a 180° hemi-spherical analyzer. There are two types of samples analyzed by this technique : as-deposited samples as shown in Figure 3.16 (a) and back-etched samples as shown in Figure 3.16 (c). All the samples analyzed by XPS were treated by the paste-polished method. For the as-deposited samples, the top surface of the diamond film was analyzed. Figure 4.10 shows the spectra of two different samples; one was left in the air for several weeks before the analysis and for the other the analysis was performed within 15 minutes after the deposition. Oxygen peaks were observed in addition to the carbon peak on the sample exposed to the air for a long time. Since the sample has some pinholes, silicon dioxide might in principle be a contributor to the oxygen peaks. However, as the analyzing angle (the angle of the beam relative to the sur- face) decreases the 0 peak increases. This suggested that the contamination came from the diamond film surface rather than pinholes. This does not necessarily mean that the diamond surface has formed carbon-oxygen bonds. The oxygen signal could be simply a result of non-outgassing H20 on the surface, since hydrogen is not de- tectable with XPS. Alternatively, oxidation of impurities in grain boundaries might be a contributor, although no other elemental signal were observed. Back-etched samples were used to analyze the diamond / silicon interface. In Fig- ure 4.11 (a) C, 0, K and Si were observed on the surface of the back-etched sample under the elemental survey scans. The K peak came from the K 0H which was in the silicon etching solution. Si peaks may have come from the silicon residue or S iC (as discussed below) which was not completely etched, or silicon from the etching bath. An additional source of Si, as well as 0, may come from contamination from the quartz disk. Such contamination has been previously reported for microwave CVD diamond deposition. [106] However, it is noted that the Si signal was not observed for the top surface XPS analysis. The big 0 peak, may also be due to contamination 88 10 v r L #t fi‘ .* i 4 c t ;

- 3 .. 0 1. .. fl 2 "" O .0- <)- 4,. 1 4M 7 A _... * - ‘ 0 .. 1,, 0 : : : % : ¢ ¢ ¢ ; : t 4. : : . r -1 x A 1110.0 9%.0 801.0 770.0 801.0 550.0 40.0 33.0 220.0 110.0 0.0 111mm DEM. 0V ‘ 1° ; 4. 4 Y . # 4 ¢ c i 4 . : qr- C Th 0 ‘P J»- ’ 4b 8 1P {b .. 41 7 w .. I. <1- 5 0 » '"' «- § 5 + .. i .. ,P . 4 1f «- . 3 1+- .. 4» 2 v .. .. .. 1 4- ., '"' 4)- 0 . ¢ ‘ ¢ 4 : g i - —A 770.0 600.0 3.0 Illllli ENERGY. 0V A I A A V I I 1100.0 ”.0 00.0 40.0 1 330.0 220.0 110.0 Figure 4.10. ESCA spectra of samples exposed to air for (a) a long time and (b) no time before the analysis. (From Dr. Hook) 89 of the torr-seal during the back-etch process. However, another contributor might be the oxidation of the silicon residue after the back-etch process. Figure 4.11 (b) shows more detailed information about the C peak. The most intense contribution to the overall peak shape is from the peak centered at 284.25 eV due to the deposited diamond surface layer. The smaller peak present at the lower binding energy side of the diamond peak is a contribution from the S iC interface layer (282.75 eV). It has been suggested that the growth of a thin layer of SiC (20 - 100 A) in the early stage of deposition is crucial to the formation of diamond films. [107, 108, 109, 110] In any case, the observation of a SiC layer is consistent with several other groups’ studies. [111,112,113] Typically Argon sputtering is the most used method to clean the surface impurities from an XPS sample. In this work, 3 KeV Argon sputtering at 15 mPa gun pressure was performed for 30 seconds. After the surface cleaning, it was observed that the 0 peak is obvious reduced from Figure 4.12 (a) which indicates that part of the contamination was removed. Also from Figure 4.12 (b) it is shown that the SiC shoulder has completed disappeared. Based on the sputtering rate of SiC, it is estimated that the carbide layer was approximately 30 A thick. However, the SiC signal was not observed in some of the back etched samples. For these samples, it is believed that the S iC layer was etched by the back-etch solution because the samples were not removed from the etching solution right after the silicon was completed etched. 4.4 Dek-Tak Analysis In chapter 3 (section 3), it was mentioned that the diamond powder preparation approach produced much finer grained films than did the diamond paste preparation method. Microscope examination shows the powder-polished film to be made of fine, 90 10 * . ¢ ¢— : . : '1 a 1 4!- O C d!- 9 T 0 8 1» 4)- <1- «L 7 4|- <> 0 4»- T- < 0 11' h: 5 4)- 1p z «1- <1- 4 4p 4»- .. ‘1) N K - 3 ~0- '1‘". . <- w/W" -. lWM St Si .. 2 4) "W , 4 4)- 4)- 1 <1- 4» 0- 4L 0 : ¢ : a 4+ ¢ ¢ 4 * t . t : : ¢ : ¢ : llmfi 931.0 880.0 770.0 650.0 550.0 40.0 330.0 220.0 110.0 0.0 01mm rm. 0" lo ‘ 4 *7 * i 4 ¢ ¢ i i 41 4v f 9 4% C 284.25 CV 41- 11- o- 8 ~0- 4» 4r d? 7 4L 4)- s 4r .. s - \ - :0 5 " «1- 2 <1- 4» 4)- r- 4 j 282.75 eV 1 3 4" .. 1h h’zP ‘F r 3’? «p 4)- 1 1* W «- .mev \ 1 0 ¢ ¢ : t : t ‘ : ¢ : : : : - ¢ : : fl : 310.0 238.0 23.0 291.0 232.0 2W3 230.0 25.0 281.0 282.0 29.0 010110 DERBY. ev Figure 4.11. (a) Elemental survey scan of the sample before the Ar sputtering (b) higher resolution narrow scan of (a) in the carbon region. (From Dr. Hook) 91 A I V V V I U U T MK I([)/E 00 A A j I 7 I ... 1 A j J Y Si - Si “ J l L 1 J I ‘1 ME "I an 1100.0 09.0 “.0 770.0 09.0 550.0 40.0 330.0 010110 DERBY. 0V L J ' Y 1 220.0 110.0 0.0 4—f-O-+-1-+- + —1-+~+-+— +——1—+—+—+—+——+—- A A L 1 V j 284.0 282.0 200.0 Figure 4.12. (a) Elemental survey scan of the sample after the Ar sputtering (b) higher resolution narrow scan of (a) in the carbon region. (FromtDr. Hook) 92 sub-micron crystallites whereas the paste-polished surface produced crystallites which were larger than one micron for similar deposition conditions. The difference is also obvious to the eyes. Prior to deposition, a silicon substrate has a mirror finish and reflected images are easily observed. After deposition on a paste-polished silicon substrate, the deposited diamond films show a highly specular surface with a gray appearance and no observable reflected images. However, with the powder prepared surfaces, the diamond film is flat and somewhat shiny with some ability to produce reflected images. There are also some other interesting visual observations. First, both types of films appear glittery under the sun or strong light, but the film-produced by the paste-polished method did show a darker background. Secondly, because the film prepared by the powder method is less specular, some of the scratches on the silicon substrate surface could be seen through the film. Third, if the grain sizes are small enough, film produced by the powder-polished method showed colorful interference rings due to thickness variation across the sample. For the samples produced by the paste-polished method, optical and electron microscopy of the transferred film shows a relatively flat back surface compared to the original top surface of the film. This observation is consistent with the cross- sectional view of the film and underlying substrate shown in Figure 4.13. It shows the relative smoothness of the back surface relative to the top surface. In order to quantify film smoothness, a Sloan DekTak II surface profiler was used. The relative smoothness of the two surfaces of the paste-polished diamond film is shown in Figure 4.14. Shown here are surface profiles measured over a 50 pm scan across the samples. A standard deviation of 940 A is observed about the mean for the top surface of the diamond film as deposited on the silicon substrate. When the silicon is removed as shown in Figure 3.16 (c) and the back surface is scanned, a 93 <—— Top Surface of Diamond Side View of *—'— Diamond 4—— Interface 4— Si Substrate 15w x7299 @063 1% ceoee Figure 4.13. SEM view of the paste-polished produced diamond film on a cleaved sample showing the silicon substrate, the interface, and the side view and top surface of the diamond film. 94 standard deviation of 130 A is observed. For the samples produced by the powder-polished method, SEM cross-sectional view shows relative smoothness of the top and bottom surfaces in Figure 4.15. It is clearly seen that the difference between these two surfaces is not as big as that of the paste-polished produced samples. The quantified smoothness of the two surfaces is shown in Figure 4.16. Typically, a standard deviation of 630 A is observed for the top surface and 570 A is for the bottom surface of the diamond film. As shown in Figure 3.4 and Figure 3.5, a rougher surface on the back side of the diamond film produced by the powder-polished method is expected. Figure 4.17 shows the top surface profiles of two extreme samples produced by the paste-polished and the powder-polished nucleation methods respectively. Standard deviations of 1600 A and 420 A are observed for the large-grain-size and small-grain- size diamond film respectively. 4.5 Scanning Electron Microscope Analysis The scanning electron microscope (SEM) has unique capabilities for analyzing sur- face. It is analogous to the conventional optical microscope, but a different radiation source serves to produce the require illumination. Whereas the optical microscope forms an image from light reflected from a sample surface, the SEM uses electrons for image formation. The different wavelengths of these radiation source result in dramatically different resolution levels. Electrons have a much shorter wavelength than light photons, and shorter wavelengths are capable of generating high-resolution information. Enhanced resolution then permits higher magnification without loss of details. The maximum magnification of the optical microscope is about 2000X and the theoretical resolution limit is about 0.17 pm. In practice it is difficult to clearly dis- 95 A 0° v :ol - "i 5.000 '3: i f = 4.000 3% g \ 4‘“ h 3 3,939 :3 ... 9 0 f l .i if 2.000 3 U l 3 .... g 3 l‘ A U : 2 5 0 ei'é‘é—Th—Tfihjg—ih'fig'Te 4 : scan length (pm) (b) .1 3 {xi 0 L U fl— :1 '3 s 1" V v , 1: ; . s : 5 .6... a E ~eee ab—‘i—rs-Tfimirsf—zh‘fi 51‘9” scan length (pm) Figure 4.14. The surface profile on (a) the top surface of an as-deposited paste- polished produced diamond film and (b) the back surface of the film after transfer to the epoxy substrate. ' 96 Q4; 4-. as «it 3:25:- j:- H'i,‘ ‘}: - ‘n 1". . “7' fl ‘L‘q‘; 3&9; 4" . '..,.:_'_ f . ’ v ‘2’ 4—-—_ Top Surface of 31"!” (7': "-‘vl‘i' .."2 “ “‘O'VA Diamond 0 .. v «-‘ ‘ fig ,4 ’\ l \ ‘37\:fi;~‘§¢_" *' ' _- u- -v'-4,- , van-r- . ‘-— ~_ (‘52 «rc- .- 4—— Side View of Diamond +—— Interface +—— Si Substrate Figure 4.15. SEM view of the powder-polished produced diamond film on a cleaved sample showing the silicon substrate, the interface, and the side view and top surface of the diamond film. 97 surface deflection(A) scan length (pm) fl) 0| 0 '9 ht— —-’—J q'1 P'———._ Ffl—i r H in 0 G my} “Mu-1H0... I. . UL” F. 1"qu . * W v—“v v a - 1 .- BEE! ”bl l-—.. .5? ,3 U! 3: '3 surface deflection(A) - 7" '-" 5 00 §3* 40 4s 00 .“0 f. p G .... I 0 J ..B . h scan length (pm) Figure 4.16. The surface profile on (a) the top surface of an as-deposited powder- polished produced diamond film and (b) the back surface of the film after transfer to the epoxy substrate. ' 98 ‘ 1.. 000 1" [V1 .2 ' J ‘ I L fi L___1 El 3 i M JU will R A “Q q [i L.. 1 .. .333 g s l l l Ill [ l l a: : [A I a '1] | 2.000 0 I v s l l l c L A . P3) 889 8 i . l| 7 I I '13 l I r 4.000 a 5 ll! ' V #53868 0 s 10 1s. 20 2... 30 are... 42773—30 scan length (pm) (b) ; . I :‘i a 2 $500 ‘5 3'1 L1 .000 .9. El \ z 8 I . 1 $1.500 “i: l ‘L I 1 ’ .1. 000 “U i Lani ' “I |' (1'. iv" mug WV J W lfifi .s. E 3 , 59g 8 : ' ‘l f V F." ii ° . cg ' ;-3.000 a : : m ' '3.568 : L4.000 0 JET 10 157-‘50 2. 30+..«. 46%45 J0 scan length (pm) Figure 4.17. The extreme top surface profiles of (a) large-grain-size and (b) small- grain-size diamond films. . 99 tinguish features smaller than 1 pm. In comparison, the wavelength of the electrons is less than 0.5 A, and theoretically the maximum magnification of electron beam instruments is beyond 800,000X. However, because of the instrumental parameters, practical magnification and resolution limits are about 75,000X and 40 71 in a conven- tional SEM [114]. Since polycrystalline diamond films often have sub-micron feature sizes, the high resolution capabilities of SEM are crucial for determining crystal mor- phology. In chapter 4 (section 4), it was noted that different grain-size polycrystalline di- amond films result from different nucleation techniques. Relatively large-grain-size diamond films, as in Figure 4.18, are formed by the paste-polished method and rel- atively small-grain-size films, as in Figure 4.19, are formed by the powder-polished method. The major reason for the difference is that the powder-polished method pro- vides a much higher density of nucleation sites than did the paste-polished method. Diamond particle residue and the scratches associated with polishing by diamond par- ticles provide nucleation sites which enhance the local configuration for the diamond growth. As shown in Figure 3.4 and Figure 3.5, more scratches and particle residue were observed by the powder-polished method than the paste-polished method. As the nucleation sites density increases, the space of lateral growth of diamond for each site is limited. Correspondly, the grain size becomes much smaller as shown in Fig- ure 4.20. This phenomenon also can be proved by a careful experiment described as follows. The surface was intentionally polished with less nucleation sites in one place than in the other places by the powder-polished method. After the deposition, the difference of the crystal growth is obvious under the SEM in Figure 4.21. Large grain size diamond particles show up in the area with less nucleation sites compared to the small grain size diamond particles in the area with a higher density of nucleation sites. This shows that the density of nucleation sites is a major factor in determining grain ll surfac surfac of llllt the a press them plan and Ples incre 00m Pea; 59% ‘1 mm 100 grain size. This observation is also confirmed by J. F. DeNatale and coworkers [115]. The main objectives for using SEM analysis in this research are to examine the surface morphology and grain size and to determine the film thickness. From the surface micrograph the average grain size of a film can be estimated by the method of linear intercepts, which is explained by the following equation. total path length l - . . . 4.2 no. of intercepts magmfzcatzon ( ) < grain size >= The results in Table 4.1 and Table 4.2 show that for a given preparation method the average grain size has a tendency to increase as the microwave power or plasma pressure increases. The higher the microwave power, the higher the plasma energy, then the higher the reaction rate, so the bigger the grain size. On the other hand, plasma density increases as the plasma pressure increases, so does the reaction rate and grain size. In Table 4.1 the data also indicates that in the paste-polished sam- ples the CH4/H2 concentration plays an important role since the average grain size increases significantly as methane concentration increases. It is understandable since more methyl radicals can form the same crystal at the same time. It was noted that the samples prepared by the powder-polished method were deposited at lower microwave power and plasma pressure conditions than those pre- pared by the paste-polished method since the experiment was performed sequentially for these two groups. The samples were prepared by the paste-polished method in the beginning. However, it was found from the Raman spectrum that a sample at the condition of 700 W, 70 Torr, and l % methane concentration showed only graphite peaks instead of a diamond peak since the deposition temperature is too high. Con- sequently the deposition conditions for later samples prepared by powder-polished method were lower. Y'— Dist. WM] 101 I . r a j \ y ‘E\ 1 ISKU X48 Figure 4.18. Typical SEM photo of the top view of the diamond film prepared by the Paste-polished method. The triangular shapes indicate [111] crystallite faces. (MW power: 600 W, plasma pressure: 60 Torr, methane concentration: 0.5%.) 102 ‘ 1% X " ~ “.2 1 V} ‘1‘ . -. \‘€." 1 Figure 4.19. Typical SEM photo of the top view of the diamond film prepared by the powder-polished method. (MW power: 600 W, plasma pressure: 60 Torr. methane concentration: 0.5%.) Voids Nucleal Sites g”re 4. (bl Powd. 103 (a) Voids g ‘ I i . \\_ ‘ \\ Diamond . \ ‘—‘ Columns Nucleation \. Sites \ SiC Layer \ / \- 4 ?--Silicon (b) Voids 1 10 \ \ \_ .3: Diamond Nugeation\\ - - Columns 'tesix \ SiC Layer \ ~ / V '\. - v v fw ~ ~—- Silicon Figure 4.20. Growth mechanism of diamond film prepared by (a) paste-polished and (b) powder-polished method. The latter has a higher nucleation density and therefore a finer grain film. 104 3.3.3 .. 21*! ‘3 \ :3“. ' ISKU X1888 4285 Figure 4.21. This SEM photo shows large and small grain size diamond growth on the same substrate. 3V5 (a) (b) (C) Table 4.1. Relation of average grain size vs. 105 CH4/H2 Concentration : 0.5 % Average grain sizes (pm) are listed below. Plasma Pressure Microwave "'9‘“ Power 60 Torr 70 Torr 80 Torr 600 W 0.83 ..- ..- 700 W 0.89 1.18 1.28 800 W 1.01 ..- ..- CH4/H2 Concentration : 1.25 % 600 W, 60 Torr : 1.41 pm CH4/H2 Concentration : 1.5 % 600 W. 70 Torr : 2.14 pm power and plasma pressure by the paste-polished method. methane concentration, microwave 106 CH4/H2 Concentration : 0.5 ‘70 A verage grain sizes ( pm ) are listed below. Microwave Plasma Pressure Input Power 50 Torr 60 Torr 80 Torr 400 W 0.47 --- 500 W --- 0.57 --- 600 W 0.55 0. 63 0.76 Table 4.2. Relation of average grain size vs. microwave power and plasma pressure by the powder-polished method. Mi n1 8" ...4. . I? 107 The relationship of the growth rate or the deposition rate (pm/hour) versus methane concentration, microwave power and plasma pressure by the two different preparation methods are listed in Table 4.3 and Table 4.4. Methane concentration is a major factor for the growth rate since the growth rate increases as the methane concentration increases in both preparation methods. The higher the methane concen- tration, the more methyl radicals (CH3) are available for deposition, so the growth rate increases. Likewise, the growth rates also had a tendency to increase as the microwave power and plasma pressure increase since the reaction rate increased as plasma energy or plasma density increased , however, the effect is smaller than the methane concentration effect. 4.6 Film Uniformity Analysis So far, in this chapter Raman Spectroscopy was used for film quality analysis, XPS was performed for diamond/ silicon interface studies, DekTak profiles were used for the film surface smoothness test, and SEM were used for the grain size and growth rate studies. But there is another important parameter, which is the film uniformity. When depositing the diamond film by using the plasma CVD technology described in chapter 3 (seCtion 4), usually an approximately hemispherical shape discharge is formed right above the substrates. "This phenomenon becomes particularly evident when the discharge pressure is above 50 Torr. The discharge size increases as the pressure decreases because at about 10 Torr or less the discharge tends to fill the quartz confinement chamber. The deposition rates of the film are dependent on the positions correspond to the density of the discharge. If at low pressures, the discharge volume is large enough to uniformly cover the sample, the deposition rate will be fairly uniform over the sample. At high pressures as the discharge size decreases, the deposition rates over the sample area will show more variation. The trade-off is that (a) (b) (C) Table 4.3. Relation of deposition rate vs. methane concentration, microwave power 108 CH4/H2 Concentration : 0.5 % Deposition rates ( um/ hour) are listed belbw. Microwave Input Power Plasma Pressure 60 Torr 70 Torr 80 Torr 600 W 0.34-0.38 700 W 0.35-0.4 0.36-0.41 0.37-0.42 800 W 0.39-0.44 CH4/H2 Concentration : 1.25 % 600 W. 60 Torr : 0.54 - 0.6 rim/hour CH4/H2 Concentration : 1.5 % 600 w, 70 Torr : and plasma pressure by the paste-polished method. 0.92 - 1.06 urn/hour 109 (a) CH4/H2 Concentration : 0.5 % Deposition rates (um/ hour) are listed below. Plasma Pressure Microwave "1901 Power so Torr so Torr so Torr 400 W 0.28-0.32 500 W ..- 0.33-0.38 «- 600 W 0.41-0.42 0.42-0.45 0.58-0.63 (b) CH4/H2 Concentration : 1 % Deposition rates (um/ hour) are listed below. Microwave Plasma Pressure input Power so Torr so Torr 600 W 0.48-0.52 0.560. 62 Table 4.4. Relation of deposition rate vs. methane concentration, microwave power and plasma pressure by the powder-polished method. 110 deposition rate goes down as the pressure and plasma density decreases. To determine the thickness on different parts of the film, SEM is still the most accurate measurement method. However, a gold coating of the sample is necessary to obtain good image resolution and sample cleavage is required. Consequently, the SEM technique is destructive. In order to determine a technique for measuring thickness uniformity non-destructively, a laser scanning confocal microscope (LSM) was used in this research. The LSM is a light microscope, but one with a difference! In the microscope’s name the words ”laser” and ”scanning” refer to the method of illumination, while ”confocal” refers to the method of image formation. The microscope has four light sources: a fiber optic tungsten lamp, a mercury lamp, an argon-ion laser with 488 and 514 nm lines, and a helium-neon laser with a 543 nm line. So the LSM can be operated both as a conventional microscope (using the tungsten or the mercury lamp) and a laser scanning instrument. The term ”confocal” indicates that the microscope is aligned so that the illumi- nated spot and imaged spot coincide precisely, which is not the case in conventional light microscopes. In a conventional microscope, light reaching the observer comes from all parts of the specimen within the field of view - both from the narrow hori- zontal plan which is in focus and from out-of-focus regions above and below it. The light from out-of-focus areas, which severely degrades the focal-plane image, generally limits to just a few microns the depth to which a specimen can be examined. In a confocal instrument the specimen is scanned point-to-point with a finely focused beam, most effectively by a laser, and a pinhole aperture is placed directly in front of the detector at the focal point of light coming from the in-focus part of the specimen. The effect of these modifications is to block light from out-of-focus regions because the focal point of such light falls either in front of or behind the pinhole 111 aperture. The result of this instrument configuration on the final image is a dramatic increase in resolution and contrast. The theoretical limit of resolution for a conventional light microscope is about 0.17 pm. But much smaller objects can be easily seen in the LSM. There are multiple reasons for this, chief among them being the elimination of out—of-focus light by the confocal pinhole. In addition, monochromatic light (the laser) eliminates chromatic aberration; scanning a specimen with a small spot, no matter what the light source, always improve resolution; and the photomultiplier detector is more sensitive than the human eye. Magnification in the LSM ranges from 200x to 16,000x [116]. This upper limit is significantly higher than a conventional optical microscope. In our case, however, the samples prepared by paste-polished method have a better resolution in the diamond/silicon interface than those prepared by powder- polished method since the interface was flatter by the former method. A sample with the biggest average grain size and thickest diamond film was used to perform the uniformity study. Under the SEM analysis, the thickness of the diamond film on an area of 0.2 cm X 0.4 cm is between 6.5 and 7.5 pm. By the LSM technique, a scan in the Z (or vertical) axis of the sample can be carefully observed since diamond is transparent to visible light. A 488 nm laser scan was used for the best resolution in our studies. The thickness of the film was then determined by the distance between A plane and D plane as shown in Figure 4.22(a). Eight thickness measurements were performed on an area of 1 cm x 2 cm of the same sample in different locations as in Figure 4.22(b). A distribution of thickness between 5.8 and 8.0 pm were obtained. This study did show that the LSM technique indeed can perform the uniformity studies efficiently without significant loss of accuracy and also without any sample destruction and contamination. 112 .................................................................................. A ................................................................... B Voids . \\ \s\ \ \ ,\ Diamond NUCIGati0n\ — ’ Co'umns Sites ‘\‘. ................................................... C V“ i\ \ / SiC Layer .1: ...... D — —Silicon (b) 8.0 6.9 6.1 6.5 7.8 7.4 5.8 Figure 4.22. (a) Cross section view of laser scan from plane A to D. (b) Thickness (pm) uniformity analysis on an area of 1 cm X 2 cm of a sample. CHAPTER 5 Electrical Characterization 5.1 Introduction In this chapter, conductivity vs. temperature results for the as-deposited diamond films will be described in chapter 5 (section 2). Then current-voltage characteristic of ' samples with dual-side metal contacts on the isolated diamond films will be discussed in chapter 5 (section 3). Finally, current-voltage characterization of the samples with metal-diamond-silicon structure will be discussed in chapter 5 (section 4). 5.2 Four Point Probe Characterization 5.2.1 Experimental Method The measurement of bulk resistivity, particularly vs. temperature, provides a fun- damental means of electrically characterizing materials and is essential to investigate current transport in diamond films. In order to avoid contact effects, a method of choice for measurement of electrical resistivity is the four point probe method. How- ever, on high resistivity thin films (such as diamond films), the measurement technique is nontrivial because of the requirement of accurately measuring small voltages and 113 9X Spa Tali 114 currents. A standard instrumentation approach such as is used on silicon wafers is not adequate. Consequently, a sensitive four point probe apparatus, with the capability of changing the measurement temperature, was constructed as in Figure 5.1. The sheet resistance of diamond films on insulating silicon nitride substrates (Si3N4) was measured with a Signatone four point probe station as follows. Four equally spaced point probes are brought into contact with the sample surface. A Hewlett Packard 4145 B Semiconductor Parameter Analyzer is used as the ammeter to measure the current (I), which is supplied by a dc power supply, through the two outer probes. The supply voltage is set at 40 V in this study. A high impedance digital voltmeter (Fluke Model 8840 A) connected to the two inner-probes is used for the voltage (V) measurement. This arrangement largely eliminates contact resistance effects, since the voltage measurement probes draw negligible current. The probe sta- tion is then placed in a Thermotron Environmental Control Chamber (Model 31.2) which allows the temperature to be varied from —75°C to 175°C. The sheet resistance Ra has a constant of proportionality between V/ I, and is expressed as follows Ro=€( V 7) (5-1) where 5 is a correction factor, the value of which is determined by the shape of the test sample and the ratio between the size of the sample and the probe spacing. In this experiment, the size of the Si3N4 substrate is 0.5” x 0.5” x 0.2” and the probe spacing is 0.0625 inches. For a square substrate and a substrate size to probe spacing ratio of 8, the correction factor 6 is determined to be approximately 4 [117]. The resistivity (p) of the diamond film is then obtained by p = Ra - t (5.2) 115 Ammeter (Model : HP414SB) @— Voltmeter (Model : Fluke such Temperature v Controlled Chamber V (Model : Thermotron $1.2) ..... / A \AAAA AAAAAAAAAAAAAAAAAAAAAAAAAAA.— Diamond Film AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA —- Silicon Nitride ( SiaN 4) Figure 5.1. The set-up of the four point probe method. 116 where t is the film thickness, and the conductivity (0) of the film is Eli-t 5.2.2 Theory of Conductivity vs. Temperature The conductivity of the diamond film on insulating material (Si3N4) was studied at different temperature levels in order to understand the conduction mechanism. As is generally the case for semiconductors, the electrical properties of diamond are dominated by the effect of dopants and other impurities or defects. Experimental measurements of the electrical conductivity provide information about the concentra- tion of electrically active impurities and defects as well as their energy levels. Thermopower measurements on the diamond films used in this research show that the films are p-type, indicating the presence of acceptor-type impurities or defects even though the films were not intentionally doped with acceptors. For a semiconductor with a single acceptor level at energy Ea in the energy gap, the hole concentration, p, is given by [118, 119] P = NueXP - [(Er - 190/le (5-4) where N” is the effective density of states in the valence band, E f is Fermi level, E0 is top level of the valence band and k and T denote the Boltzmann constant and absolute temperature, respectively. From charge neutrality, p = n + N," (5.5) where n is the electron concentration, No is the concentration of acceptors, and Na‘ Fr It prr Val 117 is the concentration of ionized acceptor. Consequently, Na 1+ 4exp[(Ea — Ef)/kT] p = n + (5.6) The term on the left side of the equation corresponds to positive charges, and those on the right side correspond to negative charges. However, at the temperature of interest here the electron density in p-type material is very small, so the first term on the right hand side can be neglected and Eq. (5.6) becomes [118] _ Na 1" ‘ 1 + 4exp[(E., — E,)/kT] From Eq.(5.4) and (5.7), one obtains 1 Eu — Ea p = §exp( kTE°)X[—N,,/4 + \/N,,2/16 + Nanezp( E” [T )1 (5.8) The hole concentration is directly related to the measured conductivity by the ex- pression 0’ = (“11)? (5'9) where q and up are electron charge and carrier mobility respectively. The reported value of hole mobility pp is 1200 cmz/V-s. [120] In this research, N” was calculate from N. = 2(21rmp'kT/h2)3/2 (5.10) where m,‘ is effective hole mass and h is Planck constant. [121] The reported value of m,‘(= 0.75 mo) of natural diamond was used [120], which yields N, = 3.137 - 1o15 - T3/2cm'3 ' (5.11) 118 From Eq.(5.8), (5.9) and (5.11), and the measured conductivities at different temper- atures, (Ea-E”) and Na may be used as parameters to fit the experimental data. The comparison of the experimental results and theoretical calculation will be discussed in chapter 5 (section 2.4). 5.2.3 Comparison with Physical Characterization There are four samples in this four point probe study, three of which are prepared by the diamond powder nucleation method and one which is prepared by the diamond paste nucleation method. The three powder-polished samples (N DF-S3,S4,S6) have similar sub~micron crystallite morphology and the paste-polished sample (N DF ~Sl) has a larger (greater than 1 pm) grain size diamond film based on optical microscope analysis. The deposition conditions for the samples are described as follows. The deposition times are all 6 hours. NDF-Sl, CH4/H2 : 0.5 %(1.25 sccm/250 sccm), M.W input power : 600 W, plasma pressure : 60 Torr, temperature : 1060 °C. NDF-S3, CH4/H2 : 0.5 %(0.75 seem/150 sccm), M.W input power : 500 W, plasma pressure : 50 Torr, temperature : 1035 °C. NDF-S4, CH4/H2 : 0.5 %(0.75 seem/150 sccm), M.W input power : 400 W, plasma pressure : 50 Torr, temperature : 1000 °C. NDF-SB, CH4/H2 : 0.5 %(0.75 seem/150 sccm), M.W input power : 320 W, plasma pressure : 50 Torr, temperature : 950 °C. Samples N DF-S3, S4 and S6 are as-deposited diamond films, for which the deposition was terminated by turning off the microwave power while both methane and hydrogen gas flows were on. However, the deposition for NDF-Sl was terminated by first turning off the methane gas flow, exposing the sample to a hydrogen plasma and 119 . then turning off the microwave power. This sample was subsequently treated in a solution (2H20:16H3P04:1HN03:1 acetic acid) at 80 °C for 1 hour in order to remove the conducting layer caused by the hydrogen plasma during the process. The corresponding Raman spectrum for each sample is shown in Figure 5.2 and Figure 5.3. In Figure 5.2, the Raman spectra, which were performed by Dr. Mark Holtz in Physics department of Michigan State University, of NDF-S3, S4, 36 are compared. Note that the horizontal wavenumber scale is in absolute wavenum- bers with photon energy increasing from left to right and phonon energy increasing from right to left. More typically, diamond Raman spectra are plotted vs. shifted wavenumber. In terms of shifted wavenumber, the peak that is apparent in each spec- trum is at 1331 cm’1 plus or minus 1 cm;1 and corresponds to the diamond peak. At all temperatures shown in this figure a strong diamond peak is noted. There are two indicators that the diamond films approach the Raman properties of natural di- amond as temperature increases from 950 °C’ to 1035 °C. First, the height of the diamond peak relative to the background level increases as the temperature increases. Secondly, the width of the peak increases as the temperature decreases. For natu- ral diamond, the peak is very sharp, with full-width-half-maximum (FWHM) of 2.1 cm”. For diamond films, FWHM values are substantially larger, in the range of 7 - 17 cm'1 [102]. In Figure 5.3, the Raman spectrum, which was performed by Dr. Kevin Gray in Norton Company, of N DF -Sl is shown. The spectrum shows a very sharp diamond peak along with a small graphitic peak on the right shoulder. This spectrum is similar to the spectrum of N DF-S3, with a FWHM equal to 9 cm“. 1N7 “IVY lC/SI r l .— .-. .. . : 17700 17.40 am am guano um . um i ... _ . -..- ..- --n _ - l (b) a ; INTENSITY (C/Sl Figure 5.2. Raman spectra of (a) NDF-S3, (b) NDF-S4, and (c) NDF-S6. (From Dr. Holtz) . INTENSITY 121 RAMAN SPECTRUM SAMPLE: NDF-Si 1010.0 890.00 770.00 850.00 530.00 415.20 l+llllllllllllllll TITTITTII'TTTTIITTI' 1 T T T I I I V I ‘ I V V V I V I V I l fii V V V 1 430.00 700.00 980.00 1280.0 1540.0 1810.0 RECIPROCAL CM Figure 5.3. Raman spectrum of N DF-Sl. (From Dr. Gray) 122 5.2.4 Experimental Results and Match with Theory The films in this study were not intentionally doped with impurities. However, im- purities may come from a variety of sources including impurities in the feed gases. Although the methane used was the highest purity readily available (99.99 ‘76), this is not high purity by semiconductor standards. A methane purity of 99.99 % essentially corresponds to one impurity in 10,000 methane molecules. If, as a case in point, there is one impurity per 10,000 carbon atoms in the diamond film, this would correspond to an impurity density of 1x1019 cm'3 which is more than sufficient to dominate the electrical properties. In conventional semiconductors like silicon , impurity densities in active device regions are typically on the order of 1x1015 cm‘3. Other possible sources of impurities include residual gases in the vacuum system, air leaks, and sam- ple handling. Only a mechanical roughing pump was used to. evacuate the system. Furthermore, structural defects in the crystallites and grain boundaries can introduce states in the gap which may act as traps, acceptors, or donors. Consequently, even though the films are not intentionally doped, it is anticipated that electrical properties of the film will be controlled by defects and impurities. Simple hot probe measurements based on the thermopower phenomenon showed that all of the samples were p-type, indicating that defects and/or impurities play the role of acceptors. By combining the theory of chapter 5 (section 2.2).with exper- imental results, information is obtained about the concentration of these states, and their energies. Performing the four point probe measurement, one can get the (V/I) ratio. Then following Eq. (5.1), it was found that the sheet resistances (R0) for NDF-Sl, S3, S4 and 86 at room temperature are 1.2 x 108, 1.3 x 106, 5.6 x 105, and 2.1 x 105 Q/D respectively. It was also noted that the sheet resistance of N DF-Sl before the cleaning procedure was 1 x 104 Q/D. All of these resistivities are low compared to 123 natural, un—doped, diamond. However the variation of resistivities among the samples is consistent with the Raman indication that higher deposition temperature produced properties closer to natural diamond since the diamond peak is more similar to that of natural diamond. Since the thickness of the samples were estimated to be about 3 pm thick for 6 hours’ deposition, from Eq. (5.2) the resistivities (p) at room temperature were calculated to be 3.6 x 10‘, 3.9 x 102, 1.68 x 102 and 6.3 x 101 Q-cm for NDF-Sl, S3, S4 and 36 respectively. Taking the inverse of the resistivity (p), then the conductivity (0‘) was determined and plotted. Figure 5.4, Figure 5.5, Figure 5.6 and Figure 5.7 show the temperature dependence of the conductivity for N DF-Sl, S3, S4 and 86 respectively. In all cases, points show experimental results and lines show the results of theoretical calculation from Eq. (5.8), (5.9) and (5.11) assuming a constant mobility (pp = 1200 cmz/V-s). The values of Ea-Ev and Na are presented in the following. NDF—Sl, Ea-E.,=0.51 eV and Na=2.5x1012 cm'3. NDF-S3, E.-E.=o.31 eV and 1v..=2.0x101'3 cm-3. NDF-S4, Ea-Eu=0.24 eV and Na=4.0x10‘3 cm‘3. NDF—SG, Ea-E.,=0.22 eV and Na=1.0x10” cm'3. However, in reality the carrier mobility for polycrystalline diamond films is much smaller than that in single crystal diamond. If it is assumed that p, = 12 cmz/V-s, the values of Ea-Ev and Na after the same curve fitting procedure are presented in the following. NDF—Sl, Ea-E.,=0.42 eV and Na=5.5x10“ cm'3. NDF-S3, Ea-E.,=0.23 eV and N¢,=3.5x1015 cm‘3. NDF-S4, E.-E,,=0.15 eV and N.,=4.0x1015 cm‘3. NDF—SG, E.-E.,=0.13 eV and N..=1.2><1016 cm‘3. 124 Generally, the model calculated data for both )1, = 1200 cmz/Vos and p, = 12 cmz/V-s fit quite well to the experimental results. However, there are some deviations from the experimental plots. This may indicate the existence of other levels in the forbidden gap or non-monoenergetic states, also the mobility is general not constant with temperature, but may either decrease or increase with temperature depending on whether impurity scattering or lattice scattering dominates. The paste-polished sample N DF-Sl has a much higher activation energy than the powder-polished samples N DF-S3, S4, S6. Also, the concentration of acceptors is an order of magnitude less than for the other samples. From chapter 4 (section 4), it is known that paste-polished samples usually have bigger grain size diamond crystals than the powder-polished samples. Comparatively, the concentration of grain bound- aries for paste-polished samples are smaller than those of powder-polished samples. This is consistent with a hypothesis that acceptor type states are associated with grain boundaries. However, the situation is evidently more complex since the chang— ing value of Ea-E'v indicates that the nature of acceptor level changes as well as the concentration. For comparison purposes, it is interesting to note that type IIb di- amonds which are naturally doped with boron are reported to have an activation energy of 0.37 eV [120]. An annealing process was also performed on all the samples to study if the temper- ature dependence of the conductivity would change. The samples first were cleaned by acetone, methanol, DI water and dried with N2. Then they were annealed at 500 °C for 1 hour in a furnace atmosphere of nitrogen with a 500 sccm flow rate. After the annealing, the sheet resistance of the N DF-SG is 1.6x109 Q/D at room temper- ature. It increased by nearly 4 orders of magnitude. The sheet resistance of the other samples could not be measured because the current was too small. For these samples, the sheet resistance is beyond the limit of the measuring equipment used in Conductivity (Q’l-cm'l) 0.001 0.0001 le—05: H 0 l 142—07 3 125 06 . p p I l T l 1 I l I 1 Theory — : Experiment 0 l LILJlll l L L l l l l L 3.2 3.4 3.6 3.8 4 4.2 4.4 4.6 4.8 1000/T (°K-1) Figure 5.4. Conductivity vs. 1000/T of NDF-Sl Conductivity (Q‘l-cm’l) 126 0.01 _ I I I I I I I I : Theory — 1 Experiment 0 . 0.001 _ 0.0001 1 L l l l I 3 3.2 3.4 3.6 3.8 4 4.2 4.4 4.6 4.8 1000/T (°K-1) Figure 5.5. Conductivity vs. 1000/T of NDF-S3 Conductivity (9'1 ~cm'l ) 0.1 0.01 0.001 3 127 I l I I T I 1 r Theory — Experiment 0 0 o O O l l l l l l L l 3.2 3.4 3.6 3.8 4 4.2 4.4 4.6 1000/T (ox-1) Figure 5.6. Conductivity vs. 1000/T of N DFoS4 4.8 Conductivity (9‘1 -cm‘1 ) 128 1 I r I - l I I I I Theory(before anneal) - - - - Theory(after anneal) — 0.1 Experiment(before anneal) D Experiment(after anneal) O , ..... a .................... 0.01 D D - [3 .......................... 0.001 0.0001 1e — 05 <> 0 1 — 06 e x 18 __ 07 1 1 l 1 l 1 l 1 3 3.2 3.4 3.6 3.8 4 4.2 4.4 4.6 1000/T (°K-1) Figure 5.7. Conductivity vs. 1000/T of NDF-SG 129 this investigation, that is greater than 1010 Q/Cl. The calculated Ea-E” and N, for N DF-S6-anneal are 0.44 eV, 1.9x 1010 cm‘3 when p, = 1200 cmz/V-s and 0.36 eV, 2.2x1012 cm‘3 when p, = 12 cm2/V-s respectively. No matter what the value of the mobility is, the significant decrease of the acceptor concentration indicates that part of the defects or impurities are expelled from the samples during the annealing process. The increase of the activation energy suggests that there are multiple impurity energy levels existing in the forbidden gap. When one level is annealed out, the previous minor level becomes dominant. Landstrass and Ravi presented a specific explanation for such an annealing effect; a model of hydrogen passivation of deep donor-like traps in the inter-band states. Hy- drogenation electrically neutralizes the traps and the resistivity is governed by shallow acceptor levels, the effective acceptor concentration increases and the conductivity in- creases. The annealing process on the other hand causes dehydrogenation resulting in electrical activation of deep traps. These donor-like traps cause the effective acceptor concentration to decrease because of compensation and the conductivity decreases. When the hydrogenated diamond films are heat treated in a neutral ambient, the hy- drogen can be expelled from the crystals, restoring the high resistivity. For example, with a 780 °C, 2 hour treatment in flowing nitrogen ambient, the resistivity increases from ~105 to ~10“ fl-cm. [122, 123] Albin et al. [124] also had a similar observation that the conductivity of the diamond films will increase several orders of magnitude after hydrogenation by the hydrogen plasma. However these measurements were per- formed by the two probe method instead of the four point probe method. Defects states due to dangling bonds and grain boundaries and inter-band levels due to impurities play major roles in the conduction mechanism of the diamond films. Consequently, from the four point probe experiment, there are indeed multiple inter- band energy levels existing in the forbidden gap and some of the impurities, such as :0 di hc 130 hydrogen, can be expelled from the samples by the annealing process. The effect of defects states will be discussed in chapter 5 (section 3). 5.3 Back-Etched Samples. 5.3.1 The Back-Etched Samples and I-V Measurement Set- Up Typical deposition parameters and some physical characterization of diamond films deposited for back-etched samples are described as follows. A mixture of methane and hydrogen, with flow rates of 0.75 sccm and 150 sccm respectively, was allowed to flow into the chamber and a gas discharge was maintained with 600 W microwave input power. The plasma pressure was 50 Torr and the substrate temperature was approximately 1000°C. Films were deposited on a sacrificial silicon substrate that were diamond powder polished. Scanning electron microscopy of the top surface of the resulting films showed well defined crystallites with an average grain size of 0.55 pm as determined by the linear intercepts method. A surface profile as measured by a stylus profileometer showed a standard deviation of 630 A. Raman characterization of the films, as illustrated in Figure 5.8, showed the characteristic diamond peak at 1332 crn’l and indicates an absence of appreciable non-diamond carbonaceous material. After deposition, dual side contacts were made to the top and bottom of the film as described in chapter 3 (section 5.3). The top metal contacts are circular with a diameter of 400 pm and approximately 20 contacts are on each transferred film. This effectively provides 20 two-terminal devices for electrical characterization, with the bottom contact being common to all devices. 131 RAMAN SPECTRUM SAMPLE: NDF-P47 888.00 Y . . . I . I 4* I—* I ”I r I n 1 795.00 ._ ,; _ r i . ~ -1 702.00 _. _ ~ 1 )- _ -4 1... H _ .I “2’ I “ .01 509.00 ._ H .- 2 H b— 516.00 L 423.11 . . . 1 :42 . . . 1 . . . . I I 430.00 700.00 990.00 1260.0 1540.0 1810.0 RECIPROCAL CM Figure 5.8. Raman spectrum of the diamond film as deposited on the silicon substrate with substrate temperature at 1000 °C. (From Dr. Gray) 132 The measurement set-up is illustrated in Figure 5.9. The sample was placed on the Signatone microprobe station. Current-voltage (I-V) characteristics were measured at room temperature, with and without photo-excitation. For voltages up to 100 V, an HP 4145B semiconductor parameter analyzer was used to collect the data, with a current resolution of approximately 100 pA. For higher voltages, a Tektronix 577 curve tracer was used. 5.3.2 Contact Effects on Back-Etched Samples In this study, Au, Ag, and In contacts were used in order to investigate the contact effect of different metal work functions. The work functions for Au, Ag, and In are 5.2 eV, 4.42 eV, 3.97 eV respectively [125]. For low voltages, less than 35 V, the I-V characteristic of powder-polished samples were nearly linear and symmetric for gold, silver, and indium contacts, as shown in Figure 5.10. For a film thickness of 3.5 pm, 35 V corresponds to an electric field of 105 V/cm. This indicates that for electric fields below 105 V/cm, the films exhibited predominantly ohmic behavior with a conductivity that was independent of the applied voltage for the high work function metal contacts (Au) and low work function metal contact (In). However, for large grain films described later in chapter 5 (section 4), results show that under certain conditions, metal-diamond contacts are non-ohmic and dominate device I-V characteristics. 5.3.3 'High Field Effect The combination of dual-side contacts and relatively thin films facilitates measure- ment of electrical properties at higher electric fields than have been generally reported for previous studies of diamond films with metallic contacts [126]. In the last section, it is shown that ohmic behavior was predominant at low voltages for different metal 133 WWWSWI 0850c» HP 4145 B Semiconductor Parameter Analyzer Tungsten .' Probe ~. / \ IJq-o-a“.—._s—--o-aq-n—o—-—o—o_-—-_u---o-c—s-s-o—o—-_.d / / ' Top Metal Contact ,° / . / Contact / / / Torr Seal /' l a/ . . L , Diamond Film / . ._ f _ Bottom Metal Contact , ammo. ./ ' AI Coating l.’ Si Substrate ,' ll ’ V ., Signatone Microprobe Station Figure 5.9. The I-V measurement set-up of the back-etched samples. \ < f 1“ Fig, and 5am] 134 6e - 09 T I I I I I > 412 — 09 - “ 2e — 09 )- ' “ s 0 a t: g —2e - 09 ‘- - S 0 -4e — 09 - ‘ -6e - 09 " -8e — 09 ‘ 1 1 ' l ' -20 -15 -10 -5 0 5 10 15 20 Voltage (V) Figure 5.10. I-V characteristics of a small grain size sample with gold contacts top and bottom. It shows linear and symmetric behavior at low voltages. (Electrical sample : P47-T1) C0 10 11C V0 CO: For 135 contacts. However, at high voltages, the current increases more rapidly than linearly, as shown in Figure 5.11. As shown in Figure 5.12 (a) and (b), current-voltage relationship did not follow the space charge limited current-voltage power law where in (a) I ocV3/ 2 and in (b) I ocV’. However, the nonlinear behavior at high voltages is well modeled by a voltage activated conductivity. The total dark conductance of the device may be expressed as G = Goo + Goexp(aV) (5.12) where the first term represents ohmic behavior corresponding to low field conduc- tion in the diamond film and second term represents the nonlinear behavior at high voltages, with V being the applied voltage and a representing the slope of the curve. Figure 5.13 and Figure 5.14 show that this model fits the data over the entire measurement range for both Au-Au contacts on the top and bottom, and In contacts on the top and Au contact on the bottom respectively. For both cases the diamond film thickness was 3.5 pm. At voltages higher than 250 V, a breakdown regime is entered in which a negative resistance state is followed by an irreversible breakdown. For voltages less than 250 V, however, no hysteresis in the I-V characteristic is ob- served. The experimental data is repeatable and the same for increasing voltage as for decreasing voltage. Since both contact combinations gave the same low and high field characteristics, the work function of the contact does not appear to contribute to the I-V characteristics of the small grain size samples. This result is consistent with some other reported work on metal-diamond contacts [127]. The slopes a of Figure 5.13 and Figure 5.14 are 0.042 V‘1 and 0.045 V‘1 respectively. Both Au-Au and In-Au contacts gave rise to nearly symmetric I-V characteristics and exhibited a low-field, constant conductance (ohmic) region with a conductivity ago. For Figure 5.13 and 136 -100 —50 0 50 100 Voltage (V) Figure 5.11. I-V characteristics of a small grain size sample with gold contacts top and bottom. It shows nonlinear behavior at high voltages. (Electrical sample : P47-T1) 137 1.8¢ - 07 T I T 1.6e -07 1.4e — 07 1.2e — 07 le—07 8e-08 Current (A) 6: -08 4e-08 2e-08 0.. 1.88 - 07 T r 1.6e - 07 1.4e - 07 1.2e- 07 1e-07 8e-08 Current (A) lie-08‘ 4e-08 2e-08 0 Voltage2 (V2) Figure 5.12. The I — V3/2 characteristic and (b) the I — V2 characteristic of Figure 5.11. (Electrical sample : P47-T1) fi sh C0 41 Hz of pr 3P V‘s II, 10 d8: “‘3 138 Figure 5.14, 000 is equal to 7.3x10“1 (fl-cm)”1 and 5.9x 10“1 (Q~crn)"1 respectively. For samples deposited at similar conditions with a thickness of 2 pm. Figure 5.15 shows that this model also fits the data over the entire measurement range for Ag- Ag contacts on the top and bottom. The breakdown regime happens at voltages higher than 150 V. The slope a of Figure 5.15 is 0.08 V“. The Ag-Ag contacts also gave‘rise to nearly symmetric I-V characteristics and exhibited a low-field, constant conductance (ohmic) region with a conductivity 0'00. For Figure 5.15, 000 is equal to 4.6X10“l (fl-cm)“. The slope a is approximately 0.045 V“ for a sample with a thickness of 3.5 pm. However, the slope a is 0.08 V“ for a sample with a thickness of 2 pm. For samples of varying thickness, the slope of the conductivity vs. voltage is found to be inversely proportional to the sample thickness, indicating that this increase is related to the applied electric field. Consequently, the conductivity may be expressed as o = 000 + ooexp(aF) = 000 + ooexp(F/Fo) (5.13) where F is the electric field and 0 represents the slope of the log of the conductivity vs. electric field and F0 is the inverse of the a. The value of a and F0 for Figure 5.13, Figure 5.14 and Figure 5.15 are 1.47><10'5 (V/cm)-1, 6.8)(104 V/cm; 1.58x10“5 (V/cm)"1, 6.3x10‘ V/cm; and 1.6X10'5 (V/cm)-1, 6.25x104 V/cm respectively. In order to investigate Whether the high voltage increase in conductance is due to an increase in dark carrier concentration or an increase in mobility, the voltage dependence of the photoconductivity was also investigated. A tungsten light source was used to illuminate the devices so that the current increased by an amount AIM. 139 1e — 05 : I I T I : Experiment 0 . . Model — 1 r J 1e—06 : A O “E v 16-07 _ v ' i ‘53 ‘63 5 le — O8 : "D I 1:: O 0 1e — 09 : 1e — 10 1 ' ' L o 50 100 150 200 250 Voltage (V) Figure 5.13. I-V characteristic of diamond film with gold contacts top and bottom. Experimental data is shown by data points. The solid line represents the model results of Eq. (5.12) with Goo=2.6x10“° 9“, Go = 2.1x10“l fl“, and a = 0.042 V“. (Electrical sample: P47-T1) 140 1e - 05 : I I I I E Experiment 0 ’ Model -— 1 112-06E 113—07: 1e-08: Conductance (mho) 16-09: 1e — 10 1 1 1 1 0 50 100 150 200 250 Voltage (V) Figure 5.14. I-V characteristic of diamond film with top indium contacts and bottom gold contact. Experimental data is shown by data points. The solid line represents the model results of Eq. (5.12) with Goo=2.lx10“° 9“, G0 = 2.0)(10’1l fl“, and a = 0.045 V“. (Electrical sample : P47-T3) 141 0.0001 I I I I I I I I ' Experiment 0 _ Model — le — 05 ,r A O I- E le — 06 g . v : 9 Q) . U 5 1e — 07 y +3 I: ’I U . =1 i E 1 08 ° _ - Q 0 e E ,s’ O , ‘s‘ § 3 + .s‘ \\ n—ogg .sy : 5).)“. ‘ 16 _ 10 1 1 1 1 1 1 1 l o 20 40 60 80 100 120 140 160 180 Voltage (V) Figure 5.15. I-V characteristic of diamond film with silver contacts top and bottom. Experimental data is shown by data points. The solid line represents the model results of Eq. (5.12) with Gm=2.9x10“° 0“, Go = 4.0)(10‘12 fl“, and a = 0.08 V“. (Electrical sample: P49-T2) 142 The photoconductance is defined here as GP}. = AIPh/V. (5.14) The results of the photoconductance are shown in Figure 5.16 for several photon flux intensities. In all cases, the photocurrent was less than 10 % of the dark current, and so may be considered as a small signal contribution to the total current. For a given light intensity, the photoconductance is GP}. = qAnphpA/t (5.15) where A is the area of the top contact, t is the film thickness, )1 is the carrier mobility, and An,”I is the increase in carrier concentration due to photo-excitation. Eq. (5.15) is written generally for any carrier type, that is Anph may refer to photo-generated electrons, or holes, or both. If the increase in dark conductivity at high voltages is primarily due to a field activated mobility, then the photoconductance would be expected to show a similar increase at high voltages. In fact, however, the data in Figure 5.16 shows that GP], is essentially constant with respect to voltage. Over the same voltage range, the dark conductance increased by approximately an order of magnitude. Consequently, the field activated dark conductivity seems to be primarily due to an increase in carrier concentration. An electric field activated conductivity has been previously reported in a wide variety of non-single crystal insulating and semiconductor films. A linear plot of the logarithm of the conductivity versus the applied field is evidence of Poole’s Law and is often interpreted as being a result of Poole-Frenkel reduction of the ionization energy associated with Coulombic potentials surrounding ionizable sites resulting from impurities, local non-stoichiometry, or defects. [128, 129, 130] The 143 16—08. I I I I I f I 999. 99.9 [00° —i N“? 1e—09 ‘I l 1e-10 _ Photoconductance (Arb. Unit) 1e—11 1 1 1 l 1 L 1 1 1 0 10 20 30 40 50 60 70 80 90 100 Voltage (V) Figure 5.16. The photoconductance is nearly independent of the applied voltage. Shown here are data for different photon fluxes corresponding to different optical density (O.D) filter values. (Electrical sample : P47-T1) 144 Poole-Frenkel mechanism causes an increase in conductivity due to an increase in carrier concentration, resulting from ionization of Coulombic centers by the applied electric field. This is consistent with our experimental evidence that it is a carrier concentration increase, not a mobility increase, that gives rise to the field activated conductivity. When Coulombic potentials may be considered as non-overlapping, their contri- bution to conductivity is proportional to exp(,BF1/2/kT) where 6 is the Poole-Frenkel constant, equal to e3/2(1r£)“/2, and F is the electric field [130]. However, when the Coulombic center density is sufficiently high that there is appreciable overlap of the Coulombic potentials, then the contribution of the Coulombic centers to the conduc- tivity is proportional to exp(ozF) where a is a function of temperature and distance between centers [130]. The conductivity exhibited by the films in this study are ex- amples of the latter case, as indicated by Eq. (5.13) and Figure 5.13 to Figure 5.15. A direct indication of the density of the Coulombic centers may be found from the slope of the log of conductivity vs. voltage in Figure 5.13 to Figure 5.15. From Hill, the expected slope would be es / 210T t where s is the separation of Coulombic centers (or defect centers) and t is the sample thickness. [130] For the experimental slope of0.045 V“ for t = 3.5 pm, the corresponding value of s is 4x10“ cm. Taking s to be equal to N “l 3 where N is the Coulombic center density, the value of N is 1.6x1019 cm“. The overlap of Coulombic potentials is a matter of degree, and setting a maximum separation for overlap is necessarily arbitrary. Following Hill, the maximum separation which still produces appreciable overlap may be taken, as an approximation, as twice the distance from a site to the maximum in the barrier. The lower limitation of the density for overlapping is (efl’1F'1/2)3 [130]. Taking ($13 = N = (efl'1F1/2)3 (5.16) 145 this approximation leads to a relationship between 3 and the electric field according to s = fl/eF1/2. As the electric field increases, this maximum separation decreases. For 3 = 4x10‘7 cm, the corresponding electric field is calculated to be 6x105 V/cm. This value is within the range of fields at which we observed field activated conductivity and, given the rough approximation used as an overlap criteria, is an indication that overlap of Coulombic potentials is a reasonable hypothesis at these densities. Since the lattice constant of diamond is 3.56721 and the lattice configuration is face center-cubic structure, the diamond crystal has 1.76><1023 atoms/m3. The calculated Coulombic center density corresponds to approximately one center per 10,000 host atoms. While this value is high by single crystal semiconductor standards, it would not necessarily be unexpected for polycrystalline films deposited by chemical vapor deposition. States at grain boundaries may be a contributor to these centers. Additionally, thin film deposition system purity considerations are also a factor in terms of impurity or defects states within individual crystallites. Because of the field activated conductivity, the current is substantially larger at high electric field than would otherwise be the case. The negative resistance observed prior to breakdown is evidence of thermal effects which apparently cause thermal runaway. For 3.5 pm and 2 pm thick films, this occurs at a voltage of 250 V and 150 V respectively. It corresponds to a breakdown field of 7.2x105 and 7.5x105 V/ cm. Consequently, the dielectric strength of the polycrystalline diamond samples in this study are substantially less than those reported for single crystal diamond (0.6 - 1x107 V/cm) [131]. 5.3.4 Photo Efl'ect If an incident photon has sufficient energy to excite a valence electron into the con- duction band, then, with a certain probability, that photon will be absorbed in the 146 material creating a hole-electron pair. Alternatively, a valence electron may be excited to a higher lying defect state, creating a free hole, or a trapped electron may be excited to the conduction band, creating a free electron. In any case, these photo-generated carriers, being in thermal equilibrium with their surroundings, recombine after some time, generally via trapping dynamics. During the lifetime of the photo-generated carriers, an increase in electrical conductivity will be observed. Photon absorption in high purity, single crystal semiconductors and insulators is generally characterized by an absorption edge which occurs at the minimum energy required to free a valence electron and cause band-to—band excitation. Below this energy there is little photon absorption, above it the absorption increases sharply. The presence of defects and impurities allow different absorption phenomena which may be exhibited by a tail on the absorption edge which extends into the energy gap, or by structure in the absorption spectra within the energy gap. This investigation studied photo-conductivity due to photon energies smaller than the energy gap, and therefore corresponding to excitation involving defects or impurities. In this research, two sets of optical filters, which are visible light filters and infrared filters, were used to study the photo-effect. The monopass wavelengths of the visible filters are between 412 nm and 714 nm and those of the infrared filters are between 775 nm and 1480 nm. Consequently, the covered range corresponds to photon energies between 3 eV and 0.84 eV. Before the measurement were conducted on the back- etched samples, the relative power density for each filter was measured. A Newport power meter (model 815) with Si photodetector (model 818-SL) and Ge photodetector (model 818-IR) were used to measure the power for photon energies above 1.2 eV and below 1.6 eV respectively. As shown in Figure 5.17 (a), a calibration factor was applied to the power meter for different wavelengths of light for each photodetector in order to get the accurate readings. Since the photon flux passing through each 147 filter is different, the relative power intensities corresponding to each filter are shown in Figure 5.17 (b). The photoconductance versus photon energy at -20 V and 20 V for the Au-Au contact sample is shown in Figure 5.18(a) before the normalization of the relative power intensity factors and in Figure 5.18(b) the normalized photoconductance versus photon energy is shown. Similarly, for the In-Au (In contact on the top) contact sample, the relationship of the photoconductance versus energy before and after the normalization are shown in Figure 5.19(a) and (b) respectively. For both the Au—Au contact sample and the In—Au contact sample, the relationship of photoconductance versus photon energy is nearly the same for positive and neg- ative bias. The existence of appreciable photoconductance well below the band gap indicates many defect states existing in the polycrystalline diamond films. The phe- nomenon of increasing sub-bandgap photo-conduction with increasing photon energy is also observed by a group with an international cooperation effort using a differ- ent approach [132]. They found that all CVD diamond films exhibited an almost monotonically increasing absorption withiincreasing photon energy. As the absorp- tion increases, the generation of electron-hole pairs increases and the photo current increases. 5.4 The Metal/ Diamond/ Silicon Samples 5.4.1 The I-V Measurement Set-up The metal / diamond / silicon samples as described in chapter 3 (section 5.2) were placed on the Signatone microprobe station as shown in Figure 5.20. Current-voltage (I- V) characteristics were measured at room temperature, with and without photo- excitation. As for the back-etched samples, an HP 4145B semiconductor parameter 148 (a) m T I I T I Si Detector 9- A Ge Detector 4- '2 700 " «A D .5 coo , « l- < v .1 h 500 ' 3 .2 .... . = .9. - 3 300 i- :2 ‘3 200 - - D 100 1 1 1 1 l 400 ' 600 800 1000 1200 1400 1600 Wavelength of Optical Monopass Filter (nm) (b) Normalization Factor (Arb. Unit) 1 L 1 0 1 L 400 600 800 1000 1200 1400 1600 Wavelength of Optical Monopass Filter (nm) Figure 5.17. (a) The calibration factors corresponding to different optical wavelength for Si and Ge photodetector. (b) The relative power intensity factors for Si and Ge photodetector at different wavelength of the optical'monopass filters. 149 18 - 08 _ I I I I r bin: 20V 0- ? : hilt-20V '0- I G . . :D I- E 1 < > . v 4 8 4 a la - 10 F '5 o E 1 a ’ 1 '5 P I t: » J g le - 11 l:- 1 a t 1 O I . .3 r 1 D- * 1 le — 12 * E 1 ‘ L 0.5 l 1.5 2 2.5 3 3.5 Photon Energy (eV) 16 - 08 ’ T I— I T r j ’ bias: cows; Detector) e- A bias: 20V(Ge Detector) E— .‘u': ' bi8:-20V(5i Detector) ~0— 5 * biu:o20V(Ge Detector) --- . lc - 09 ;- -° I . h ’ < . v ’ 8 5 1e - 10 :- 1 U + . z . l 'U . 8 0 1e - 11 f 1 § E a ..r: I 1 0.. . 4 1c - l2 ' 4 i ‘ 1 1 0.5 l 1.5 2 . 2.5 3 Photon Energy (eV) 3.5 Figure 5.18. Relation of photoconductance vs. photon energy for Au-Au contact sample (a) before normalization and (b) after normalization. (Electrical P47-T1) sample : 150 18 -08 ’ I I I r I A E bias: 20v 9- i .2 ’ biuz-20V -e— < = ' ‘ D ‘9' 1c - 09 r 1 l- , I < I I v > 4 v ‘ o l g lc - 10 .- 1 U ; . = W '5 l j = . . 8 0 1c — ll :- 1 a : : O . . .2 l G- r 4 r 4 1c - 1?. ‘ ‘ ‘ ‘ ' 0.5 1 1.5 ‘2 2.5 3 3.5 Photon Energy (eV) 19 — 08 I I I f I E bin: 20V(Si Detector) 0- ' bias: 20V(Ge Detector) B- ’ biu:-20V(Si Detector) o— ’ biu:o20V(Ge Detector) Q— l 3 l J 4 lc-OQF Photoconductance (Arb. Unit) 1e - 10 )- lc - ll :- 1 E 1 . 1 1c - l2 1 ‘ 1 ' 0.5 l 1.5 2 2.5 :3 33.5 Photon Energy (eV) Figure 5.19. Relation of photoconductance vs. photon energy for In—Au contact sample (a) before normalization and (b) after normalization. (Electrical sample : P47-T3) 151 analyzer was used to collect the data with a current resolution of approximately 100 pA. In all cases, p-type silicon was used as the substrate. 5.4.2 Contact Effects on Metal/Diamond/ Silicon Samples There are two ways of fabricating the metal/ diamond/ silicon samples as previously mentioned in chapter 3 (section 5.2). The I-V characteristic of the large grain size diamond samples (paste-polished samples) with Al contacts and the small grain size diamond samples (powder-polished samples) with Au, Ag, and In contacts will be described and compared to the results reported in the last section for back-etched samples. Silver paste was used to form contact on the back side of the silicon wafer. For the p-type silicon used here, the paste contact was ohmic. For low voltages, less than 25 V, the current-voltage (I-V) characteristics were nearly linear and symmetric for all the Au, Ag, and In contacts as shown in Figure 5.21 and Figure 5.22 on fine grain, diamond-powder prepared samples. It is strongly believed that in these small grain size diamond films, the defect state density is so high that the tunneling process dominates the metal/ diamond contact I-V properties. Consequently, ohmic behavior is observed for both high work function metal contacts (Au) and low work function metal contacts (In) of the metal/ diamond contact. This is consistent with the metal / diamond contacts on the back-etched samples. The data in Figure 5.21 and Figure 5.22 also indicate that there is no rectifying behavior at the diamond/silicon interface. On the diamond side of this interface, it is reasonable to assume that, if a barrier did exist, a high defect density again produces such a thin barrier that tunneling allows ohmic behavior. For the silicon, the starting wafer which has been severely abraded as shown in Figure 3.5. Con- sequently, the defect density in the powder abraded silicon is also expected to be high, which would result in a silicon barrier that was also sufficiently thin to tun- 152 WMWWI odors HP 4145 B Semiconductor Parameter Analyzer Tungsten / Probe \ /_._._._._._...4.-._._._._._._._._._.-._._._.-.-.-.-..] /AlDot ', AAAAAAAAAAAAAAAAAAAAAAAAAA / Diamond Film _/ /P-typeSi /‘ /Ag Paste /’ b.-._.‘.—._u-.—._----._.---v—.-.—.—e-e—o—o_u_.-._.o Signatone Mlcmprobe Station Figure 5.20. The I-V measurement set-up of the metal/ diamond/ silicon samples. 153 nel through. In fact, several decades ago, ohmic contacts to semiconductors were sometimes made by abrading the semiconductor with sandpaper in order to create a defect-laden surface. Alternately, the lack of a rectifying barrier may also be due to a lack of appreciable band bending in the silicon. As will be elaborated on later, the results of photo-excitation experiments described in the next section indicate that thereis no significant band bending in the silicon, either for powder-polished samples or for paste-polished samples. In contrast to the powder polished, small grain samples, for the large grain size paste-polished diamond samples, the I-V characteristics of the Al/diamond/silioon structure showed rectifying behavior as shown in Figure 5.23 and Figure 5.24. This indicates that the defect density is not as high as in the small grain size diamond films. It is reported that polycrystalline diamond films have a much higher defect density than the single crystal, and the concentration of defect increases as the concentration of methane increases [132]. This research indicates that different nucleation tech- niques and/ or different grain sizes are also factors contributing to defect states in the films. Rectifying phenomena of metal / diamond/ silicon structures have been previously reported by several groups [133, 134] in recent years, and similar behavior was also ob- served for bulk boron-doped diamond synthesized under ultrahigh pressure conditions [135]. The rectifying property has been variously attributed to the band bending at the top-contact / diamond interface [133] and back-contact/diamond/silicon interface [134]. It is important to know which interface in fact contributes to the rectifying characteristics in our case. Further investigation using additional information from photo-excitation will be discussed in the next subsection. 154 00m15 F I I I I I I 1 0.0001 A 5c — 05 :5. ‘5 o 2’. I- :3 0 -5e - 05 -0.0001 l l 1 1 i 1 1 -0.00015 L . --25 -20 -15 -10 -5 0 5 10 15 20 25 Voltage (V) Figure 5.21. I-V characteristic of the small grain size Au/diamond/silicon samples. (Electrical sample : P39) 155 16-05 I 1* I I I I I I 7 8e—06 - .. '6c-06 - - A 4c—06 P ' " < . V g 2e—06 - t- ‘5 0 O —2c-06 - ~ -4e-06 - ‘ —6e-06.~ . ‘ -86-06 I l J L L 1 l 1 -25 -20 -15 -10 -5 0 5 10 15 20 25 Voltage (V) Figure 5.22. I-V characteristic of the small grain size In/diamond/silicon samples. (Electrical sample : P39) 156 113-09 —1e—09 -2c-09 -3e-09 Current (A) —4e-09 —5e-09 -6¢ _ 09< 1 1 L 1 1 1 1 1 -25 -20 -15 —10 -5 0 5 10 15 20 25 Voltage (V) Figure 5.23. I-V characteristic of the large grain size Al/diamond/silicon samples. The average grain size is 2.1 pm. (Electrical sample : P6) 4c-06 157 2e—06 - 0 -2¢ — 06 —4e — 06 -6e - 06 -8e - 06 —1e - 05 -1.2e - 05 —1.4e — 05 -l.6e — 05< —1.8e - 05 Current (A) l l l 1 l l —25 —20 —15 -10 —5 0 5 10 15 20 '25 Voltage (V) Figure 5.24. I-V characteristic of the large grain size Al/diamond/silicon samples. The average grain size is 1.4 pm. (Electrical sample : P7) 158 5.4.3 Photo Efl‘ect The experiments of the photo effects on the metal / diamond / silicon samples used the same method and technique as that described in chapter 5 (section 3.4). Figure 5.25 and Figure 5.26 show the relationship of photoconductance versus photon energy for the small grain size Au/ diamond/ silicon sample and the small grain size In/ diamond/ silicon sample respectively. Similarly, the photoconductance versus photon energy characteristics for different large grain size Al/ diamond/ silicon samples are shown in Figure 5.27, Figure 5.28 and Figure 5.29. If the rectification happens at the diamond/ silicon interface and is a result of silicon band bending, then silicon should play a role in contributing to the photo current. Consequently, the photo current should abruptly increase as the photon energy increases above 1.1 eV, which is the energy gap of the silicon. However, in both large and small grain size metal/ diamond / silicon samples there are no indications that photoconductance abruptly increases at photon energies above 1.1 eV. This showed that the rectifying properties are not contributed by the diamond/ silicon interface but rather by the Al/ diamond interface and that band bending happens at the Al/ diamond interface. It is also observed that a negative bias did generate more photo current than a positive bias in Figure 5.27, Figure 5.28, and Figure 5.29. Figure 5.30 shows a possible energy—band diagram of the Al/p-type diamond interface. During the photo-excitation the valence electrons are excited into the higher lying acceptor level creating more holes in the valence band. Since the band bending happens at the Al / diamond inter- face, that a negative bias drawing more photo current from the diamond is reasonable. Generally, this research indicates that large grain size diamond films prepared by the paste-polished method provided better metal/ diamond rectifying properties 159 13 - 06 I I I T T ’ bill: 15V 0- ‘ biee:-15V -- 1 A 1 .".'.’. G , 3 J A. P i . g Q 3 “U , 4 G 8 3 O ...: G... Ic - 07 ‘ 1 f ‘ ‘ 0.5 l 1.5 2 2.5 3 3.5 Photon Energy (eV) (b) 18 - 05 P I I I I T : bias: 15V(Si Detector) 0- . bin: 15V(Ge Detector) G- . bile:-15V(Si Detector) -e- , biuz-15V(Ge Detector) O- I A A A AA Photoconductance (Arb. Unit) 1c - 06 :- 1 ' 1 1c - 07 4 ‘ i ' 4 0.5 l 1.5 2 2.5 3 3.5 Photon Energy (eV) Figure 5.25. Photoconductance versus photon energy (a) before normalization and (b) after normalization for the small grain size Au/ diamond/ silicon sample. (Electrical sample: P39) 160 (a) 18-07 I I I I I bin: 15V 0- ’ biuzolsv 4- t P 4 Photoconductance (Arb. Unit) 1‘ - 080.5 i if: 2 2:5 3 3.5 Photon Energy (eV) (b) 1e - 06 I r . bite: 15V(Si Detector) @- . bill: 15V(Ge Detector) B— . . biee:-15V(Si Detector) «o— biee:-15V(Ge Detector) o— 1 LA A Photoconductance (Arb. Unit) 1c — or r 1 i 1 P J 1‘ - 08 4 ' 1 1 1 0.5 1 1.5 2 2.5 3 3.5 Photon Energy (eV) Figure 5.26. Photoconductance versus photon energy (a) before normalization and (b) after normalization for the small grain size In / diamond / silicon sample. (Electrical sample : P39) 161 13 - 06 I I I I I I bin: 15V 0— 1 c ; him-15V .- j 5 le - 07 r 1 3?; . 1 1c - 08 r $ ‘ i o ’ I U D 5 1c - 09 g- 1 a : . U D g D 1 5 1c - 10 )v 1 o » 1 O I , fl .2 1c — 11 g- 1 D... E i r 1 r J 1e - l2 1 l 1 1 4; ' 0.5 l 1.5 2 2.5 3 3.5 Photon Energy (eV) 16 - 06 r I I I I : his: 15V(Si Detector) O- : c : bin: 15V(Ge Detector) €- 1 .E 1 07 bi.:-15V(Si Detector) -e- D c ' 1’ hint-15V(Ge Detector) O- 1 e i 3 1c - 08 .3 1’ ‘ I o P Q P 5 1c - 09 g- 1 a P : o ; 1 e . . 1 — 10 8 ‘ E 1 Q r I o 1 . a 2 1c - 11 g' 1 le - 12 1 l 1 l 1 0.5 l 1.5 2 2.5 3 3.5 Photon Energy (eV) Figure 5.27. Photoconductance versus photon energy (a) before normalization and (b) after normalization for the large grain size Al/ diamond/ silicon sample. The average grain size is 2.1 pm. (Electrical sample : P6) 162 (a) 18-06 1 I I fl I I .11 le—07: Photoconductance (Arb. Unit) 1c - 08 :- 1 lc - 09 ' ‘ 1 1 1 0.5 l 1.5 2 2.5 3 23.5 Photon Energy (eV) 13 "' 06 I I I I I 4 bill: 15V(Si Detector) o- 1 A ) bite: 15V(Ge Detector) e- . f: F bieez-15V(Si Detector) ce— ‘ 1: . bieez-15V(Ge Detector) e- * ED . 'e lo - 07 r 1 < : v > 8 : E , U 5 E lc - 08 E- 1 c r e: O- . 1e - 09 m 1 1 1 1 0.5 l 1.5 2 2.5 3 3.5 Photon Energy (eV) Figure 5.28. Photoconductance versus photon energy (a) before normalization and (b) after normalization for the large grain size Al / diamond/ silicon sample. The average grain size is 1.4 pm. (Electrical sample : P7) 163 19 - 05 I I I I I ‘ bin: 15v 0- 3 E? : bias-15V -e- j = .. D 16 w E - - : 2 #2 t a e; = r < 1: - 07 g- 1 8 i . U * I Ila " 4 g M“ W 1, u E : o 4 ‘5 i i ‘ _= 1: - 10 f o. a 3 1e -— 11 ‘ 1 ‘ ‘ ‘ 0.5 l 1.5 2 2.5 3 3.5 Photon Energy (eV) 0.001 r r l l r I bill: l5V(Si Detector) O- A ' bin: 15V(Ge Detector) Q- ‘ =3 °~°°°1 { munavm Detector) ..— 1 :5 E biu:-I5V(Ge Detector) O— : , le - 05 .o F l t- ; j 5. 1e - 06 F 1 q; I : U ’ 4 g le - 07 r '1 a E i g b . “U 1: - 08 g- 1 s E 5 8 1c - 09 r 1 a ’ : .2 . . 1e - 11 L l l L 0.5 l 1.5 2 2.5 3 3.5 Photon Energy (eV) Figure 5.29. Photoconductance versus photon energy (a) before normalization and (b) after normalization for the large grain size Al/ diamond/ silicon sample. The average grain size is 1.1 pm. Electrical sample : P20) 164 A' Diamond 7 5° 7 ----- FF++4————EF (')%7(__.£x {r o {g g, Ev ‘ //4 ........................................... Figure 5.30. The energy band diagram in the Al/p-type diamond interface. 165 than the small grain size diamond films prepared by the powder-polished method. However, it doesn’t mean that the larger the grain size the better the rectifying properties, independent of other variable. In this work, the sample which has the best rectifying properties is not the sample with biggest grain size diamond crystal. The degree of rectifying is also dependent on other properties of the metal / diamond interface. Details of studies on the device with the best rectifying properties in this study will be discussed in the next subsection. 5.4.4 Diamond Schottky Barrier Diode The best metal/diamond/silicon rectifying structures were prepared by the paste- polished method. The best of these rectifying characteristics were formed on film N DF -P20, deposited at conditions of 700 W microwave input power, 60 Torr pressure, 1 % methane/ hydrogen concentration (1.5 sccm : 150 sccm). Typical I-V characteris- tics of the tungsten point contact / diamond / silicon and Al / diamond / silicon structures on the film are shown in Figure 5.31 and Figure 5.32 respectively. The Raman spec- trum of N DF -P20 is shown in Figure 5.33. The point contact structure shows the ohmic behavior which again supports the mechanism that the rectifying property is a result of the Al/diamond interface. When two coplanar contacts are made, with one contact being the evaporated aluminum circle and the other being the tungsten point probe, SBD characteristics are again observed as shown in Figure 5.34. In this case the current passes via the rectifying diamond/Al contact through the diamond film to the silicon, through the silicon, and back up through the diamond film to the ohmic tungsten point contact. V Figure 5.35 shows that the forward bias current (1;) to the reverse bias current (In) ratio at 10 V is almost 2x105. However, the ratio drops to 2x102 when the voltage increases up to 25 V. Similar phenomena have been reported by other groups 166 8e-O5 66-05 48—05 2? 2.3—05 +3 5 o t-a S O -2e-05 —4e - 05 -63 - 05 —86-05 1 l l l l l l l —25 —20 -15 —10 —5 0 5 10 15 20 25 Voltage (V) Figure 5.31. The LV characteristic of the point contact/diamond/silicon structure showed ohmic behavior. The top contact is a tungsten point probe and the bottom contact is the silicon wafer. (Electrical sample : P20) 167 53‘05 I I I fl I I I I -5e — 05 —0.0001 —0.00015 I Current (A) -0.0002 _0.00025' m i 1 1 1 i 1 L 1 -25 -20 -15 -10 -5 0 5 10 15 20 25 Voltage (V) Figure 5.32. The best Schottky barrier diode (SBD) characteristic of the large grain size Al/ diamond/ silicon samples. The top contact is aluminum and the bottom con- tact is the silicon wafer. (Electrical sample : P20) 168 100000 J ' I ' I ' I ' l ' l ‘ I u 5‘ 80000 - - U! C 0 fl .5 60000 - .. A L l L l l l 1 A L I L l 400 600 800 1000 1200 1400 1600 wavenumber (cm") Figure 5.33. The Raman spectrum of N DF-P20. The peak between 1550cm‘1 and 1600cm'l indicates that the existence of graphitic component in the film. 169 58-06 I I I w I I I I 0 -5e—06 —le—05 —1.5e-05 —2e-05 -2.5e — 05 Current (A) —3e — 05 -3.5e - 05 —4e - 05< l l l —25 -20 -15 -10 --5 0 5 10 15 20 25 —4.5e — 05 L ‘ 1 1 Voltage (V) Figure 5.34. The SBD I-V characteristic of a film with coplanar surface contacts. One contact is aluminum and the other contact is a tungsten point probe. (Electrical sample : P20) 170 [76, 80, 137]. It is noted that the samples of [76, 80] are intentionally boron-doped and the samples of [133, 136, 137] and of this research are self-p-typed-doped during the deposition. The current-voltage results of the diode are best analyzed by considering the current as a function of both the voltage across the junction and the voltage across the bulk region. For the former IzIoexp(qu/nkT) (5.17) where V,- is the junction voltage, 17 is the diode ideality factor (1 S 17 S 2), T is temperature, I: is Boltzmann’s constant and 10 is the saturation current. Then for any current, the junction voltage is found to be __nk_T Vj q ln(I/Io) (5-18) and the bulk voltage is next found from ill) = VApplicd " V7 (519) Consequently, the forward I-V characteristic of the total structure is modeled by nkT v = _q_1n(1/10)+ f(I) (5.20) where Vb = f (I ) represents the I-V characteristics of the bulk material. In its simplest form, the relationship between the bulk voltage and the current would be ohmic, v. = IR (5.21) 171 0.001 r T 0.0001 le - 05 1e — 06 ‘3. 1 . 0 E 1) . 1e - 07 0 ‘5 Q5 lc - 08 0 (5 Current (A) le-09 le—lO le_11 l 1 l L l l l l —25 -20 —15 —10 —5 0 5 10 15 20 25 Bias Voltage (V) Figure 5.35. The log(I)-V characteristic of the SBD. (Electrical sample : P20) 172 where R = pL/A is the resistance of the diamond film. However non-ohmic behavior is often observed in diamond films, an example being the field activated conductance reported in chapter 5 (section 3.3) of this research. The data to be modeled by Eq. (5.20) is the forward l—V characteristic of the diode shown in the semilogarithmic plot of Figure 5.36. The parameters used in fitting the equation to the data are 10, 17, and the functional relationship f(I). The data shown in Figure 5.36 doesn’t show any straight line region in which the I-V characteristics are dominated by the diode portion of Eq. (5.20). For all currents in the range of measurements, the bulk voltage plays a major role in the total voltage. However, two straight lines representing the diode portion of the voltage are superimposed on the plot of Figure 5.36 which are consistent with the measured data. These straight lines correspond to quite different Io and n values. The solid line shows the diode voltage versus current for 10:5.2x10‘16 A and for n = 1. The dashed line shows the diode voltage versus current for 10:2.9x10‘“ A and for 17 = 2. As will be shown below, both lead to similar conclusions about the bulk I-V relationship, f(I). One might expect that the f(l) relationship would follow the field activated con- ductivity model of Eq. (5.12). However Figure 5.37 shows that this is not the case. Above 10 V the data is consistent with a field activated conductivity with Fo=6x104 V/cm, consistent with the field activated model. However, below 10 V the model does not fit, since the conductivity decreases rapidly instead of approaching a con- stant value. The data is better fit by assuming a power law for f(I) where loch'" (5.22) which m is the degree of power. As shown in Figure 5.38 and Figure 5.39 both m=3/ 2 and m=2 give a reasonable fit to the data, with the m=3/2 fit being marginally 173 0.01 I I I I : Experiment 9- ’ Ideal diode: 17:1 — 0-001 ,r Ideal diode: q=2 0.0001 g 5 ' ' A 1e —05 E 5 <1 , 3 .~, :: le — 06 r 3 4:" a E I 0 Q , : 4! : le — 07 I ‘1’ 5 E .0 0 1e — 08 r3 so 1e — 09 ° 1c — 10 I 18 _ 11 D _L 1 L l 0 5 10 15 20 25 Bias Voltage (V) Figure 5.36. The forward bias I-V characteristic of the SBD. The 0 represents the experimental data, the solid line shows the ideal diode with 17 = 1, 10:5.2x10‘16 A and the dashed line shows the ideal diode with 17 = 2, Io=2.9x10"“ A. (Electrical sample : P20) 174 0.0001 E . , I I . : Bulk Voltage(17=1) — 5 Bulk Voltaga(n=2) - - - - 4 A . lc — 05 :- _ o : — 1 F: I E 1 V 8 le - 06 E _ E g u .. “c 1e -- 07 1 C: I - 1 O ’ 2 U h 16 — 08 _: 16 - 09 l 1 1 1 0 5 10 15 20 25 Bulk Voltage (V) Figure 5.37. Conductance-bulk voltage characteristic. It follows the field activated model above 10 V. (Electrical sample : P20) 175 better. The energy band diagram and the equivalent circuit of the SBD are shown in Figure 5.40(a) and (b) respectively. The exact choice of Io and 17 is not critical to the fits since the diode portion of the voltage drop is relatively negligible, especially at the higher range of voltages. The range of Io values corresponds to a barrier height range of between 1.1 eV and 1.2 eV. The significance of the power law dependence may be considered further as fol- lows. Lampert and Mark loosely defined materials with band gap E, S 2 eV as semiconductors and those with E, > 2 eV as insulators [138]. By this definition, un-doped diamond with E9 = 5.5 eV can be considered as an insulator. In a perfect trap free solid state insulator, the space-charge limited current-voltage relation can be expressed as IocV2 (5.23) rather than the V3/2 . In considering the difference it is noted that the derivation of Eq. (5.23) is based on the assumption that carriers drift at a velocity, v, with v = pE (5.24) where p is carrier mobility and E is applied electric field. However, if the field strength is too high, the drift velocity of the carriers may vary as the square root of the applied electric field when above a certain critical field strength E, [138]. This is known as a characteristic of ”warm” carriers when acoustic phonon scattering is dominant. Then for E > 15., v = p(EE,.)1/2 (5.25) The current-voltage relation becomes maxi/Wm , (5.26) 176 0.0003 T I I I I Bulk Voltage 71:1; — Bulk Volta; 71:2 0.00025 , . ‘ I r 0.0002 I 0.00015 Current (A) 0.0001 5e—05 I 0 l 1 l l l - 0 20 40 60 80 100 120 Bulk Voltage3/2 (V3/2) Figure 5.38. The I-Vb3/2 characteristic of the SBD. (Electrical sample : P20) Current (A) 177 0.0003 1 I I I 1 Bulk Voltage(q=l) .— Bulk Voltage(q=2) 0.00025 r 4 0.0002 - - 0.00015 - - 0.0001~ — 5e - 05 - '1 0 i l l L l 0 100 200 300 400 500 600 Bulk Voltage2 (V2) Figure 5.39. The I-VI,2 characteristic of the SBD. (Electrical sample : P20) 178 Al Diamond / W..NFPW.N.—IP.N.-w.wr- — —— -—— ————— EA *— 5‘1 0 .. .’ 'I . _. .' _. .' .1 ..1 ... .. .. .. .. .. .. .. .. . t'-.‘-.--.‘-.~-.--.‘-.'-.'-.'- .......... ......... . .. .. .. .. .. .. .. .. .. . ...., .,_....._. _. . . . ‘. ..'I . . .° .".".".' e I' 'I- .- '.0 ‘I- '.- ‘.- '.v '.- ‘.- I. . .......... .. .. .. .. .. .I .. .. .. .. - v.,-.,-.,-.,~._-._-.,-c.'-.'. .' ‘.“.‘.',..'..I"hl',l.‘,'.'...‘..-'.. . , ...... .. .. .. .. .. .. .. .. .- . ‘ .,-o,-.,-. -._-.,-._e.,-I.'. ......... .1, ... .__ ._‘ ... '.- .1, ._, ... b. * . I. o. u 4.... g . .~ 0.. ........................................................ |~.,-..-.,-..'._~.,-.,-..-..-. ......... .............. .................. ............................. f(I) {<1 I I zIoexp(qV,- / nkT) I 0: VI,” Figure 5.40. (a) The energy band diagram of the SBD. The barrier height d), equals to the sum of built-in potential V.- and activation energy Ea. (b) The equivalent circuit of the SBD. 179 which has the same functional form as the observed data. For single crystal diamond, the high field phenomenon happens above 1x10s V/ cm. In this case the film thickness is about 4 pm, so a voltage of 10 V corresponds to an electric field of 2.5x10‘ V/ cm. The high field effect might not contribute to the phenomenon observed here. An obvious point is that the powder-polished samples of chapter 5 (section 3.3) fol- low a field activated conductivity and exhibit ohmic, non—Schottky behavior whereas the paste-polished samples of this section follow a power law I-V and Schottky behav- ior. Both of these observations are consistent with the hypothesis that the powder- polished films have a larger defect concentration. Consequently, metal / diamond space charge layers are sufficiently thin to allow tunneling and ohmic behavior and their high field properties are dominated by ionizable defects. I It must also be noted, here that some of the SBD exhibited a particular form of I instability. The current becomes much smaller after several times of measurements. However, the rectifying behavior still exist. Capacitance versus frequency measurement were also performed on the Al/ diamond/ silicon diodes with a HP4192A impedance analyzer and the data is pre- sented in Figure 5.41 for different values of reverse bias. The barrier height 45, can also be determined by the capacitance versus voltage measurement. By plotting l/C'2 against reverse bias, one can get built-in potential V.- from the extrapolated intercept on the horizontal axis. From the slope of the straight line one can also calculate the doping concentration. As shown in Figure 5.40(a) the barrier height (13,, can be found from psi/,- + E, (5.27) where E, is activation energy. However, from Figure 5.42 the data shown did not lie 180 1e—07 . . if...” T shun, f . . ”m, r . . .... bias: -1V 0 bias: 0V ‘1' bias: IV D ‘ _ bias: 2V X _ 16 08 o bias: 3v A bias: 4V * I A + o bias: 5v o - hut (>0 . " Q) +%> : g D + . C] if. '3 the" o 3 161-10 0 x ‘1' o i . am We 0 044m 5 ER“ le-ll 16-12 1 . A..1LLL 1 r 1...”! A .4..Lui 1 10 100 1000 Frequency (KHz) Figure 5.41. Capacitance versus frequency characteristic at different reverse bias. (Electrical sample : P20) 181 in a straight line. This may indicate that the self-doping of the film is non-uniform. Consequently, the barrier height can not be determined from Figure 5.42. In Penn State University’s work [133, 136, 137], they determine the ideality factor as 1.8, and the barrier height as 1.15 eV for Al and Au contacts to p-type CVD diamond films. They were not able to determine barrier height from the I-V curve, instead they use the technique of internal photoemission to determine the barrier height. In H. Shiomi, et al.’s work [76], an ideality factor of 2.1 and barrier height of 1.2 eV were all determined from the I-V measurement of the W contact to boron- doped diamond films. They noted that barrier height could not be obtained from C-V curve due to the high series resistance in the bulk. In D. G. Jeng, et al.’s work [80], they noted that an ideality factor of 1.85 was determined from the low voltage region (0.1-0.5 eV) slope for the Al/ diamond Schottky diode. It is obvious that the understanding of the synthetic diamond film diodes is still preliminary. Many factors contribute to the film properties and since the deposition conditions are so different from group to group, more experiments are needed to further investigation. 182 5 I I —I— F I I A ‘7’ 4' in ‘1: :L 3‘ “I' 8 5 2‘ :2 8‘ 1. O o l 1 l L 1 L -3 -2 -1 0 l 2 3 4 5 Bias Voltage (V) Figure 5.42. Capacitance versus reverse bias characteristic at 50 kHz. (Electrical sample : P20) CHAPTER 6 Summary and Future Research 6.1 Summary of Important Results The application of the microwave plasma disk reactor (MPDR) chemical vapor depo- sition system for diamond synthesis has been successfully developed. Good quality polycrystalline diamond films have been successfully deposited and characterized on silicon and silicon nitride substrates. Two sample preparation methods, which are paste-polished and powder-polished nucleation techniques have been used for deposit- ing large grain size diamond films and small grain size diamond films respectively. A back-etching processing technique was also developed to isolate the deposited dia- mond films from the silicon substrate in order to study the diamond/ silicon interface and allow access to evaporate metal contacts on both sides of the diamond films in order to study the electrical properties of the diamond films. A goal of this research has been to provide an increased understanding about the relationship between properties of thin film diamond and the preparation conditions. Toward this purpose several important physical characterizations of the diamond films, such as Raman spectroscopy, X-ray photoelectron spectroscopy, DekTak pro- file measurement, scanning electron microscopy, and laser scanning: microscopy were 183 184 carefully studied (see chapter 4). A particular focus of this research has been on the electrical properties of the films, and consequently several important electrical prop- erties of the diamond films, such as activation energy, I-V characteristics, high field effect, and contact phenomenon were also studied (see chapter 5). The importance of preparation conditions on the nature of metal contacts is described in chapter 5 and new information about the relationship between defects and high electric field properties is provided by this research. The following subsections provide specific summary highlights. 6.1.1 Nucleation Method The nucleation method is’important for the diamond synthesis since as was shown in this research, the density of nucleation sites is a major factor in determining the grain size of the diamond films. The paste-polished nucleation method produced comparatively larger grain size di- amond films than the powder-polished nucleation methods did since the latter method provides many more nucleation sites than the former method. It was also observed experimentally that the average grain size obviously increased as the methane con- centration increased for the paste-polished nucleation method but not the powder- polished nucleation method. For both nucleation methods, the average grain size of diamond increased as the microwave power or plasma density increased, but the effect was smaller than the effect of increasing methane concentration in the case for the paste-polished nucleation method. For both methods, the growth rate of diamond increased as methane concentration increases. The growth rate also increased as the microwave power or plasma density increased, however, the effect was smaller than the methane concentration. At the same deposition conditions, the growth rate of diamond by the powder-polished nu- 185 cleation method is slightly higher than that by the paste-polished nucleation method. 6.1.2 Quality of Diamond Films Raman spectroscopy is used as the major technique to distinguish the quality of the diamond films. The reported natural diamond peak is at 1332 cm“. The larger the Raman signal at 1332 cm“1 and the smaller the other peaks, the higher quality of the diamond films. It is known that the temperatures for depositing good quality diamond films is a critical variable for diamond synthesis. If the temperature is too low, an amorphous diamond-like component can become dominant and graphite becomes dominant instead of diamond if the temperature is too high. Generally, from this research it was observed, based on Raman results, that at lower methane concentration one can get good quality diamond films in a wider temperature range than at higher methane concentration. It was found that for the range of power and pressure investigated, the preferential temperature range for good quality diamond films is between 1030 °C and 1060 °C. It was also noted that the two nucleation methods, under the same deposition conditions, appears to make no obvious difference in the quality of the diamond film. 6.1.3 Back-Etching Technique For film characterization, it is advantageous to have access to both sides of the film. In this research, a back-etching process was successfully developed in cooperation with Dr. Engemann at the University of Wuppertal (Germany) to transfer the diamond film from the silicon substrate to an epoxy substrate. There are two kinds of back-etched samples fabricated by this technique. One kind of samples were used for physical characterizations (specifically XPS) of the back surface (diamond/silicon interface). The other kind of samples were processed 186 to have metal contacts on both sides of the film for electrical property studies of the diamond film. 6.1.4 Diamond/ Silicon Interface From the back-etched samples prepared by the paste-polished nucleation method, it is found that a thin layer of SiC existed at the diamond/silicon interface by X-ray photoelectron spectroscopy analysis. This supports the hypothesis that the formation of a thin layer of SiC is an inherent part of the growth of diamond on the silicon substrate. 6.1.5 Activation Energy of Diamond Films A four-point probe technique was used for sheet resistance measurements of the di- amond films. Diamond films were deposited on an insulating composite material, silicon nitride (Si3N4), using both paste-polished and powder-polished nucleation methods. All the diamond films were determined as p-type by the hot probe tech- nique. The sheet resistance for the as-deposited samples prepared by the powder-polished nucleation method was on the order of 105 to 106 9/0. By varying the temperature for the sheet resistance measurement, activation energies of 0.22 to 0.31 eV and 0.13 to 0.23 eV were obtained for carrier mobility equals to 1200 and 12 cm2/V-s respectively (see chapter 5, section 2.4). The samples were then annealed in a nitrogen ambient furnace at 500 °C' for one hour. This caused the sheet resistance to increase by at least four orders of magnitude and the activation energy to increase as well. However, the sheet resistance of the as-deposited samples prepared by the paste- polished nucleation method was on the order of 10‘ fl/D. This occurred because a different system shut off procedure caused formation of a conducting layer by the 187 hydrogen plasma. When the sample was cleaned by a solution (see chapter 5, section 2.4) in order to remove the conducting layer, the sheet resistance was determined on the order of 108 0/0 with an activation energy of 0.51 eV and 0.42 eV for hole mobility equals to 1200 and 12 cmz/V-s respectively (see chapter 5, section 2.4). 6.1.6 Electric Field Dependent Conductivity of Diamond Films The dc electrical conductivity of polycrystalline diamond films with submicron grain sizes and ohmic contacts was studied as a function of the applied electric field up to the point of electrical breakdown. For electric fields below approximately 105 V/ cm, the films exhibited predominantly ohmic behavior with a conductivity that was independent of the applied voltage for both high work function metal contacts (Au) and low work function metal contacts (In). For higher electric fields, however, the conductivity was field activated according to Poole’s Law. The data is consistent with a Poole-Frenkel reduction of the ionization energy associated with Coulombic potentials surrounding ionizable centers, where the Coulombic potentials overlap. The ionizable centers may result from impurities or defects. In this study, experimental data showed that it is a carrier concentration increase, not a mobility increase, that gave rise to the field activated conductivity which is consistent with the Poole-Frenkel mechanism. Because of the field activated conductivity, the current at high electric fields is substantially larger than would otherwise be the case. For 3.5 pm and 2 pm thick films, the breakdown happens-at voltages higher than 250 V and 150 V respectively, corresponding to a breakdown field of 7.1 x105 and 7.5x 105 V/ cm respectively. Con- sequently, the dielectric strength of the sub-micron grain size polycrystalline diamond films in this study are substantially less than those reported for single crystal dia- 188 mond (0.6 -1x107 V / cm). The slope of the conductivity versus electric field indicates approximate one ionizable impurity or defect per 10,000 host atoms in such films. 6.1.7 Diamond Schottky Barrier Diode Polycrystalline diamond Schottky barrier diodes were fabricated by using the large grain size diamond films with the A1 / diamond/ p—silicon structure. Rectifying behav- ior was determined in the Al/diamond interface as opposed to the diamond/silicon interface. The I p/ I 3 ratio is almost 2x105 at 10 V in the best device, but only 2x102 at 25 V. The I-V characteristic can be modeled as an ideal Schottky diode in series with an insulator, for which the property (I ocV’" relationship), is indicative of a space charge limited current effect in the bulk diamond. However, the metal/diamond/p. silicon samples for the small grain size diamond films exhibited ohmic property since the defect states in these films are so large that carriers can easily tunnel through the barrier. 6.2 Future Research This research has studied the synthesis of diamond films in the MPDR deposition system; physical characterizations, and electrical characterization of the diamond films and diamond/ silicon samples. However, the understanding of the relationship between the physical characterization and electrical properties is still in the early stage. More detailed investigation into the topics covered in this dissertation as well as the effects of other parameters (such as the vacuum purity, the addition of oxygen, and other gases, and lower plasma pressure) are still needed to complete our understanding of this research. Recommendations for future research follow. 189 6.2.1 Improvement for Diamond Deposition The deposition system described in this research can be considerably improved with regard to system purity and with regard to deposition over larger area substrate. With regard to the latter, considerable progress has been made by a colleague, J. Zhang [139]. With regard to system purity, the vacuum system used in this research was mechanically pumped with a ultimate pressure of 1x10" Torr. Residual gas composition and leak/outgas rates were not specially quantified and monitored on a run-to-run basis. In order to better control impurities it would be useful to up- grade the system to a 1><10'7 Torr ultimate pressure and to perform residual gas analysis prior to runs. By providing a lower pressure capability, this also offers the opportunity to investigate ECR plasma deposition of diamond at lower pressures and temperatures. If the ECR plasma technique can be successfully used in an MPDR system, the deposition area could be quite large, 6 inches in diameter or larger. Other things being equal, there is always a trade-off between a large deposition area and a high deposition rate since the. amount of reaction species is fixed for a given reaction mixture, gas flow and microwave power. Consequently, the larger the deposition area, the lower the deposition rate. With the addition of oxygen, however, it is known that the quality and deposition rate can be improved. The extent to which oxygen affects the quality and deposition rate needs to be carefully studied on different configurations of this system. 6.2.2 The Techniques for Physical Characterization It is known that Raman spectroscopy is the best technique to distinguish diamond, graphite, and amorphous carbon. However, Raman spectroscopy only provides lim- ited information about the sample, specifically it determines if the film is similar to natural diamond having a sharp peak at 1332 cm“. For example, Raman spec- 190 troscopy can’t show the difference between a sample with and without a very thin layer of conducting graphite or chemical contamination on top of the films. Also as shown in Figure 4.7, Raman spectroscopy can’t show the difference between a large grain size diamond film and a small grain size diamond film deposited at the same conditions. Other characterization techniques are therefore also needed in future work to provide the basic properties of the film to assist the Raman spectroscopy in order to have a better understanding of the over-all physical properties of the film. Examples include secondary ion mass spectroscopy (SIMS) and Auger electron spectroscopy (ABS) to determine the elemental composition of the film; X-ray diffraction (XRD) to determine the crystal structure and lattice spacing; electron energy loss spectroscopy (EELS) to determine the localized bonding in the bulk film; X-ray photoelectron spectroscopy (XPS) to examine the chemical composition at the surface of the film; and scanning electron microscopy (SEM) to examine the surface morphology. 6.2.3 The Role of SiC at the Diamond/ Silicon Interface It is known that a thin layer of SiC exists at the diamond/silicon interface from this and other research. It may be hypothesized that SiC contributed to the ohmic behavior of the diamond/p-silicon interface for both small and large grain size dia- mond films in this research. However, it is not clear at this point how SiC affects the electrical properties of the diamond / silicon hetero junction. It would be of interest in future research to carefully prepare back-etched samples with and without the SiC layer in order to study this further. It would also be interesting to investigate how the interfacial electrical properties vary if the nucleation methods is changed from abrasion to seeding since the abrasion nucleation method scratches the silicon surface and the seeding nucleation methods does not. 191 6.2.4 Defects States in Diamond Films There are clearly defect states in polycrystalline diamond films because of the exis- tence of grain boundaries. However, defect states in each single crystal is also possible since the methane and hydrogen gases used in this research are 99.99 % and 99.999 % pure respectively. In this research, it was shown that defect states play an important role contributing to the electrical properties. For small grain size metal/ diamond / p- silicon samples, the number of defect states is so large that it contributes to the ohmic contact behavior. Large grain size Al/diamond/p-silicon samples, however, did show some rectifying properties since there are less defect states. Further knowledge of the defect states in the diamond films under different plasma pressure and. different deposition system becomes an important future task for understanding the electrical properties of synthetic diamond films. 6.2.5 Diamond Devices A major future goal of diamond synthesis research is to fabricate useful dia— mond devices, such as diamond diodes, diamond transistors, diamond metal-oxide- semiconductor structures, and diamond integrated circuits (IC) with performance advantages based on the excellent properties of diamond (see chapter 2, section 4). There is a need for considerable future work toward the development of electronic grade diamond. A difficult, but important, future task for diamond device research is the devel- opment of the capability to synthesize epitaxial diamond films on non-diamond sub- strates. The existing techniques only can deposit epitaxial diamond films on diamond substrates and polycrystalline diamond films on non-diamond substrate. Further- more, it is important to evaluate and improve the performance of the poly-diamond devices. Future device related tasks also include the development of improved tech- 192 niques for diamond doping and etching. The investigation of the electrical properties of synthetic diamond is still in the preliminary stage and the fabrication of diamond devices is still far from mature. Consequently, much more future research effort is needed in order to explore the potential development of diamond devices. APPENDICES APPENDIX A Deposited Diamond Films ( 1 ) Samples by Diamond-Paste Nucleation Method Sample CH4/ H2 MiCrowave Plasma Number Fl (39% ate PIQEVUGtI’ Pressure Time Date (NDF-#) (sccm) (W) (Torr) (hour) N6 "5 % 600 60 7 6/17/‘89 (3 : 200 ) P6 ( £1523, ) 600 60 7 6/18/‘89 0 N7 (2132230 ) 600 50 7 6/19/‘89 0 P7 (2132:5230 ) 600 50 7 6/20/‘69 0.5 % ‘ P8, N8 (125 : 250 ) 700 80 6 8/31/' 89 0.5 % P9, N9 (125 , 250) 700 30 6 9/2l’89 P10, N10 (1 3557550 ) 700 80 6 9/3l'89 0.5 % P11. N11 (125 : 250 ) 825 80 6 9/4l'89 193 . _ L I 194 Sample CH4/ H2 Microwave PI and In Ut asma ° In??? Flow Rate poem; Pressure Time Date ( ' ) (sccm) (W) (Torr) (hour) 0.5% P12: N12 (1.25:250) 700 70 6 9/5f89 P13 N13 05% 700 70 6 9/6l’89 ' (1.25:250) 0.5 % P14, N14 (125150) 700 60 8 9/7/’89 P15 N15 05% 800 60 8 SIB/’89 ' (1.25:250) 0.5% P16, N16 (125150) 600 60 a 9/9l’89 0.57 61 (1.25: 2°50) 600 60 6 9/10/‘89 0.5% 82 (125150) 600 - 60 6 9/11/‘89 0.5% P17, N17 (125150) 700 60 1o 9/12/‘89 2% P18,N18 (2,100) 700 60 5 10/18/‘89 2% P19,N19 (2:100) 700 50 5 10/19/‘89 1°/ P20, N20 (1.5350) 700 60 3 11/5/89 10/ . P21,N21 (1.5350) 700 70 8 11/6/‘89 1% P22, N22 800 60 10 11/7/‘89 (1.5:150) 195 Microwave 33mg: :Eéégie (43553, Ifr'easfs'iife Time Date (NDF-#) (sccm) (W) (Torr) (hour) P23, N23 (1.51150) 800 50 10 11/8/‘89 P24, N24 (1.51330) 700 70 10 11/9/39 P25, P26 (1.51:?50') 700 70 14 11/10/39 P27, N27 (1.51150) 700 70 10 1/11/90 P28, N28 (2255:0150) 700 70 6 1/22/90 P29, N29 (2313505) 700 70 5 1/23/90 P30, N30 (1.;51:?50) 700 70 6 1/24/'90 P31,N31 (1.; 7:50) 700 70 5 2/6/‘90 P32, N32 (113'? ,‘Vgo, 700 70 6 2/3r90 N25, N26 (1.857;?50) 700 70 6 2/13I'90 196 ( 2 ) Samples by Diamond-Powder Nucleation Method Sample CH 4/ H2 Microwave Plasma Numb” Floiimiiato P311711 Pressure “me Date (NDF'#) (scorn) (W) (Torr) I(hour) 0.5 % P33 (0.75: 150) 600 30 6 379790 0.5 % P34 (035, 150) 600 70 6 3/13790 P35 1 % 600 70 5 3/151'90 ( 1.5: 150) 1.5 % P36 (225,150) 600 70 5 3/16l'90 1 % P37 (1.5: 150) 600 60 5 3/19/‘90 0.5 % P38 (075: ,50) 600 60 6 3122790 . 0.5 % . . P39 (0.75: 150) 600 50 6 3123/90 P40 ’ % 600 50 5 3/27/‘90 ( 1.5 : 150) P41 1 % 750 50 5 3/29/‘90 ( 1.5 : 150) ‘ 0.5 % P42 (0.75: 150) 500 60 6 4/6/‘90 0.5 % P43 (075, 150) 500 50 6 4/9/‘90 0.5 % 33 (075,150) 500 50 6 4/11/‘90 0.5 °/ 34 (0.75, :50) 400 50 6 4/12/‘90 197 Microwave Sample CH4/ H2 Plasma In ut Number Floaviffaate peas, Pressure “"19. Date (NDF-#) (scorn) (W) (Torr) (hour) 0.5 % 55 (0.75 : 150); 600 50 6 4/13/90 P44 0.5 % ((175,150) 500 60 10 4/14790 P45 05% 400 60 10 4715790 (0.75 : 150) P46 0'5 % 600 60 10 4/16/‘90 (0.75 : 150) P47 0'5 % 600 50 10 4/17790 (0.75 : 150) 0.5 % P48 ( 0.75 ; 150) 700 60 10 4/18/‘90 $6 0'5 % 320 6 4/19/‘90 ' (0.75 : 150) 5° P49 0'5 % 400 50 6 4120790 (0.75 : 150) 0.5 % P50 (075 : ,50) 800 60 6 4/23790 P 1% 400 51 (15,150) 60 5 4124/90 P52 1% . (1.5 : 150) 500 60 5 4/257'90 P 1% 53 (15,150) 700 60 5 4/27r90 0 s7 1 P 50 5 4/29/90 (1.5:150) 400 APPENDIX B Electrical Samples ( 1 ) Metal/Diamond/Silicon Samples Film # Metal Contact P6 Al N6 Al P7 Al N7 Al P8 Al N8 Al P9 Al N9 Al 198 199 Film # Metal Contact P1 0 Al N1 0 Al P20 Al N20 Al P21 Al N21 Al P39 Au P39 Ag P39 In P49 Au P49 Ag P49 In (2) Metal/Diamond/Metal Back-Etched Samples 200 Film # Top Bottom Metal Contact Metal Contact N14-T1 - - - Cr/Au N14-T2 - - - Au P33-T1 Ag A9 P33-T2 Ag Pt/Ag P33-T3 In Pt/Ag P44-T1 Au ' Ag P44-T2 In In P44-T3 In Pt/Ag P46-Tl Au Ag P46-T2 Au Ag P46-T3 In In P46-T4 Au In 201 an # Top Bottom Metal Contact Metal Contact P45-T1 - - - Ag P45-T1 - - - A9 P45-T1 - - - Ag P47-T1 Au AU P47-T2 Au Au P47-T3 In Au P48-T1 - - - Au P48-T2 - - - Au P48-T3 - - - Au P49-T1 Ag Ag P49-T2 Ag Ag P49-T3 Au Ag BIBLIOGRAPHY BIBLIOGRAPHY [1] F. P. Bundy, H. T. Hall, H. M. Strong, R. H. Wentorf Jr., Nature, 176, pp.51, 1955. [2] J. Asmusson and J. 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