William Angerer - Department of Physics and Astronomy - University ...

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67 PM[ reflector on s I=Blk er 1-- KDP M F 88 reflector on transl a 1i on stage Figure 3.9: Schematic of the autocorrelator. BS is a beam 50/50 splitter. ~I is a mirror, KDP is the phased matched nonlinear crystal, I is an iris, and F is a short pass filter which filters out any residual fundamental light. 3.4 Autocorrelation Cnlike a dye pumped Nd:YAG laser, the pulse length of the Ti:AI 2 0 3 laser changes as a function of wavelength and the laser cavity alignment. In order to fully characterize the Ti:AI 2 0 3 pulse and optimize laser operation, we built an autocorrelator to measure the sub-picosecond laser pulse. Fig. 3.9 displays the optical setup of the autocorrelator. The autocorrelator is es- Reproduced with permission of the copyright owner. Further reproduction prohibited without permission.
68 sentiallya nonlinear optical interferometer, which functions as follows. The Ti:AI 2 0 3 pulse enters the autocorrelator and is split by a 50/50 beam splitter. The beams are reflected from pairs of mirrors mounted on a speaker and a translation stage. The beams are separated by '" 1 em when they reach a lens with a 100 mm focal length. which focuses the beams to a point inside a nonlinear crystal. vVe used a 0.-1 mm thick KDP crystal cut for type I phase matching, i.e. both of the non-collinear fundamental beams have the same polarization, at 800 nm. The two beams are coupled in the KDP crystal to produce an SHG signal whose magnitude is proportional to the temporal overlap of the fundamental beams. Note, the geometry of this optical setup. non-collinear phase matching, is ideally suited for separating the SHG signal from the overlapped fundamental pulses from the SHG from the individual pulses. In "ultrafast units", the speed of light has a value of 0.3 J.Lm/fs. Therefore, increasing the path length of one of the interference arms by 50 J.Lm drastically changes the temporal overlap of the Ti:AI 2 0 3 pulses in the KDP crystal. vVe can exploit this experimentally to measure the duration of the Ti:AI 2 0 3 pulse by oscillating the speaker mirrors at 60 Hz and detecting and analyzing the SHG signal intensity from the overlap of the ultrafast pulses with a PMT and an oscilloscope. The measurement of the pulse duration is as follows. First, with the time constant of the oscilloscope set to 5 ms, the pulse width is measured. The pulse corresponds to the envelope function of the temporal overlap of the individual pulses. Second. Reproduced with permission of the copyright owner. Further reproduction prohibited without permission.
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SHG SPECTROSCOPY OF GALLIUM NITRIDE
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COPYRIGHT vVilliam E. Angerer 1998
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ACKNOWLEDGEMENTS I am most grateful
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vi and support over the last three
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viii and we report on photoluminesc
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x 2.5 ~ovel Technique and Apparatus
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Xll 7.3 7.2.3 Registering and Posit
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xiv
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xvi 2.10 Device for measuring ultra
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xviii 6.5 Polarization and propagat
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2 scopies as a probe of these featu
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4 tionallinear microscopy is unable
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6 interference by group velocity mi
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Chapter 2 Introduction to Nonlinear
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10 the electric fields as In this t
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12 SHG is a virtual process, Le. th
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14 2.3 (2) Xijk and Symmetry In gen
Page 35 and 36: 16 X (2) zxx = ,\.zyy v(2) (2) = v(
Page 37 and 38: 18 X~}k(W = 2wo) of our GaN samples
Page 39 and 40: 20 nonlinear element of quartz, X~~
Page 41 and 42: 22 the transmitted wave, E:t'°, Th
Page 43 and 44: 24 150 I I "1 I :) ~ >- -. iii c v
Page 45 and 46: 26 Quartz fundamental Figure 2.5: I
Page 47 and 48: 28 The bound wave, which propagates
Page 49 and 50: 30 1/e 2 its ma.'{imum value. This
Page 51 and 52: 32 Here, x~;!Aw = 2wo) is a constan
Page 53 and 54: 34 simplifications (2.39) and (2.40
Page 55 and 56: 36 nonlinear waves. This model assu
Page 57 and 58: 38 Fourier transform to E /2 (r, w)
Page 59 and 60: 40 3 mm and with the parameters dis
Page 61 and 62: 42 I " i iii iii iii iii iii iii ii
Page 63 and 64: 44 parameter value Bl 2.35728 B2 -0
Page 65 and 66: 46 is measured as a function of tra
Page 67 and 68: 48 send pulse into device \11 input
Page 69 and 70: 50 2.6 Conclusion In this brief sec
Page 71 and 72: 52 LOCK-IN AMPLIAER LOCK-IN AMPLIAE
Page 73 and 74: 54 After polarization, the beam was
Page 75 and 76: 56 PO HR !l o IV team BP Figure 3.3
Page 77 and 78: 58 .. ........... • / ~ '" ~ r --
Page 79 and 80: 60 The production of ultrafast, hig
Page 81 and 82: 62 800 ~ 0 0 J 0 0 0 0 J ~ 0 600~ 0
Page 83 and 84: 64 measurements. Typically, I incre
Page 85: 66 described below. Note that laser
Page 89 and 90: 70 780 800 820 840 860 880 900 920
Page 91 and 92: 72 Unlike the linear spectroscopic
Page 93 and 94: 74 fore, the ratio of these two qua
Page 95 and 96: 76 of :UN is deposited on the Ah03
Page 97 and 98: 78 computer HeNe Las polarizer chop
Page 99 and 100: 80 ~------".... GaN A12a3 index flu
Page 101 and 102: 82 + d I , GaN A12a3 Figure 4.3: Co
Page 103 and 104: 84 4.2 Measurement of Indices of Re
Page 105 and 106: 86 fields at the lh interface to th
Page 107 and 108: 88 traveling wave, i.e. (-1.7) wher
Page 109 and 110: 90 Note that the additional subscri
Page 111 and 112: 92 £b, are defined only at the int
Page 113 and 114: 94 Equations (4.30) and (4.32) are
Page 115 and 116: 96 the calculation of the transmitt
Page 117 and 118: 98 '- -0 OJ N 0.4 o E ~ o Z 0.2 o 2
Page 119 and 120: 100 2.0 "'"" "I 1.5 E ::t ~ --c 0 -
Page 121 and 122: 102 4.3 Photoluminescence of GaN To
Page 123 and 124: 104 a photoluminescence measurement
Page 125 and 126: 106 :J 0.01 0 ~ L ~ 0.008 r- :n :v
Page 127 and 128: 108 0.08 ~. j -i ,-... I I ""I :::l
Page 129 and 130: Chapter 5 Properties of GaN In rece
Page 131 and 132: 112 5.1 Crystal Structure :\ crucia
Page 133 and 134: 114 PJO'tI [{fall Figure 5.1: \Vurz
Page 135 and 136: 116 e 4 r .1 It Figure 5.2: Calcula
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118 Parameter Symbol Value electron
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120 high intrinsic electron concent
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122 equation (5.2), is represented
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124 C6v E E £l. 2C3 2C 3 2C6 2C 6
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126 gap, the nonlinear susceptibili
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128 rrb 10.0 eV -------- 5 9.0 eV r
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130 In> 1m> 1m>
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132 Emission of a photon on the bra
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134 5.5 MOCVD Growth of GaN Our GaN
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136 # dopant thickness mobility car
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138 6.1 Nonlinear Optical Spectrosc
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140 y lab X)lSlaJ / 2m Figure 6.1:
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142 Fig. 6.2 displays the azimuthal
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144 includes the effects of pulse p
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146 6.3 Theory of Nonlinear Optical
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148 L x i d 1 E( 00) air GaN sapphi
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150 wavevector components. The free
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152 z y x E( ro) air GaN Figure 6.5
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154 various free waves and summing
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156 factors are: the nonlinearity o
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158 where v /2 is the group velocit
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160 i N -' '- 0 ::J a 0 o.sf fiftH!
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162 4 ""' ::J en Q) - -' .D 2L ·oJ
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164 approximation. The agreement be
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166 midgap state) could playa role
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168 r: b S ~ r b I rs ~ r b I 0)1 r
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170 in various bonding geometries w
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, 172 .----. ::l U'J Q) ttl 0 '-.,;
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Chapter 7 SHG Microscopy The majori
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176 7.1 Historical Context of Secon
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178 comPJter - - - - - - - - - ~ ,-
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180 second-harmonic light towards t
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182 ~ 20 _____ ~ ____ J -----f- ---
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184 wave at normal incidence is (7.
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186 polarization is negligible for
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chopper AGate B Gate Signal Figure
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190 E 4000 1 c: 0 3000 ~ rJl -' 0 c
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192 depend on two components: a hig
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194 nanorope ~ Figure 7.8: Carbon n
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196 of light reflected from the sam
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198 mean square deviation, of the p
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200 7.3 Calculated SHG Signal from
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202 parameter symbol value laser re
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204 parameter symbol value surface
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Chapter 8 Conclusion In this brief
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208 properties of carbon nanotubes.
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210 that propagate through quartz a
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Appendix B Theory of Nonlinear Resp
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214 Fourier transforming equation (
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216 and (CA) with f.b == t(.:.vo) a
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218 The polarization, et, of the po
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220 and (0.1.,1) respectively. Equa
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Appendix E Effect of Sapphire Miscu
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224 with cosO 0 - sin (} o 1 o (E.3
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226 Let us compare the light transm
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228 , .............................
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230 it ( (fp·top..,(arr (ll, M r "
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232 nal-2.00 tab'(:r[ihi]-:r[ila] )
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234 1 - 2500.0; III - xU]; 1/ ti. t
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Bibliography [1] R. K. Chang~ J. Du
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238 [12] J. QL "V. Angerer, M. S. Y
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240 Diamond, SiC and Wide Bandgap S
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242 [40] M. M. Choy and R. L. Byer,
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244 [55] \V. P. Lin, P. M. Lundquis
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246 [70] J. vV. Yang, J. N. Kunzia,
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248 [85] B. Monemar and O. Lagerste
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250 [99] R. C. Miller, Optical Seco
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252 [114] "V. de HeeL W. S. Bacsa,
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William Angerer - Department of Physics and Astronomy - University ...

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