Radiation Transport Around Kerr Black Holes Jeremy David ...

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154 CHAPTER 5. STEADY-STATE α-DISKS Figure 5-5: Sample of normalized photon energy spectra produced by steadystate α-disks for a variety of black hole masses, spins, and inclinations. For each case, a range of Eddington-scaled luminosities are shown. The peak energy E max scales as in equation (5.91) while the ratio E cut /E max is sensitive to the spin and inclination angle.
5.4. OBSERVED SPECTRUM OF THE DISK 155 rotational instability as the driving force behind angular momentum transport in the disk, especially the inner regions where the majority of energy is released. Furthermore, to completely match the X-ray spectra from black holes in the Thermal-Dominant state, one must also include a small high-energy power-law component (McClintock & Remillard, 2004). It is likely that this high-energy tail is caused by the Compton upscattering of thermal photons through a hot, low-density electron corona above the disk. In the next Chapter, we introduce a Monte-Carlo code to calculate the effect of this scattering on the continuum photon spectra.
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Radiation Transport Around Kerr Bla
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5 Acknowledgments Gravity can not b
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Contents 1 Introduction and Outline
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CONTENTS 9 A Formulae for Hamiltoni
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List of Figures 1-1 Sample of obser
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List of Tables 3.1 Black hole param
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Chapter 1 Introduction and Outline
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1.2. HISTORICAL BACKGROUND 17 to th
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1.2. HISTORICAL BACKGROUND 19 disk
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1.2. HISTORICAL BACKGROUND 21 tral
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¼ÐÀÓÐÒÖ× 1.3. OUTLINE OF ME
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1.3. OUTLINE OF METHODS AND RESULTS
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1.4. ALTERNATIVE QPO MODELS 31 isot
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1.4. ALTERNATIVE QPO MODELS 33 jets
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Chapter 2 Ray-Tracing in the Kerr M
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2.1. EQUATIONS OF MOTION 37 Killing
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2.1. EQUATIONS OF MOTION 39 flat sp
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2.1. EQUATIONS OF MOTION 41 conveni
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2.1. EQUATIONS OF MOTION 43 in sepa
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2.2. GEODESIC RAY-TRACING 45 basis
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2.2. GEODESIC RAY-TRACING 47 throug
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2.2. GEODESIC RAY-TRACING 49 with a
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2.2. GEODESIC RAY-TRACING 51 since
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2.2. GEODESIC RAY-TRACING 53 dx µ
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2.2. GEODESIC RAY-TRACING 55 In the
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2.3. NUMERICAL METHODS 57 a long pa
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2.4. BROADENED EMISSION LINES FROM
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Chapter 3 The Geodesic Hot Spot Mod
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3.1. HOT SPOT EMISSION 71 Figure 3-
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3.2. NON-CIRCULAR ORBITS 77 Figure
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3.2. NON-CIRCULAR ORBITS 79 Figure
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3.2. NON-CIRCULAR ORBITS 81 paramet
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3.2. NON-CIRCULAR ORBITS 83 at (2/3
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3.2. NON-CIRCULAR ORBITS 85 form at
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3.3. NON-PLANAR ORBITS 87 3.3 Non-p
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3.3. NON-PLANAR ORBITS 89 Table 3.1
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3.4. SUMMARY 91 binaries in many wa
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Chapter 4 Features of the QPO Spect
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4.2. PARAMETERS FOR THE BASIC HOT S
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4.3. PEAK BROADENING FROM HOT SPOTS
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4.3. PEAK BROADENING FROM HOT SPOTS
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4.4. DISTRIBUTION OF COORDINATE FRE
Page 103 and 104: 4.4. DISTRIBUTION OF COORDINATE FRE
Page 105 and 106: 4.4. DISTRIBUTION OF COORDINATE FRE
Page 107 and 108: 4.5. ELECTRON SCATTERING IN THE COR
Page 113 and 114: 4.6. FITTING QPO DATA FROM XTE J155
Page 115 and 116: 4.6. FITTING QPO DATA FROM XTE J155
Page 117 and 118: 4.7. HIGHER ORDER STATISTICS 117 ob
Page 119 and 120: 4.7. HIGHER ORDER STATISTICS 119 bi
Page 121 and 122: 4.7. HIGHER ORDER STATISTICS 121 Fi
Page 123 and 124: 4.7. HIGHER ORDER STATISTICS 123 12
Page 125 and 126: 4.8. SUMMARY 125 els. Clearly the h
Page 127 and 128: Chapter 5 Steady-state α-disks The
Page 129 and 130: 5.1. STEADY-STATE DISKS OUTSIDE THE
Page 139 and 140: 5.2. GEODESIC PLUNGE INSIDE THE ISC
Page 141 and 142: 5.2. GEODESIC PLUNGE INSIDE THE ISC
Page 143 and 144: 5.3. NUMERICAL IMPLEMENTATION 143 F
Page 145 and 146: 5.3. NUMERICAL IMPLEMENTATION 145 a
Page 147 and 148: 5.3. NUMERICAL IMPLEMENTATION 147 (
Page 149 and 150: 5.4. OBSERVED SPECTRUM OF THE DISK
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Page 157 and 158: Chapter 6 Electron Scattering If we
Page 159 and 160: 6.1. PHYSICS OF SCATTERING 159 Θ
Page 161 and 162: 6.1. PHYSICS OF SCATTERING 161 the
Page 163 and 164: 6.1. PHYSICS OF SCATTERING 163 and
Page 165 and 166: 6.1. PHYSICS OF SCATTERING 165 colo
Page 167 and 168: 6.2. EFFECT ON SPECTRA 167 Let g(z)
Page 169 and 170: 6.2. EFFECT ON SPECTRA 169 (1979);
Page 171 and 172: 6.2. EFFECT ON SPECTRA 171 Figure 6
Page 173 and 174: 6.3. EFFECT ON LIGHT CURVES 173 Fig
Page 179 and 180: 6.4. IMPLICATIONS FOR QPO MODELS 17
Page 181 and 182: Chapter 7 Conclusions and Future Wo
Page 183 and 184: 7.1. SUMMARY OF RESULTS 183 the low
Page 185 and 186: 7.2. CAVEATS 185 back to the coordi
Page 187 and 188: 7.3. NEW APPLICATIONS OF CURRENT CO
Page 189 and 190: 7.4. NEW FEATURES FOR CODE 189 grou
Page 191 and 192: 7.5. DEVELOPMENT OF NEW MODELS 191
Page 193 and 194: Appendix A Formulae for Hamiltonian
Page 195 and 196: 195 The relevant spatial derivative
Page 197 and 198: Appendix B Summing Periodic Functio
Page 199 and 200: 199 Over a sample time T f ≫ T l
Page 201 and 202: Bibliography Abramowicz, M. A., Lan
Page 203 and 204: BIBLIOGRAPHY 203 Damour, T., & Espo
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BIBLIOGRAPHY 205 Hawler, J. F., & G
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BIBLIOGRAPHY 207 McClintock, J. E.,
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BIBLIOGRAPHY 209 Psaltis, D. 2001b,
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BIBLIOGRAPHY 211 Stern, B., et al.
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