
High Energy Radiation from Black Holes
Gamma Rays, Cosmic Rays, and Neutrinos
By: Charles D. Dermer, Govind Menon
Paperback | 4 January 2010
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Bright gamma-ray flares observed from sources far beyond our Milky Way Galaxy are best explained if enormous amounts of energy are liberated by black holes. The highest- energy particles in nature--the ultra-high-energy cosmic rays--cannot be confined by the Milky Way's magnetic field, and must originate from sources outside our Galaxy. Understanding these energetic radiations requires an extensive theoretical framework involving the radiation physics and strong-field gravity of black holes. In High Energy Radiation from Black Holes, Charles Dermer and Govind Menon present a systematic exposition of black-hole astrophysics and general relativity in order to understand how gamma rays, cosmic rays, and neutrinos are produced by black holes.
Beginning with Einstein's special and general theories of relativity, the authors give a detailed mathematical description of fundamental astrophysical radiation processes, including Compton scattering of electrons and photons, synchrotron radiation of particles in magnetic fields, photohadronic interactions of cosmic rays with photons, gamma-ray attenuation, Fermi acceleration, and the Blandford-Znajek mechanism for energy extraction from rotating black holes. The book provides a basis for graduate students and researchers in the field to interpret the latest results from high-energy observatories, and helps resolve whether energy released by rotating black holes powers the highest-energy radiations in nature. The wide range of detail will make High Energy Radiation from Black Holes a standard reference for black-hole research.
Industry Reviews
"There is definite need for a book on this topic. Dermer and Menon have gathered together a wide range of useful results and the book's rigorous and comprehensive coverage of high-energy processes will be valuable to the advanced researcher in the field. Astronomers working on black-hole processes, jets, AGN, and gamma-ray bursts will want to have this for reference."-Andrew Fabian, University of Cambridge
Preface | p. xix |
Introduction | p. 1 |
Black Holes in Nature | p. 1 |
Energy Fluxes | p. 8 |
Timing Studies and Black-Hole Mass Estimates | p. 10 |
Flux Distribution | p. 11 |
The Nighttime Sky | p. 12 |
Relativistic Kinematics | p. 14 |
Lorentz Transformation Equations | p. 14 |
Four-Vectors and Momentum | p. 16 |
Relativistic Doppler Factor | p. 18 |
Three Useful Invariants | p. 19 |
Relativistic Reaction Rate | p. 21 |
Secondary Production Spectra | p. 23 |
Introduction to Curved Spacetime | p. 25 |
Special Relativity | p. 25 |
Curved Space/Spacetime | p. 29 |
The Schwarzschild Metric | p. 33 |
Physical Cosmology | p. 36 |
Robertson-Walker Metric | p. 36 |
Friedmann Models | p. 39 |
Hubble Relation from the Cosmological Principle | p. 39 |
Expansion of the Universe | p. 40 |
Einstein-de Sitter Universe | p. 43 |
Universe with Zero Cosmological Constant | p. 43 |
Flat Universe | p. 43 |
Luminosity and Angular-Diameter Distances | p. 44 |
Event Rate of Bursting Sources | p. 45 |
Flux and Intensity from Distributed Sources | p. 47 |
Radiation Physics of Relativistic Flows | p. 50 |
Radiation Preliminaries | p. 50 |
Invariant Quantities | p. 53 |
Blackbody Radiation Field | p. 53 |
Transformed Quantities | p. 56 |
Transformation of Total Distribution and Energy | p. 56 |
Transformation of Differential Distributions | p. 56 |
Fluxes of Relativistic Cosmological Sources | p. 59 |
Blob Geometry | p. 60 |
Spherical Shell Geometry | p. 63 |
Equivalence of Blob and Blast Wave Geometries | p. 68 |
Compton Scattering | p. 70 |
Compton Effect | p. 70 |
The Compton Cross Section | p. 71 |
Transforming the Compton Cross Section | p. 73 |
Differential Thomson Cross Section | p. 75 |
Head-on Approximation | p. 77 |
Differential Compton Cross Section | p. 77 |
Moments of the Compton Cross Section | p. 79 |
Compton Scattering in the -Function Approximation | p. 80 |
Energy-Loss Rates in Compton Scattering | p. 81 |
Thomson Energy-Loss Rate | p. 81 |
Klein-Nishina Energy-Loss Rate | p. 82 |
Differential Compton Cross Sections and Spectra | p. 83 |
Comparison of Scattered Spectra for Different ERF Photon Energies | p. 83 |
Spectral Comparisons for Isotropic Monochromatic Photons and Power-Law Electrons | p. 84 |
Thomson Scattering: Isotropic Photons and Electrons | p. 92 |
Thomson-Scattered Radiation Spectrum in the -Function Approximation | p. 92 |
Spectral Comparisons for Isotropic Power-Law Photons and Electrons | p. 93 |
External Photon Fields Compton-Scattered by Jet Electrons | p. 94 |
Thomson-Scattered Spectrum for an External Point Source of Radiation from Behind | p. 96 |
Thomson-Scattered Spectrum for External Isotropic Radiation in the ?-Function Approximation | p. 97 |
External Isotropic Photons Compton-Scattered by let Electrons | p. 99 |
Cosmic Microwave Background Radiation Compton-Scattered by Jet Electrons | p. 103 |
Accretion-Disk Field Compton-Scattered by Jet Electrons | p. 105 |
Optically Thick Shakura-Sunyaev Disk Spectrum | p. 106 |
Integrated Emission Spectrum from Shakura-Sunyaev Disk | p. 107 |
Transformed Accretion-Disk Radiation Field | p. 108 |
Thomson-Scattered Shakura-Sunyaev Disk Spectrum in the Near Field | p. 112 |
Thomson-Scattered Shakura-Sunyaev Disk Spectrum in the Far Field | p. 113 |
Beaming Patterns | p. 113 |
Broad-Line Region Scattered Radiation | p. 114 |
Synchrotron Radiation | p. 117 |
Covariant Electrodynamics | p. 118 |
Synchrotron Power and Peak Frequency | p. 119 |
Elementary Synchrotron Radiation Formulae | p. 121 |
Relations between Emitted, Received, and 90° Pitch-Angle Powers | p. 123 |
Particle Synchrotron Radiation | p. 126 |
Synchrotron Spectrum from a Power-Law Electron Distribution | p. 127 |
-Function Approximation for Synchrotron Radiation | p. 129 |
Equipartition Magnetic Field | p. 131 |
Equipartition Magnetic Field: Qualitative Estimate | p. 132 |
Equipartition Magnetic Field: Quantitative Treatment | p. 133 |
Energelics and Minimum Jet Powers | p. 135 |
Synchrotron Self-Compton Radiation | p. 138 |
SSC in the Thomson Regime | p. 138 |
SSC in the Thomson Regime for Broken Power-Law Electron Distribution | p. 140 |
Accurate SSC for General Electron Distribution | p. 141 |
Synchrotion/SSC Model | p. 142 |
SSC Electron Energy-Loss Rate | p. 143 |
Synchrotron Self-Absorption | p. 143 |
Einstein Coefficients | p. 145 |
Brightness Temperature and Self-Absorbed Flux: Qualitative Discussion | p. 146 |
Derivation of the Synchrotron Self-Absorption Coefficient | p. 148 |
-Function Approximation for Synchrotron Self-Absorption | p. 148 |
Synchrotron Self-Absorption Coefficient for Power-Law Electrons | p. 149 |
Maximum Brightness Temperature | p. 150 |
Compton Limits on the Doppler Factor | p. 153 |
Self-Absorbed Synchrotron Spectrum | p. 154 |
Hyper-Relativistic Electrons | p. 156 |
Jitter Radiation | p. 158 |
Binary Particle Collision Processes | p. 160 |
Coulomb Energy Losses | p. 161 |
Stopping Power of Cold Plasma | p. 161 |
Thermal Relaxation | p. 163 |
Stopping Power of Thermal Plasma | p. 164 |
Knock-On Electrons | p. 165 |
Bremsstrahlung | p. 166 |
Electron Bremsstrahlung Energy-Loss Rate | p. 167 |
Electron Bremsstrahlung Production Spectra | p. 167 |
Secondary Nuclear Production | p. 169 |
Rays from 0 Decay | p. 171 |
Cross Section for p + p &leftarrrow; + X Production | p. 172 |
Electron-Positron Annihilation Radiation | p. 180 |
Annihilation in a Thermal Medium | p. 181 |
Thermal Annihilation Line and Continuum Spectra | p. 182 |
Nuclear -Ray Line Production | p. 185 |
Photohadronic Processes | p. 187 |
Scattering and Energy-Loss Timescales | p. 189 |
Photopion Process | p. 190 |
Photopion Cross Section | p. 191 |
Analytic Expression for Photopion Cross Section | p. 192 |
Numerical Calculation of Photopion Cross Section | p. 194 |
Photopion Energy-Loss Rate | p. 194 |
GZK Energy | p. 196 |
Stochastic and Continuous Energy Losses | p. 197 |
Photopair Process | p. 197 |
Photopair Cross Section | p. 198 |
Photopair Energy-Loss Timescale | p. 198 |
Accurate Expression for Photopair Energy-Loss Rates of Ions in an Isotropic Radiation Field | p. 201 |
Relative Importance of Photopion and Photopair Losses | p. 203 |
Expansion Losses | p. 203 |
Cosmogenic Neutrino Flux | p. 204 |
Ultrahigh-Enetgy Cosmic-Ray Evolution | p. 208 |
Normalization to Local Luminosity Density | p. 209 |
Energy Evolution of Cosmic-Ray Protons | p. 210 |
Rate Density Evolution and the Star Formation Rate | p. 211 |
Waxman-Bahcail Bound | p. 213 |
UHECR and GZK Neutrino Intensities | p. 215 |
Photonuclear Reactions | p. 219 |
Photodisintegration Reaction Rate | p. 222 |
Effective Photodisintegration Energy-Loss Rate | p. 224 |
Neutrinos from Photodisintegration | p. 225 |
Pair Production | p. 227 |
Pair Production Cross Section | p. 228 |
Absorption by a Blackbody and a Modified Blackbody Photon Gas | p. 231 |
Absorption by a Power-Law Photon Gas in a Relativistic Jet | p. 233 |
Attenuation in Anisotropic Radiation Fields | p. 235 |
?-Function Approximation for | p. 236 |
Opacity of the Universe to Attenuation | p. 237 |
Optical Depth of the Universe | p. 238 |
Measurements of the EBL | p. 240 |
Attenuation at Low Redshifts | p. 241 |
Attenuation at All Redshifts | p. 244 |
The -Ray Horizon | p. 244 |
Compactness Parameter | p. 245 |
Minimum Doppler Factor from Constraint | p. 247 |
Correlated -Ray and Neutrino Fluxes | p. 249 |
Electromagnetic Cascades | p. 253 |
Cascades in Jets | p. 254 |
Cascades in the Intergalactic Medium | p. 256 |
&leftarrrow; | p. 257 |
Blast-Wave Physics | p. 258 |
Fireballs and Relativistic Blast Waves | p. 258 |
Blast-Wave Deceleration | p. 260 |
Blast-Wave Equation of Motion | p. 261 |
Dissipated Internal Energy | p. 270 |
Elementary Blast-Wave Theory | p. 270 |
Characteristic Electron Energies | p. 271 |
Characteristic Synchrotron Frequencies | p. 274 |
Afterglow Theory | p. 278 |
Relativistic Shock Hydrodynamics | p. 282 |
Relativistic Shock Thermodynamics | p. 282 |
Synchrotron Radiation from a Relativistic Reverse Shock | p. 288 |
Beaming Breaks and Jets | p. 290 |
Synchrotron Self-Compton Radiation | p. 292 |
Theory of the Prompt Phase | p. 294 |
X-Ray Flares and -Ray Pulses from External Shocks | p. 295 |
Colliding Shells and Internal Shocks | p. 301 |
Thermal Photospheres | p. 303 |
The Amati and Ghirlanda Relations | p. 303 |
Thermodynamics of a Steady Relativistic Wind | p. 304 |
Photospheric Radius | p. 306 |
Pair Photosphere | p. 308 |
Thermal Neutrons | p. 310 |
GRB Cosmology | p. 312 |
Introduction to Fermi Acceleration | p. 314 |
Stochastic and Shock Fermi Acceleration | p. 316 |
Wave Turbulence Spectrum | p. 317 |
The Hillas Condition | p. 320 |
Energy Gain per Cycle from Fermi Acceleration | p. 321 |
Diffusion in Physical Space | p. 322 |
Maximum Particle Energy | p. 324 |
First-Order Fermi Acceleration | p. 327 |
Nonrelativistic Shock Hydrodynamics | p. 328 |
Convection-Diffusion Equation | p. 330 |
Nonrelativistic Shock Acceleration | p. 332 |
Spectral Index from Convection-Diffusion Equation | p. 332 |
Spectral Index from Probability Arguments | p. 334 |
Finite Shell Width | p. 335 |
Cosmic-Ray Pressure and Shock Width | p. 337 |
Maximum Particle Energy in Nonrelativistic Shock Acceleration | p. 339 |
Maximum Particle Energy in Nonrelativistic Shocks | p. 343 |
Amplification of Upstream Medium Magnetic Field | p. 344 |
Relativistic Shock Acceleration | p. 346 |
Fokker-Planck Equation for a Stationary, Parallel Shock | p. 347 |
Spectral Index in Relativistic Shock Acceleration | p. 348 |
Maximum Particle Energies in Relativistic Shock Acceleration | p. 349 |
Second-Order Fermi Acceleration | p. 351 |
Power-Law Particle Spectra from Second-Order Fermi Acceleration | p. 353 |
The Resonance Condition | p. 353 |
Plasma Waves | p. 355 |
Diffusive Particle Acceleration | p. 359 |
Approximate Derivation of Diffusion Coefficients | p. 362 |
Pitch-Angle Diffusion Coefficient | p. 362 |
Momentum Diffusion Coefficient | p. 363 |
Energy Gain and Diffusive Escape Rates | p. 364 |
Momentum Diffusion Equation | p. 367 |
Ramaty-Lee Spectrum for Hard-Sphere Scattering | p. 368 |
Green's Function Solution | p. 370 |
Maximum Particle Energy in Second-Order Fermi Acceleration | p. 372 |
Gyroresonant Stochastic Acceleration | p. 373 |
Stochastic Energization in Nonrelativistic Shocks | p. 374 |
Stochastic Energization in Relativistic Flows | p. 376 |
The Geometry of Spacetime | p. 379 |
Introduction | p. 379 |
Splitting Spacetime into Space and Time | p. 380 |
The Kerr Metric | p. 384 |
The Geodesic Equation and Its Integrability in Kerr Geometry | p. 386 |
The Kerr Metric in Kerr-Schild Coordinates | p. 391 |
The Ergosphere | p. 394 |
The Event Horizon | p. 396 |
The Penrose Process | p. 397 |
Hawking Radiation | p. 402 |
Scalar Fields in Curved Spacetime | p. 402 |
The Quantum Field for a Scalar Particle in a Flat Spacetime | p. 404 |
Particle Creation in Curved Spacetime | p. 405 |
Particle Creation in Rindler Spacetime | p. 408 |
Particle Creation in Schwarzschild Geometry | p. 415 |
Black-Hole Electrodynamics | p. 417 |
3+1 Electrodynamics | p. 417 |
The Energy-Momentum Tensor | p. 424 |
The Blandford-Znajek Process | p. 427 |
Explicit Expressions for the Fields and Currents | p. 431 |
The Force-Free Constraint Equation | p. 432 |
The Znajek Regularity Condition | p. 433 |
Energy and Angular-Mom en turn Extraction from the Force-Free Magnetosphere | p. 435 |
Geodesic Currents in the Magnetosphere | p. 436 |
An Exact Solution | p. 439 |
Fields and Energy Extraction for the - Solution | p. 441 |
An Approximate Solution | p. 442 |
Uniqueness of the _ Solution | p. 447 |
Energy Extraction for the + Solution | p. 448 |
Blandford-Znajek Process in Astrophysical Sources | p. 450 |
High-Energy Radiations from Black Holes | p. 452 |
Rays | p. 453 |
Modeling Rays from Black Holes | p. 454 |
Statistics of Black-Hole Sources | p. 456 |
Blazar Physics | p. 457 |
GRB Classes | p. 458 |
Unresolved and Diffuse ?-Ray Background | p. 458 |
Cosmic Rays | p. 459 |
Acceleration of Cosmic Rays at Supernova Remnant Shocks | p. 461 |
Acceleration of UHECRs at Relativistic Blast Waves | p. 462 |
Charged-Particle Astronomy | p. 463 |
UHECR Propagation | p. 466 |
UHECR Source Power Requirements | p. 466 |
Neutrinos | p. 468 |
Concluding Remarks | p. 471 |
Essential Tensor Calculus | p. 473 |
Introduction | p. 473 |
The Tangent Vector | p. 473 |
Dual Vectors | p. 476 |
The Space T**(M) | p. 477 |
Tensors | p. 478 |
The Metric Tensor | p. 480 |
The Volume Element and the Levi-Civita Tensor | p. 481 |
The Covariant Derivative | p. 483 |
The Divergence Theorem | p. 485 |
The Einstein Equation | p. 486 |
Mathematical Functions | p. 488 |
The Gamma Function and Error Function | p. 488 |
Modified Bessel Functions of the Second Kind | p. 488 |
Exponential Integral Function | p. 489 |
Planck's Function | p. 490 |
Bernoulli Numbers and Riemann ? Function | p. 490 |
Whittaker Functions | p. 491 |
Lambert W Function | p. 491 |
Solutions of the Continuity Equation | p. 492 |
Basics of Monte Carlo Calculations | p. 497 |
Supplementary Information | p. 499 |
Glossary and Acronym List | p. 505 |
Bibliography | p. 509 |
Index | p. 531 |
Table of Contents provided by Ingram. All Rights Reserved. |
ISBN: 9780691144085
ISBN-10: 0691144087
Series: Princeton Series in Astrophysics
Published: 4th January 2010
Format: Paperback
Language: English
Number of Pages: 568
Audience: Professional and Scholarly
Publisher: Princeton University Press
Country of Publication: US
Dimensions (cm): 23.4 x 15.2 x 3.81
Weight (kg): 0.79
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