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536 Pages
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Industry Reviews
From the reviews of the first edition:
"This excellent book is the most complete development of cosmic ray astrophysics theory published. It is aimed at current researchers and commencing postgraduate students. ... One of the great benefits of this book is the explicit description of all the assumptions that are made and the limitations they imply on interpretations from the theory. This makes the book particularly valuable for postgraduate students and established researchers starting in the field." (M.L. Duldig, The Physicist, Vol.39 (3), 2002)
Introduction | p. 1 |
The Start of Cosmic Ray Research | p. 1 |
The Scope of Cosmic Ray Research | p. 1 |
Organization of the Book | p. 3 |
Cosmic Rays as Part of the Universe | p. 7 |
Our Present View of the Structure of the Universe | p. 7 |
Interstellar Medium | p. 10 |
Cosmic Photon Fields | p. 17 |
Cosmic Magnetic Fields | p. 19 |
Intergalactic Medium | p. 23 |
Interlude | p. 24 |
Direct Observations of Cosmic Rays | p. 25 |
The Cosmic Ray Landscape | p. 26 |
Solar Modulation | p. 29 |
Solar and Heliospheric Cosmic Rays | p. 36 |
Solar Flare Cosmic Ray Particles | p. 38 |
The Anomalous Cosmic Ray Component | p. 46 |
Extrasolar Cosmic Rays | p. 46 |
Elemental Composition | p. 46 |
Isotopic Composition | p. 57 |
Anisotropy | p. 64 |
Time History from Cosmogenic Nuclei | p. 69 |
Ultrahigh Energy Cosmic Rays | p. 70 |
Interactions of Cosmic Ray Electrons | p. 73 |
Synchrotron Radiation | p. 74 |
Synchrotron Power | p. 74 |
Emission and Transfer of Synchrotron Radiation | p. 76 |
Synchrotron Radiation from Cosmic Ray Electrons in the Interstellar Medium | p. 78 |
Synchrotron Energy Loss of Relativistic Electrons | p. 80 |
Inverse Compton Scattering | p. 80 |
Inverse Compton Power | p. 81 |
Inverse Compton Scattering of Target Photons in the Interstellar Medium by Cosmic Ray Electrons | p. 84 |
Inverse Compton Energy Loss of Relativistic Electrons | p. 88 |
Triplet Pair Production | p. 89 |
Nonthermal Relativistic Electron Bremsstrahlung | p. 93 |
Nonthermal Bremsstrahlung Power | p. 93 |
Nonthermal Bremsstrahlung of Cosmic Ray Electrons in the Interstellar Medium | p. 95 |
Bremsstrahlung Energy Loss of Relativistic Electrons | p. 97 |
Ionization and Coulomb Interactions | p. 98 |
Total Energy Loss Rate | p. 99 |
Continuum Radiation Processes of Relativistic Electrons | p. 102 |
Interactions of Cosmic Ray Nuclei | p. 105 |
Relativistic Kinematics of Inelastic Collisions | p. 105 |
Threshold Energy | p. 106 |
The Energy of One Particle Seen from the Rest System of Another | p. 107 |
Interactions Between Cosmic Ray Nuclei and Cosmic Photons | p. 107 |
Photo-Pair Production | p. 109 |
Photo-Hadron Production | p. 109 |
Photo-Disintegration | p. 112 |
Interactions Between Cosmic Ray Nuclei and Matter | p. 114 |
Gamma-Ray, Electron, Positron and Neutrino Source Functions | p. 115 |
Pion Production Spectra | p. 116 |
0 Decay -Rays | p. 120 |
Secondary Electrons and Positrons | p. 123 |
Secondary Neutrinos | p. 125 |
Energy Loss by Pion Production | p. 128 |
Excitation of Nuclei | p. 128 |
Coulomb and Ionization Interactions | p. 130 |
Catastrophic Losses from Fragmentation and Radioactive Decay | p. 135 |
Total Energy Loss Rate from Interactions with Matter | p. 138 |
Ionization and Heating Rate of Interstellar Matter by Cosmic Rays | p. 139 |
Continuum Radiation Processes of Relativistic Nuclei | p. 140 |
Indirect Observations of Cosmic Rays | p. 143 |
Clues from Radio Astronomy | p. 143 |
Free-Free Emission | p. 143 |
Radio Continuum Surveys | p. 145 |
Clues from -Ray Astronomy | p. 154 |
-Ray Emission Above 10 MeV | p. 155 |
Continuum -Ray Emission Below 10 MeV | p. 162 |
-Ray Line Emission Below 10 MeV from the Orion Region | p. 163 |
Interlude | p. 164 |
-Ray Point Sources | p. 165 |
-Ray Observations of Active Galactic Nuclei | p. 165 |
Nonthermal -Ray Emission Processes in the Jets of Active Galactic Nuclei | p. 172 |
Interlude | p. 176 |
Galactic -Ray Sources | p. 177 |
Immediate Consequences of Galactic Cosmic Ray Observations | p. 179 |
Cosmic Ray Energetics | p. 179 |
Global Cosmic Ray Source Energetics | p. 180 |
Cosmic Ray Scattering, Confinement and Isotropy | p. 182 |
Statistical Mechanics of Charged Particles | p. 183 |
Basic Equations | p. 183 |
Plasma Parameter | p. 183 |
Kinetic Description of Plasmas | p. 187 |
Magnetohydrodynamics of Plasmas | p. 190 |
The Relativistic Vlasov Equation and Maxwell Equations | p. 194 |
Kinetic Theory of Plasma Waves | p. 195 |
Linearization of Kinetic Plasma Equations | p. 195 |
Solution of the Linearized Vlasov Equation | p. 196 |
Dispersion Relation | p. 197 |
The Landau Contour | p. 200 |
Polarization Vector | p. 203 |
Conductivity Tensor in a Homogeneous Hot Magnetized Plasma | p. 204 |
Energy Transfer in Dispersive Media | p. 208 |
Test Wave Approach 1. Waves in Cold Magnetized Plasmas | p. 211 |
Plasma Waves in a Cold Moving Magnetized Plasma | p. 211 |
Plasma Waves in a Cold Magnetized Plasma at Rest | p. 213 |
Cold Unmagnetized Plasma at Rest | p. 215 |
Cold Electron-Proton Plasma | p. 217 |
Propagation Along the Static Magnetic Field | p. 219 |
Propagation Across the Static Magnetic Field | p. 224 |
Oblique Propagation of Low-Frequency Waves | p. 228 |
Oblique Propagation of High-Frequency Waves | p. 231 |
More Rigorous Treatment of Dispersion Relation and Polarization of Low-Frequency Waves | p. 234 |
Faraday Rotation | p. 238 |
Test Wave Approach 2. Waves in Hot Magnetized Isotropic Plasmas | p. 241 |
Conductivity Tensor for Isotropic Distribution Functions | p. 241 |
The Longitudinal Mode | p. 244 |
Superluminal Waves | p. 247 |
Subluminal Waves | p. 249 |
Illustrative Example: Longitudinal Waves in an Equilibrium Electron Plasma | p. 250 |
Superluminal Waves | p. 252 |
Subluminal Waves | p. 253 |
Non-relativistic Plasma Temperatures | p. 254 |
Infinitely Large Speed of Light, c → ∞ | p. 257 |
Solution of the Non-relativistic Dispersion Relation | p. 257 |
Landau Damping of Subluminal Solutions | p. 262 |
Weak Damping Approximation | p. 262 |
The Transverse Modes | p. 263 |
Collisionless Damping of Transverse Oscillations | p. 265 |
An Illustrative Example | p. 266 |
Test Wave Approach 3. Generation of Plasma Waves | p. 269 |
Two-Stream Instability | p. 269 |
Cosmic-Ray-Induced Instabilities | p. 273 |
Parallel Propagating Waves | p. 274 |
Growth Rates at Arbitrary Angles of Propagation | p. 283 |
Cosmic Ray Self-Confinement in Galaxies | p. 286 |
Competition of Wave Growth and Damping | p. 287 |
Damping by Ion-Neutral Collisions | p. 287 |
Nonlinear Landau Damping | p. 287 |
Wave Cascading | p. 289 |
Super-Alfvénic Cosmic Ray Propagation? | p. 290 |
Test Particle Approach 1. Hierarchy of Transport Equations | p. 293 |
Quasilinear Theory | p. 293 |
Quasilinear Fokker-Planck Coefficients | p. 298 |
Unperturbed Particle Orbits | p. 298 |
Fokker-Planck Coefficients for Plasma Wave Turbulence | p. 302 |
The Diffusion Approximation | p. 306 |
Cosmic Ray Anisotropy | p. 309 |
The Diffusion-Convection Transport Equation | p. 310 |
Test Particle Approach 2. Calculation of Transport Parameters | p. 313 |
Linearly Polarized Alfvén Waves | p. 313 |
Alfvén Wave Fokker-Planck Coefficients | p. 315 |
Magnetic Turbulence Tensors | p. 315 |
Slab Linearly Polarized Alfvén Turbulence | p. 318 |
Isotropic Linearly Polarized Alfvén Waves | p. 319 |
Parallel Propagating Magnetohydrodynamic Waves | p. 320 |
Undamped Waves | p. 322 |
Undamped Non-dispersive Alfvén Waves | p. 322 |
Influence of Damping and Dissipation | p. 337 |
Numerical Test of Quasilinear Theory | p. 340 |
Magnetosonic Waves | p. 342 |
Fast Mode Wave Fokker-Planck Coefficients | p. 343 |
Isotropic Fast Mode Waves | p. 345 |
Cosmic Ray Mean Free Path from Fast Mode Waves | p. 357 |
Cosmic Ray Momentum Diffusion Coefficient from Fast Mode Waves | p. 359 |
Fast Mode Time Scale Relation | p. 361 |
Cosmic Transport Parameters from Fast Mode Waves and Slab Alfvén Waves | p. 361 |
Modifications Due to Slab Alfvén Waves | p. 361 |
Transport Parameters in the Case of Admixture of Slab Alfvén Waves to Fast Mode Waves | p. 362 |
Acceleration and Transport Processes of Cosmic Rays | p. 365 |
Structure ofthe Cosmic Ray Transport Equation | p. 365 |
Inclusion of Momentum Losses | p. 367 |
Continuous and Catastrophic Momentum Losses | p. 368 |
Steady-State and Time-Dependent Transport Equations | p. 370 |
Scattering Time Method: Separation of Spatial and Momentum Problem | p. 371 |
Formal Mathematical Solution | p. 371 |
Leaky-Box Equations | p. 372 |
Illustrative Example: Galactic Cosmic Ray Diffusion 1 | p. 373 |
Momentum Problem | p. 375 |
Solutions Without Momentum Diffusion | p. 378 |
Interplanetary Transport of Cosmic Ray Particles | p. 383 |
Solar Flare Events | p. 383 |
Observations | p. 383 |
Comparison with Quasilinear Theory | p. 387 |
Solar Modulation of Galactic Cosmic Rays | p. 388 |
Acceleration of Cosmic Ray Particles at Shock Waves | p. 391 |
Astrophysical Shock Waves | p. 391 |
Magnetohydrodynamic Shock Discontinuities | p. 392 |
Stationary Discontinuities | p. 395 |
Shock Waves | p. 397 |
Alfvén Wave Transmission Through a Parallel Fast Shock | p. 402 |
Basic Equations | p. 403 |
Reflection and Transmission Coefficients | p. 405 |
Only Forward Moving Waves Upstream | p. 405 |
Only Backward Moving Waves Downstream | p. 409 |
Alternative Notation | p. 410 |
Shock Effect on Wavenumbers | p. 410 |
Precursor Streaming Instability | p. 413 |
Cosmic Ray Transport and Acceleration Parameters | p. 415 |
Upstream Cosmic Ray Transport Equation | p. 416 |
Downstream Cosmic Ray Transport Equation | p. 417 |
Scattering Center Compression Ratio | p. 418 |
Importance of Downstream Momentum Diffusion | p. 419 |
Interlude | p. 420 |
Solution of the Transport Equations | p. 421 |
Basic Equations | p. 422 |
Upstream Solution | p. 424 |
Downstream Solution | p. 424 |
Qualitative Results | p. 428 |
Zero Momentum Diffusion | p. 429 |
Finite Momentum Diffusion | p. 431 |
Maximum Particle Energy | p. 433 |
Galactic Cosmic Rays | p. 435 |
Galactic Cosmic Ray Diffusion 2 | p. 435 |
Cosmic Ray Propagation in the Leaky-Box Approximation | p. 436 |
Secondary/Primary Ratio | p. 437 |
Secondary Cosmic Ray Clocks | p. 438 |
Cosmic Ray Propagation Including Interstellar Acceleration | p. 439 |
Mathematical Solution | p. 441 |
Sources of Cosmic Ray Primaries | p. 443 |
Steady-State Primary Particle Spectrum Below Rmax | p. 445 |
Influence of Source Spectral Index Dispersionon the Steady-State Primary Particle Spectrum Below Rmax | p. 450 |
Steady-State Primary Particle Spectrum Above Rmax | p. 452 |
Time-Dependent Calculation | p. 455 |
General Values &neq; 0 | p. 455 |
Special Case = 0 | p. 457 |
Secondary/Primary Ratio Including Interstellar Acceleration | p. 458 |
Formation of Cosmic Ray Momentum Spectra | p. 461 |
Fundamental Physical Picture | p. 461 |
Some Exact Solutions for q = 2 | p. 464 |
Shock Acceleration of Relativistic Electrons Undergoing Radiation Losses | p. 465 |
Shock Acceleration of Relativistic Electrons Undergoing Ionization and Coulomb Losses | p. 467 |
Bessel Function Solutions | p. 467 |
Interlude | p. 468 |
Summary and Outlook | p. 469 |
Cosmic Ray Sources | p. 470 |
Cosmic Ray Isotropy | p. 471 |
Cosmic Ray Isotopic and Elemental Composition | p. 472 |
Electron/Nucleon Ratio | p. 472 |
Formation of Particle Momentum Spectra | p. 474 |
Conclusion | p. 474 |
Appendix | |
Radiation Transport | p. 475 |
Conductivity Tensor in a Hot Magnetized Plasma | p. 479 |
The General Case | p. 481 |
Isotropic Distribution Functions | p. 482 |
Calculation of the Integral (10.3.10) | p. 485 |
The Integral J for Imaginary Values of y | p. 486 |
The Integral J for Non-imaginary Values of y | p. 487 |
A Second Form of the Integral J | p. 490 |
The Integral J for Non-relativistic Temperatures | p. 491 |
References | p. 495 |
Illustration Credits | p. 511 |
Index | p. 513 |
Table of Contents provided by Publisher. All Rights Reserved. |
ISBN: 9783540664659
ISBN-10: 3540664653
Series: Astronomy and Astrophysics Library
Published: 8th October 2002
Format: Hardcover
Language: English
Number of Pages: 536
Audience: Professional and Scholarly
Publisher: Springer Nature B.V.
Country of Publication: DE
Dimensions (cm): 23.39 x 15.6 x 3.02
Weight (kg): 0.85
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