High Energy Radiation from Black Holes : Gamma Rays, Cosmic Rays, and Neutrinos /
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...
Autores principales: | , |
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Formato: | Electrónico eBook |
Idioma: | Inglés |
Publicado: |
Princeton, N.J. :
Princeton University Press,
[2010]
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Edición: | Course book. |
Colección: | Book collections on Project MUSE.
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Temas: | |
Acceso en línea: | Texto completo |
Tabla de Contenidos:
- Frontmatter
- Contents
- Preface
- ACKNOWLEDGMENTS
- Chapter One. Introduction
- Chapter Two. Relativistic Kinematics
- Chapter Four. Physical Cosmology
- Chapter Five. Radiation Physics of Relativistic Flows
- Chapter Six. Compton Scattering
- Chapter Seven. Synchrotron Radiation
- Chapter Eight. Binary Particle Collision Processes
- Chapter Nine. Photohadronic Processes
- Chapter Nine. Pair Production
- Chapter Eleven. Blast-Wave Physics
- Chapter Twelve. Introduction to Fermi Acceleration
- Chapter Thirteen. First-Order Fermi Acceleration
- Chapter Fourteen. Second-Order Fermi Acceleration
- Chapter Fifteen. The Geometry of Spacetime
- Chapter Sixteen. Black-Hole Electrodynamics
- Chapter Seventeen. High-Energy Radiations from Black Holes
- Appendix A. Essential Tensor Calculus
- Appendix B. Mathematical Functions
- Appendix C. Solutions of the Continuity Equation
- Appendix D. Basics of Monte Carlo Calculations
- Appendix E. Supplementary Information
- Appendix F. Glossary and Acronym List
- References
- Index.