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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...

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Detalles Bibliográficos
Autores principales: Dermer, Charles D. (Autor), Menon, Govind (Autor)
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Princeton, N.J. : Princeton University Press, [2010]
Edición:Course book.
Colección:Book collections on Project MUSE.
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.