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High Energy Radiation from Black Holes

Gamma Rays, Cosmic Rays, and Neutrinos

Charles D. Dermer, Govind Menon

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Princeton University Press img Link Publisher

Naturwissenschaften, Medizin, Informatik, Technik / Thermodynamik

Beschreibung

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.

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Schlagwörter

Classical electromagnetism, Negative energy, Quantum harmonic oscillator, Fermi Gamma-ray Space Telescope, Acceleration, Blazar, Neutron star, Positron, Gravitational field, Fermi acceleration, Neutrino, Plasma (physics), Scattering, Particle physics, Gravitational redshift, Cosmic microwave background, Particle acceleration, Redshift, High Energy Stereoscopic System, Compton scattering, Neutrino detector, Dark matter halo, Hawking radiation, Magnetic dipole, Cosmic ray, Annihilation radiation, Radiation, Nuclear reaction, Accretion (astrophysics), Photon, Helicity (particle physics), Supernova remnant, X-ray background, X-ray binary, Astrophysics, Electron–positron annihilation, Gamma ray, Gamma-ray burst, Radioactive decay, Background radiation, Lorentz factor, Special relativity, Hypernova, Synchrotron radiation, Extragalactic cosmic ray, Plasma oscillation, Black hole, Electromagnetic electron wave, Astrophysical plasma, Magnetic field, Magnetosphere, Neutrino oscillation, Particle beam, Neutron, Electromagnetic spectrum, Ultra-high-energy cosmic ray, Annihilation, Electromagnetic radiation, Creation and annihilation operators, Ergosphere, Spin (physics), Superluminal motion, Relativistic particle, Supermassive black hole, High-energy astronomy, Neutrino astronomy, Synchrotron, Active galactic nucleus, Charged particle, Supernova