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High-energy astrophysics /
This textbook covers all the essentials, weaving together the latest theory with the experimental techniques, instrumentation, and observational methods astronomers use to study high-energy radiation from space.
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Princeton, N.J. :
Princeton University Press,
©2009.
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| Colección: | Princeton series in astrophysics.
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| Temas: | |
| Acceso en línea: | Texto completo |
Tabla de Contenidos:
- Introduction and motivation. The field of high-energy astrophysics
- Energies, luminosities, and timescales
- Atmospheric absorption
- Experimental tools of high energy astrophysics
- High-energy telescopes
- The high-energy sky. X-ray maps up to 10 keV
- The sky between 10 keV and 1 MeV
- Surveys up to 30 MeV
- The highest energy maps produced in earth orbit
- Relativity. Special relativity
- Relativistic transformation of physical laws
- General relativity
- Static spacetimes
- Particle acceleration. Gravity
- Electromagnetic fields
- Fermi acceleration.
- Radiative processes. The radiation field
- Intensity
- Thermal Bremsstrahlung
- Single particle synchrotron emissivity
- Thermal synchrotron
- Nonthermal synchrotron
- Compton scattering
- Accretion of plasma. Hydrodynamics
- Bondi-Hoyle accretion
- Roche lobe geometry in binaries and accretion from a companion star
- Formation of a disk. Accretion disk theory
- Viscosity and radial disk structure
- Standard thin disk theory
- Accretion columns
- Two-temperature thin disks
- Thick accretion disks. Thick-disk structure
- Radiatively inefficient flows.
- Pulsing sources. Radio pulsars
- X-ray pulsars
- Cataclysmic variables
- Black holes in binaries. Early discovery of black holes
- The archetypal HMXB Cygnus X-1
- X-ray Novae
- QPOs in black-hole binaries
- Bursting stars. X-ray burst sources
- Gamma-ray burst sources
- Supermassive black holes in AGNs. Their discovery and identification
- Nearby objects
- Supermassive black holes in AGNs
- The high-energy background. Cosmic rays
- Galaxy clusters
- Diffuse emission.