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Relativistic Astrophysics of the Transient Universe

- Gravitation, Hydrodynamics and Radiation

Relativistic Astrophysics of the Transient Universe

- Gravitation, Hydrodynamics and Radiation
Tjek vores konkurrenters priser
In this decade, the transient universe will be mapped out in great detail by the emerging wide-field multiwavelength surveys, and neutrino and gravitational-wave detectors, promising to probe the astronomical and physical origin of the most extreme relativistic sources. This volume introduces the physical processes relevant to the source modeling of the transient universe. Ideal for graduate students and researchers in astrophysics, this book gives a unified treatment of relativistic flows associated with compact objects, their dissipation and emission in electromagnetic, hadronic and gravitational radiation. After introducing the source classes, the authors set out various mechanisms for creating magnetohydodynamic outflows in winds, jets and blast waves and their radiation properties. They then go on to discuss properties of accretion flows around rotating black holes and their gravitational wave emission from wave instabilites with implications for the emerging gravitational wave experiments. Graduate students and researchers can gain an understanding of data analysis for gravitational-wave data.
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Tjek vores konkurrenters priser
In this decade, the transient universe will be mapped out in great detail by the emerging wide-field multiwavelength surveys, and neutrino and gravitational-wave detectors, promising to probe the astronomical and physical origin of the most extreme relativistic sources. This volume introduces the physical processes relevant to the source modeling of the transient universe. Ideal for graduate students and researchers in astrophysics, this book gives a unified treatment of relativistic flows associated with compact objects, their dissipation and emission in electromagnetic, hadronic and gravitational radiation. After introducing the source classes, the authors set out various mechanisms for creating magnetohydodynamic outflows in winds, jets and blast waves and their radiation properties. They then go on to discuss properties of accretion flows around rotating black holes and their gravitational wave emission from wave instabilites with implications for the emerging gravitational wave experiments. Graduate students and researchers can gain an understanding of data analysis for gravitational-wave data.
Produktdetaljer
Sprog: Engelsk
Sider: 354
ISBN-13: 9781107010734
Indbinding: Hardback
Udgave:
ISBN-10: 110701073X
Kategori: Astrofysik
Udg. Dato: 5 jul 2012
Længde: 22mm
Bredde: 173mm
Højde: 251mm
Forlag: Cambridge University Press
Oplagsdato: 5 jul 2012
Forfatter(e) Maurice H. P. M. Van Putten, Amir Levinson


Kategori Astrofysik


ISBN-13 9781107010734


Sprog Engelsk


Indbinding Hardback


Sider 354


Udgave


Længde 22mm


Bredde 173mm


Højde 251mm


Udg. Dato 5 jul 2012


Oplagsdato 5 jul 2012


Forlag Cambridge University Press

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