Relativistic Kinetic Theory

With Applications in Astrophysics and Cosmology

Nonfiction, Science & Nature, Science, Physics, Astrophysics & Space Science, General Physics
Cover of the book Relativistic Kinetic Theory by Gregory V. Vereshchagin, Alexey G. Aksenov, Cambridge University Press
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Author: Gregory V. Vereshchagin, Alexey G. Aksenov ISBN: 9781316981450
Publisher: Cambridge University Press Publication: February 16, 2017
Imprint: Cambridge University Press Language: English
Author: Gregory V. Vereshchagin, Alexey G. Aksenov
ISBN: 9781316981450
Publisher: Cambridge University Press
Publication: February 16, 2017
Imprint: Cambridge University Press
Language: English

Relativistic kinetic theory has widespread application in astrophysics and cosmology. The interest has grown in recent years as experimentalists are now able to make reliable measurements on physical systems where relativistic effects are no longer negligible. This ambitious monograph is divided into three parts. It presents the basic ideas and concepts of this theory, equations and methods, including derivation of kinetic equations from the relativistic BBGKY hierarchy and discussion of the relation between kinetic and hydrodynamic levels of description. The second part introduces elements of computational physics with special emphasis on numerical integration of Boltzmann equations and related approaches, as well as multi-component hydrodynamics. The third part presents an overview of applications ranging from covariant theory of plasma response, thermalization of relativistic plasma, comptonization in static and moving media to kinetics of self-gravitating systems, cosmological structure formation and neutrino emission during the gravitational collapse.

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Relativistic kinetic theory has widespread application in astrophysics and cosmology. The interest has grown in recent years as experimentalists are now able to make reliable measurements on physical systems where relativistic effects are no longer negligible. This ambitious monograph is divided into three parts. It presents the basic ideas and concepts of this theory, equations and methods, including derivation of kinetic equations from the relativistic BBGKY hierarchy and discussion of the relation between kinetic and hydrodynamic levels of description. The second part introduces elements of computational physics with special emphasis on numerical integration of Boltzmann equations and related approaches, as well as multi-component hydrodynamics. The third part presents an overview of applications ranging from covariant theory of plasma response, thermalization of relativistic plasma, comptonization in static and moving media to kinetics of self-gravitating systems, cosmological structure formation and neutrino emission during the gravitational collapse.

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