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Microscopic foundations of relativis...

Denicol, Gabriel S.

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Microscopic foundations of relativistic fluid dynamics

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Microscopic foundations of relativistic fluid dynamics/ by Gabriel S. Denicol, Dirk H. Rischke.
作者:	Denicol, Gabriel S.
其他作者:	Rischke, Dirk H.
出版者:	Cham :Springer International Publishing : : 2021.,
面頁冊數:	1 online resource (xvi, 292 p.) :ill. (some col.), digital ;24 cm.
內容註:	Relativistic Fluid Dynamics -- Linear Stability and Causality -- Analytical Solutions and Transient Dynamics -- Microscopic Origin of Transport Coeffcients: Linear-Response Theory -- Fluid Dynamics from Kinetic Theory: Traditional Approaches -- Method of Moments: Equilibrium Reference State -- Method of Moments: Convergence Properties -- Fluid Dynamics from the Method of Moments -- Method of Moments: Anisotropic Reference State.
Contained By:	Springer Nature eBook
標題:	Relativistic fluid dynamics. -
電子資源:	https://doi.org/10.1007/978-3-030-82077-0
ISBN:	9783030820770

Microscopic foundations of relativistic fluid dynamics
Denicol, Gabriel S.

Microscopic foundations of relativistic fluid dynamics[electronic resource] /by Gabriel S. Denicol, Dirk H. Rischke. - Cham :Springer International Publishing :2021. - 1 online resource (xvi, 292 p.) :ill. (some col.), digital ;24 cm. - Lecture notes in physics,v. 9901616-6361 ;. - Lecture notes in physics ;v. 990..

Relativistic Fluid Dynamics -- Linear Stability and Causality -- Analytical Solutions and Transient Dynamics -- Microscopic Origin of Transport Coeffcients: Linear-Response Theory -- Fluid Dynamics from Kinetic Theory: Traditional Approaches -- Method of Moments: Equilibrium Reference State -- Method of Moments: Convergence Properties -- Fluid Dynamics from the Method of Moments -- Method of Moments: Anisotropic Reference State.

This book provides an introduction to relativistic dissipative fluid dynamics, with particular emphasis on its derivation from microscopic transport theory. After a phenomenological derivation of relativistic dissipative fluid dynamics from the second law of thermodynamics, the intrinsic instabilities of relativistic Navier-Stokes theory are discussed. In turn, analytical solutions of relativistic dissipative fluid dynamics are presented. Following, the authors discuss several theories and approaches to derive transport coefficients in dissipative fluid dynamics such as the Chapman-Enskog theory, the theory of Israel and Stewart, and a more recent derivation of relativistic dissipative fluid dynamics based on kinetic theory, which constitutes the main focus of the second part of this book. This book is intended for advanced graduate students and researchers in physics and requires basic knowledge of the theory of special and general relativity. It should be of particular interest to researchers that apply relativistic fluid dynamics in cosmology, astrophysics, and high-energy nuclear physics.

ISBN: 9783030820770

Standard No.: 10.1007/978-3-030-82077-0doiSubjects--Topical Terms:

2086786
Relativistic fluid dynamics.

LC Class. No.: QA912 / D46 2021

Dewey Class. No.: 532.05

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520 $a This book provides an introduction to relativistic dissipative fluid dynamics, with particular emphasis on its derivation from microscopic transport theory. After a phenomenological derivation of relativistic dissipative fluid dynamics from the second law of thermodynamics, the intrinsic instabilities of relativistic Navier-Stokes theory are discussed. In turn, analytical solutions of relativistic dissipative fluid dynamics are presented. Following, the authors discuss several theories and approaches to derive transport coefficients in dissipative fluid dynamics such as the Chapman-Enskog theory, the theory of Israel and Stewart, and a more recent derivation of relativistic dissipative fluid dynamics based on kinetic theory, which constitutes the main focus of the second part of this book. This book is intended for advanced graduate students and researchers in physics and requires basic knowledge of the theory of special and general relativity. It should be of particular interest to researchers that apply relativistic fluid dynamics in cosmology, astrophysics, and high-energy nuclear physics.
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