Relativistic fluid dynamics: physics for many different scales
Relativistic fluid dynamics: physics for many different scales
The relativistic fluid is a highly successful model used to describe the dynamics of many-particle, relativistic systems. It takes as input basic physics from microscopic scales and yields as output predictions of bulk, macroscopic motion. By inverting the process, an understanding of bulk features can lead to insight into physics on the microscopic scale. Relativistic fluids have been used to model systems as “small” as heavy ions in collisions, and as large as the Universe itself, with “intermediate” sized objects like neutron stars being considered along the way. The purpose of this review is to discuss the mathematical and theoretical physics underpinnings of the relativistic (multiple) fluid model. We focus on the variational principle approach championed by Brandon Carter and his collaborators, in which a crucial element is to distinguish the momenta that are conjugate to the particle number density currents. This approach differs from the “standard” text-book derivation of the equations of motion from the divergence of the stress-energy tensor in that one explicitly obtains the relativistic Euler equation as an “integrability” condition on the relativistic vorticity. We discuss the conservation laws and the equations of motion in detail, and provide a number of (in our opinion) interesting and relevant applications of the general theory.
83pp
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Comer, Gregory L.
734e606a-fbae-4765-b778-4f2d844eb9f4
30 January 2007
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Comer, Gregory L.
734e606a-fbae-4765-b778-4f2d844eb9f4
Andersson, Nils and Comer, Gregory L.
(2007)
Relativistic fluid dynamics: physics for many different scales.
Living Reviews in Relativity, 10 (1), .
Abstract
The relativistic fluid is a highly successful model used to describe the dynamics of many-particle, relativistic systems. It takes as input basic physics from microscopic scales and yields as output predictions of bulk, macroscopic motion. By inverting the process, an understanding of bulk features can lead to insight into physics on the microscopic scale. Relativistic fluids have been used to model systems as “small” as heavy ions in collisions, and as large as the Universe itself, with “intermediate” sized objects like neutron stars being considered along the way. The purpose of this review is to discuss the mathematical and theoretical physics underpinnings of the relativistic (multiple) fluid model. We focus on the variational principle approach championed by Brandon Carter and his collaborators, in which a crucial element is to distinguish the momenta that are conjugate to the particle number density currents. This approach differs from the “standard” text-book derivation of the equations of motion from the divergence of the stress-energy tensor in that one explicitly obtains the relativistic Euler equation as an “integrability” condition on the relativistic vorticity. We discuss the conservation laws and the equations of motion in detail, and provide a number of (in our opinion) interesting and relevant applications of the general theory.
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Published date: 30 January 2007
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Local EPrints ID: 48197
URI: http://eprints.soton.ac.uk/id/eprint/48197
ISSN: 1433-8351
PURE UUID: 00f23743-e9e6-40c2-af0e-62d342545a1d
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Date deposited: 04 Sep 2007
Last modified: 08 Jan 2022 02:48
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Gregory L. Comer
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