The kinetic gas universe

Abstract A description of many-particle systems, which is more fundamental than the fluid approach, is to consider them as a kinetic gas. In this approach the dynamical variable in which the properties of the system are encoded, is the distribution of the gas particles in position and velocity space...

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Main Authors: Manuel Hohmann, Christian Pfeifer, Nicoleta Voicu
Format: Article
Language:English
Published: SpringerOpen 2020-09-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-020-8391-y
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author Manuel Hohmann
Christian Pfeifer
Nicoleta Voicu
author_facet Manuel Hohmann
Christian Pfeifer
Nicoleta Voicu
author_sort Manuel Hohmann
collection DOAJ
description Abstract A description of many-particle systems, which is more fundamental than the fluid approach, is to consider them as a kinetic gas. In this approach the dynamical variable in which the properties of the system are encoded, is the distribution of the gas particles in position and velocity space, called 1-particle distribution function (1PDF). However, when the gravitational field of a kinetic gas is derived via the Einstein-Vlasov equations, the information about the velocity distribution of the gas particles is averaged out and therefore lost. We propose to derive the gravitational field of a kinetic gas directly from its 1PDF, taking the velocity distribution fully into account. We conjecture that this refined approach could possibly account for the observed dark energy phenomenology.
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spelling doaj.art-1e2bb9d6aee44d76b51bac6918c7599a2022-12-22T00:02:49ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-09-018091410.1140/epjc/s10052-020-8391-yThe kinetic gas universeManuel Hohmann0Christian Pfeifer1Nicoleta Voicu2Laboratory of Theoretical Physics, Institute of Physics, University of TartuLaboratory of Theoretical Physics, Institute of Physics, University of TartuFaculty of Mathematics and Computer Science, Transilvania UniversityAbstract A description of many-particle systems, which is more fundamental than the fluid approach, is to consider them as a kinetic gas. In this approach the dynamical variable in which the properties of the system are encoded, is the distribution of the gas particles in position and velocity space, called 1-particle distribution function (1PDF). However, when the gravitational field of a kinetic gas is derived via the Einstein-Vlasov equations, the information about the velocity distribution of the gas particles is averaged out and therefore lost. We propose to derive the gravitational field of a kinetic gas directly from its 1PDF, taking the velocity distribution fully into account. We conjecture that this refined approach could possibly account for the observed dark energy phenomenology.http://link.springer.com/article/10.1140/epjc/s10052-020-8391-y
spellingShingle Manuel Hohmann
Christian Pfeifer
Nicoleta Voicu
The kinetic gas universe
European Physical Journal C: Particles and Fields
title The kinetic gas universe
title_full The kinetic gas universe
title_fullStr The kinetic gas universe
title_full_unstemmed The kinetic gas universe
title_short The kinetic gas universe
title_sort kinetic gas universe
url http://link.springer.com/article/10.1140/epjc/s10052-020-8391-y
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