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Thermodynamics and Kinetic Theory of Relativistic Gases in 2-D Cosmological Models

G. M. Kremer·F. P. Devecchi
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Abstract

A kinetic theory of relativistic gases in a two-dimensional space is developed in order to obtain the equilibrium distribution function and the expressions for the fields of energy per particle, pressure, entropy per particle and heat capacities in equilibrium. Furthermore, by using the method of Chapman and Enskog for a kinetic model of the Boltzmann equation the non-equilibrium energy-momentum tensor and the entropy production rate are determined for a universe described by a two-dimensional Robertson-Walker metric. The solutions of the gravitational field equations that consider the non-equilibrium energy-momentum tensor - associated with the coefficient of bulk viscosity - show that opposed to the four-dimensional case, the cosmic scale factor attains a maximum value at a finite time decreasing to a "big crunch" and that there exists a solution of the gravitational field equations corresponding to a "false vacuum". The evolution of the fields of pressure, energy density and entropy production rate with the time is also discussed.

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G. M. Kremer, F. P. Devecchi. 2002-02-07. Thermodynamics and Kinetic Theory of Relativistic Gases in 2-D Cosmological Models. https://doi.org/10.1103/physrevd.65.083515

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