Kinetic equation with a self-consistent gravitational field and its application to the theory of relic radiation

The kinetic equation for the relativistically invariant distribution function of particles (and also stars or galaxies) moving in a self-consistent or given gravitational field is formulated. The solution of the kinetic equation for the case of Friedmanian cosmological models is obtained. This solution is used for the analysis of relic radiation.

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Year of publication:	2000
Authors:	Akhiezer, A.I. ; Peletminskii, S.V.
Published in:	Physica A: Statistical Mechanics and its Applications. - Elsevier, ISSN 0378-4371. - Vol. 284.2000, 1, p. 161-171
Publisher:	Elsevier
Subject:	Tensor of energy momentum \| Relativistically invariant distribution function \| Kinetic equation with a self-consistent gravitational field \| Relic radiation

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Type of publication:	Article
Source:	RePEc - Research Papers in Economics

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