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

A.I. Akhiezer and S.V. Peletminskii

Physica A: Statistical Mechanics and its Applications, 2000, vol. 284, issue 1, 161-171

Abstract: 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.

Keywords: Tensor of energy momentum; Relativistically invariant distribution function; Kinetic equation with a self-consistent gravitational field; Relic radiation (search for similar items in EconPapers)
Date: 2000
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Persistent link: https://EconPapers.repec.org/RePEc:eee:phsmap:v:284:y:2000:i:1:p:161-171

DOI: 10.1016/S0378-4371(00)00188-6

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