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 solut...

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Bibliographic Details
Published inPhysica A Vol. 284; no. 1-4; pp. 161 - 171
Main Authors Akhiezer, A.I., Peletminskii, S.V.
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.09.2000
Subjects
Kinetic equation with a self-consistent gravitational field
Relativistically invariant distribution function
Relic radiation
Tensor of energy momentum
Tensor of energy momentum
Relativistically invariant distribution function
Relic radiation
Kinetic equation with a self-consistent gravitational field
05.20.Dd
98.80.Bp
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Summary: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.
ISSN:0378-4371
1873-2119
DOI:10.1016/S0378-4371(00)00188-6