The effect of the electromagnetic fields on the evolution of homogeneous cosmological models near the singularity.
Abstract
Homogeneous cosmological models of all Bianchi types with a general (nondiagonal) metric are considered near the singularity. The spaces are filled with an arbitrary sourceless sixcomponent electromagnetic field (EMF) and a perfect fluid at rest. It is shown that in the general case the models of types VI_{0}, VII_{0}, VIII, and IX have an oscillatory regime. The models of all the other types have Kasner asymptotics. The main result of the present paper is the derivation of the law of rotation of the Kasner axes.
 Publication:

General Relativity and Gravitation
 Pub Date:
 March 1982
 DOI:
 10.1007/BF00756062
 Bibcode:
 1982GReGr..14..279S
 Keywords:

 Astronomical Models;
 Cosmology;
 Electromagnetic Fields;
 Singularity (Mathematics);
 Asymptotic Methods;
 Einstein Equations;
 Ideal Fluids;
 Maxwell Equation;
 Oscillations;
 SpaceTime Functions;
 Astrophysics;
 Cosmological Models