Einstein-Cartan-Maxwell-Bianchi type-V cosmological models

Details Einstein-Cartan-Maxwell-Bianchi type-V cosmological models Einstein-Cartan-Maxwell-Bianchi type-V cosmological models

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982gregr..14..691l&link_type=abstract

General Relativity and Gravitation, vol. 14, July 1982, p. 691-701.

Physics

12

Astronomical Models, Cosmology, Einstein Equations, Equations Of State, Field Theory (Physics), Maxwell Equation, Electromagnetic Fields, Space-Time Functions, Stress Tensors, Universe

Scientific paper

Exact cosmological solutions of the Einstein-Cartan-Maxwell equations with spin, 'stiff' matter and an electromagnetic field for Bianchi type-V universes are obtained. A class of nonsingular solutions is presented. The most important characteristic of these solutions is that in one case the effect of the electromagnetic field is to reduce the value of the minimum volume while in another case there exists the possibility of enlarging this value arbitrarily.

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