Bianchi type-I models in self-creation theory of gravitation

Details Bianchi type-I models in self-creation theory of gravitation Bianchi type-I models in self-creation theory of gravitation

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.168..193v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 168, no. 2, June 1990, p. 193-199. Research supported by the Council of Sc

Astronomy and Astrophysics

Astrophysics

11

Cosmology, Gravitation Theory, Gravitational Fields, Astronomical Models, Relativistic Theory

Scientific paper

This paper studies the spatially homogeneous and anisotropic Bianchi type-I cosmological models in Barber's (1982) second self-creation theory of gravitation, when the source of the gravitational field is a perfect fluid. The field equations and the models are presented, and the physical and geometrical properties of these models, which represent radiation-dominated and Zel'dovich universes in the self-creation cosmology, are discussed. It is observed that the models are expanding, shearing, nonrotating, and nonsingular.

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