Non-existence of Bianchi type-1 perfect fluid cosmological models in a bi-metric theory of gravitation

Details Non-existence of Bianchi type-1 perfect fluid cosmological models in a bi-metric theory of gravitation Non-existence of Bianchi type-1 perfect fluid cosmological models in a bi-metric theory of gravitation

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.158..169r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 158, no. 1, Aug. 1989, p. 169-171.

Astronomy and Astrophysics

Astrophysics

21

Astronomical Models, Cosmology, Gravitation Theory, Ideal Fluids, Metric Space, Relativity, Tensor Analysis

Scientific paper

It is shown that there do not exist spatially-homogeneous and
anisotropic Bianchi type-I cosmological models in Rosen's (1973)
bi-metric theory of gravitation when the source of the gravitational
field is a perfect fluid distribution. A vacuum cosmological model, in
this theory, is presented and studied.

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