Vacuum Bianchi type-III cosmological models in Ross and Dunn theories of gravitation

Details Vacuum Bianchi type-III cosmological models in Ross and Dunn theories of gravitation Vacuum Bianchi type-III cosmological models in Ross and Dunn theories of gravitation

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.175..241s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 175, no. 2, Jan. 1991, p. 241-245.

Physics

1

Astronomical Models, Cosmology, Gravitation Theory, Field Theory (Physics), Tensors

Scientific paper

Spatially-homogeneous exact Bianchi type III vacuum models are developed
on the basis of scalar-tensor theories of gravitation proposed by Ross
(1972) and Dunn (1974). The vacuum models are written in the form of
equations for the anisotropic expansion of the universe with time. The
physical properties of these models are discussed.

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