Bianchi type-VI(0) cosmological models in Schwinger's scalar-tensor theory

Details Bianchi type-VI(0) cosmological models in Schwinger's scalar-tensor theory Bianchi type-VI(0) cosmological models in Schwinger's scalar-tensor theory

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.166..123r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 166, no. 1, April 1990, p. 123-128.

Astronomy and Astrophysics

Astrophysics

1

Astronomical Models, Cosmology, Gravitation Theory, Ideal Fluids, Scalars, Space-Time Functions, Tensors

Scientific paper

Spatially-homogeneous and anisotropic Bianchi type-VI(0) cosmological
models are obtained in the scalar-tensor theory of gravitation proposed
by Schwinger (1970), both in vacuum and in the presence of perfect fluid
with pressure equal to energy density. Some properties of the models are
discussed.

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