Bianchi type-III cosmological model in four- and five-dimensional bimetric theory of relativity

Details Bianchi type-III cosmological model in four- and five-dimensional bimetric theory of relativity Bianchi type-III cosmological model in four- and five-dimensional bimetric theory of relativity

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.295..331a&link_type=abstract

Astrophysics and Space Science, Volume 295, Issue 3, pp.331-337

Astronomy and Astrophysics

Astrophysics

Bimetric Relativity, Bianchi Type Models, Scalar Meson Field, Mesonic Perfect Fluid

Scientific paper

Four- and five-dimensional Bianchi type-III cosmological model in Rosen
(1980) bimetric theory of gravitation is considered. Restricting to a
particular type of background metric, it is observed that the Bianchi
type-III cosmological model does not exist in case of both meson field
and mesonic perfect fluid. Hence only vacuum model can be obtained.

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