Bianchi type V and VI(0) cosmological models in Lyra geometry

Details Bianchi type V and VI(0) cosmological models in Lyra geometry Bianchi type V and VI(0) cosmological models in Lyra geometry

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.182..189s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 182, no. 2, Aug. 1991, p. 189-200. Research supported by Council for Scien

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Astronomical Models, Computational Astrophysics, Cosmology, Universe, Equations Of State, Relativistic Theory, Transformations (Mathematics)

Scientific paper

Consideration is given to Bianchi type V and VI(0) models in Lyra
geometry in cases where the gage function beta is time dependent or
constant. The physical behavior of these models is discussed.

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