Bianchi Type-V Bulk Viscous Fluid String Dust Cosmological Model In General Relativity

Details Bianchi Type-V Bulk Viscous Fluid String Dust Cosmological Model In General Relativity Bianchi Type-V Bulk Viscous Fluid String Dust Cosmological Model In General Relativity

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.300..387b&link_type=abstract

Astrophysics and Space Science, Volume 300, Issue 4, pp.387-394

Mathematics

Logic

25

Bianchi Type V, Bulk Viscous String Dust, Cosmological

Scientific paper

Bianchi Type-V bulk viscous fluid string dust cosmological model in General Relativity is investigated. It has been shown that if coefficient of bulk viscosity (ζ) is inversely proportional to the expansion (θ) in the model then string cosmological model for Bianchi Type-V space-time is possible. In absence of bulk viscosity (ζ), i.e. when ζ → 0, then there is no string cosmological model for Bianchi Type-V space-time. The physical and geometrical aspects of the model are also discussed.

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