An LRS Bianchi Type I Bulk Viscous Fluid String Cosmological Model in General Relativity

Details An LRS Bianchi Type I Bulk Viscous Fluid String Cosmological Model in General Relativity An LRS Bianchi Type I Bulk Viscous Fluid String Cosmological Model in General Relativity

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.288..287b&link_type=abstract

Astrophysics and Space Science, v. 288, Issue 3, p. 287-292 (2003).

Astronomy and Astrophysics

Astrophysics

9

Scientific paper

An LRS Bianchi type I string dust cosmological model with and without bulk viscosity following a method used by Letelier and Stachel, is investigated. To get a determine solution, it is assumed that σ∝θ whereσ is shear and θ is scalar of expansion and which leads to A =αBn were n is a constant. The physical and geometrical aspects of the model are also discussed.

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