Bianchi Type-III String Cosmological Model with Bulk Viscosity in General Relativity

Details Bianchi Type-III String Cosmological Model with Bulk Viscosity in General Relativity Bianchi Type-III String Cosmological Model with Bulk Viscosity in General Relativity

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005chphl..22...29w&link_type=abstract

Chinese Physics Letters, Volume 22, Issue 1, pp. 29-32 (2005).

Physics

37

Scientific paper

The Bianchi type-III cosmological model for a cloud string with bulk viscosity are studied. To obtain a determinate solution, it is assumed that the coefficient of bulk viscosity is a power function of the scalar of expansion ζ = kθm and the shear scalar is proportional to scalar of expansion σproptoθ, which leads to the relation between metric potentials B = Cn. The physical features of the model are also discussed. It is found that the power index m has significant influence on the string model. There is a ``big bang'' start in the model when m<=1 but there is no the big-bang start when m>1. In the special case m = 0, the model reduces to the string model of constant coefficient of bulk viscosity that was the result previously given in the literature.

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