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Open Access Original Articles

String Cosmological Model with Bulk Viscosity in Higher Dimensional Space Time

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pp. 117–123Vol. 5Issue 2November 2007DOI: 10.1080/1726037X.2007.10698531XML
Received:
03 Jul 2007
Published Online:
03 Jun 2013
Article type:
Original Articles
Language:
EN
Article no.:
1726037X.2007.10698531
Pages:
117–123

Abstract

We have investigated the bulk viscous fluid string dust cosmological model in the higher dimensional space-time. To obtain a determinate solution, it is assumed that the coefficient of bulk viscosity is a power function of the scalar of expansion τ = Aθ (t) and the scalar of expansion is proportional to shear scalar, which leads to a relation between metric potentials A = KR where A and R are function of time. It is also shown that bulk viscosity plays an important role on the evolution of the universe. The physical and geometrical aspects of the model are also discussed.

Keywords

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