Tilted Bulk Disordered Distribution Cosmological Model

Abstract:

Bianchi type I bulk viscous fluid tilted cosmological model filled with disordered radiation and heat conduction is investigated. We assume that (constant), where is the coefficient of bulk viscosity and  is the expansion in the model. Here, we assume a linear relation between shear and expansion i.e. =constant, which leads to A=BC, where A, B, C are metric potentials. The physical and geometrical aspects of the model in the presence and absence of bulk viscosity are also discussed.

• Periodical: Advanced Materials Research (Volume 629)
• Pages: 635-640
• DOI: https://doi.org/10.4028/www.scientific.net/AMR.629.635
• Online since: December 2012
• Authors: Anita Bagora, Rakeshwar Purohit
• Keywords: Bianchi Type-I Universe, Bulk Viscosity, Disordered Radiation, Tilted Cosmological Model

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