FRW Bulk Viscous Cosmology with Modified Chaplygin Gas in Flat Space

Abstract

In this paper we study FRW bulk viscous cosmology in presence of modified Chaplygin gas. We write modified Friedmann equations due to bulk viscosity and Chaplygin gas and obtain time-dependent energy density for the special case of flat space.

published by Astrophysics and Space Science see http://inspirehep.net/record/1215969

References in corpus (4)

• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Cosmological Evolution of a Quintom Model of Dark Energy
• Interacting holographic generalized Chaplygin gas model
• Holographic Chaplygin DGP cosmologies

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