Advances in Astrophysics

Download PDF (558.1 KB) PP. 224 - 237 Pub. Date: November 1, 2016

DOI: 10.22606/adap.2016.13007

• J. P. Singh
  Department of Mathematical Sciences, A. P. S. University, Rewa - 486003, India
• Prashant S. Baghel^*
  Department of Mathematical Sciences, A. P. S. University, Rewa - 486003, India
• Abhay Singh
  Department of Mathematical Sciences, A. P. S. University, Rewa - 486003, India

A new class of a spatially homogeneous and anisotropic Bianchi type V cosmological models of the universe for viscous fluid distribution within the framework of general relativity is investigated by applying suitable functional form for the Hubble parameter H which yields models of the universe that describes an early deceleration and late time acceleration. We have found that cosmological term  being very large at initial times relaxes to a genuine cosmological constant at late times. The physical and kinematical parameters of the models are discussed. The models are found to be compatible with the results of recent observations.

Bianchi V, viscosity, variable cosmological term, anisotropy.

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