FRW Viscous Cosmology for Varying G, c and Λ, with Inhomogeneous Equation of State

被引:0
|
作者
Ghogre, A. S. [1 ]
Khadekar, G. S. [2 ]
Raut, Deepti [3 ]
机构
[1] Yeshwantrao Chavan Coll Engn, Dept Math, Hingna Rd, Nagpur 441110, India
[2] Rashtrasant Tukadoji Maharaj Nagpur Univ, Dept Math, Mahatma Jyotiba Phule Educ Campus,Amravati Rd, Nagpur 440033, India
[3] Rajiv Gandhi Coll Engn, Dept Math, Hingna Rd, Nagpur 441110, India
来源
关键词
VSL theory; Viscous fluid; Dark energy;
D O I
10.26713/cma.v14i2.2017
中图分类号
O1 [数学];
学科分类号
0701 ; 070101 ;
摘要
In this paper, the Freidmann equations described by inhomogeneous equation of state (EOS) of the form p = (y -1)pc2 + A(t), for a bulk viscosity media, are considered. The time dependent parameter A is considered as a linear combination of the terms as A(t) = A0 + A1RR and the bulk viscosity as ( = (0H-1p, where R is a scale factor and A0, A1 and (0, are all constants. The resultant equation to the scale factor is solved to get the exact solution by choosing some special parameters, in the framework of variable speed of light (VSL) theory.
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收藏
页码:493 / 501
页数:9
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