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Accelerating Bianchi Type-VIh Cosmological Model with Variable EoS Parameter


Affiliations
1 Department of Mathematics, Sant Gadge Baba Amravati University, Amravati (444602), India
     

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We have studied anisotropic and homogeneous Bianchi type-VIh cosmological models of the universe with variable equation of state (EoS) parameter (w) in General Relativity. A special form of deceleration parameter (q) which gives an early deceleration and late time accelerating cosmological model has been utilized to solve the Einstein's field equations. The geometrical and physical aspects of the models are also studied.

Keywords

Bianchi Type-Vih Space-Time, Dark Energy, Special form of Deceleration Parameter.
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  • Accelerating Bianchi Type-VIh Cosmological Model with Variable EoS Parameter

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Authors

K. S. Adhav
Department of Mathematics, Sant Gadge Baba Amravati University, Amravati (444602), India
D. R. K. Reddy
Department of Mathematics, Sant Gadge Baba Amravati University, Amravati (444602), India
G. B. Tayade
Department of Mathematics, Sant Gadge Baba Amravati University, Amravati (444602), India

Abstract


We have studied anisotropic and homogeneous Bianchi type-VIh cosmological models of the universe with variable equation of state (EoS) parameter (w) in General Relativity. A special form of deceleration parameter (q) which gives an early deceleration and late time accelerating cosmological model has been utilized to solve the Einstein's field equations. The geometrical and physical aspects of the models are also studied.

Keywords


Bianchi Type-Vih Space-Time, Dark Energy, Special form of Deceleration Parameter.