Bianchi type-I cosmological model with quadratic equation of state

2015 ◽  
Vol 357 (1) ◽  
Author(s):  
D. R. K. Reddy ◽  
K. S. Adhav ◽  
M. A. Purandare
2015 ◽  
Vol 2015 ◽  
pp. 1-12 ◽  
Author(s):  
G. P. Singh ◽  
Binaya K. Bishi

This paper deals with the study of Bianchi type-I universe in the context off(R,T)gravity. Einstein’s field equations inf(R,T)gravity have been solved in the presence of cosmological constantΛand quadratic equation of state (EoS)p=αρ2-ρ, whereα≠0is a constant. Here, we have discussed two classes off(R,T)gravity; that is,f(R,T)=R+2f(T)andf(R,T)=f1(R)+f2(T). A set of models has been taken into consideration based on the plausible relation. Also, we have studied some physical and kinematical properties of the models.


2018 ◽  
Vol 15 (11) ◽  
pp. 1850194 ◽  
Author(s):  
Mahbubur Rahman Mollah ◽  
Kangujam Priyokumar Singh ◽  
Pheiroijam Suranjoy Singh

The paper deals with the investigation of a homogeneous and anisotropic space-time described by Bianchi type-III metric with perfect fluid in Lyra geometry setting. Exact solutions of Einstein’s field equations have been obtained under the assumption of quadratic equation of state (EoS) of the form [Formula: see text], where [Formula: see text] is a constant and strictly [Formula: see text]. The physical and geometrical aspects are also examined in detail.


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