Inhomogeneous wet dark fluid cosmological model with time dependent \Lambda-term

2015 ◽  
Vol 9 ◽  
pp. 575-585
Author(s):  
V. G. Mete ◽  
V. D. Elkar ◽  
K. R. Mule
2010 ◽  
Vol 50 (2) ◽  
pp. 339-348 ◽  
Author(s):  
K. S. Adhav ◽  
M. V. Dawande ◽  
R. S. Thakare ◽  
R. B. Raut

2015 ◽  
Vol 55 (1) ◽  
pp. 526-534 ◽  
Author(s):  
Subrata Kumar Sahu ◽  
Endale Nigatu Kantila ◽  
Dawit Melese Gebru

2015 ◽  
Vol 357 (2) ◽  
Author(s):  
Subrata Kumar Sahu ◽  
Ayelign Gota Goda ◽  
Gebretsadik Gidey Weldemariam

2020 ◽  
Vol 98 (7) ◽  
pp. 636-642 ◽  
Author(s):  
V.J. Dagwal

This study presents mesonic tilted cosmological models with wet dark fluid in the F(T) theory of gravity, which is an extension of the Teleparallel theory of gravity, where T is the torsion scalar. In this paper, a new idea is introduced about the F(T) theory of gravity with the help of tilt angle, heat conduction, and mesonic wet dark fluid. The cosmological evolution in F(T) models is investigated. The physical and geometrical aspects of the models are also discussed.


2019 ◽  
Vol 16 (08) ◽  
pp. 1950127 ◽  
Author(s):  
S. Angit ◽  
Rakesh Raushan ◽  
R. Chaubey

We investigate the dynamical systems analysis of Friedmann–Robertson–Walker (FRW) cosmological model with wet dark fluid. A new equation of state for the dark energy component of the Universe has been used. It is modeled by the equation of state [Formula: see text], which can describe a liquid, e.g. water. To analyze the evolution equations, we have introduced suitable transformation of variables. The evolution of corresponding solutions is presented by curves in the phase–plane diagram. The nature of critical points are analyzed and stable attractors are examined for our cosmological model. We determine the classical stabilities of these cosmologies. We also examine the transition of early decelerating stage of the Universe to present the accelerating stage of the Universe.


2021 ◽  
Vol 13 (3) ◽  
pp. 869-878
Author(s):  
S. C. Wankhade ◽  
A. S. Nimkar ◽  
A. M. Pund

This paper investigates a Bianchi type VIII cosmological model with wet dark fluid in Barber self-creation theory of gravitation. To get the determinate model of the Universe, we have assumed the relationship between metric coefficients R and S. Also, the behavior of the model in the radiation Universe and the physical implications of the model are discussed in detail.


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