Tilted Bianchi type-VI0 wet dark fluid cosmological model

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

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.


2014 ◽  
Vol 11 (05) ◽  
pp. 1450043 ◽  
Author(s):  
Rajesh Kumar ◽  
S. K. Srivastava

In General Relativity, the electric (Eαβ) and magnetic (Hαβ) parts of Weyl tensor are the gravitational quantities that play an analogous role to the electric and magnetic fields in classical electromagnetism. The present study deals with Bianchi type VI0 cosmological model with purely magnetic (PM) and purely electric (PE) space time. Conditions of PM (PE) solutions satisfy Eαβ = 0, Hαβ ≠ 0 (Hαβ = 0, Eαβ≠ 0). We present a new class of cosmological model with PM and PE solutions when the source of gravitation is perfectly fluid. Some physical and geometrical properties of the models are also discussed.


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