Author(s): V. D. Elkar

Email(s): vijayelkar@rediffmail.com

DOI: 10.5958/2321-581X.2021.00002.7   

Address: V. D. Elkar
Department of Mathematics, J.D. Patil Sangludkar Mahavidyalaya, Daryapur, Dist. Amravati.
*Corresponding Author

Published In:   Volume - 12,      Issue - 1,     Year - 2021


ABSTRACT:
In this manuscript we have studied minimally interacting field Dark matter and Holographic Dark energy in Bianchi type VI0 cosmological model with cosmological constant ?. The solution of Einstein’s field equations have been obtained by using relation between metric potential and shear velocity is proportional to scalar expansion and the special law of variation for Hubble parameter which gives a constant value of deceleration parameter. Some physical and geometrical aspects of the model are also discussed.


Cite this article:
V. D. Elkar. Holographic Dark Energy in Bianchi Type VI0 Space Time With Cosmological Constant Λ. Research J. Engineering and Tech. 2021;12(1):08-14. doi: 10.5958/2321-581X.2021.00002.7

Cite(Electronic):
V. D. Elkar. Holographic Dark Energy in Bianchi Type VI0 Space Time With Cosmological Constant Λ. Research J. Engineering and Tech. 2021;12(1):08-14. doi: 10.5958/2321-581X.2021.00002.7   Available on: http://ijersonline.org/AbstractView.aspx?PID=2021-12-1-2


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