Non-static plane symmetric bulk viscous dark energy cosmological model

KV Vidyasagar; MV Ramakrishna; A Chandra Mouli

doi:10.33545/26648636.2024.v6.i1a.76

Non-static plane symmetric bulk viscous dark energy cosmological model

Author(s):

KV Vidyasagar, MV Ramakrishna and A Chandra Mouli

Abstract:

In this paper, we have investigated Non-static plane symmetric universe in the presence of pressure less dark matter and bulk viscous fluid of dark energy within the framework of general relativity. To find the solution of Einstein’s field equations, we assumed that the hybrid expansion law. The physical and geometric properties of the cosmological model are also well discussed.

DOI: 10.33545/26648636.2024.v6.i1a.76

Pages: 29-33 | 435 Views 128 Downloads

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International Journal of Physics and Mathematics

How to cite this article:

KV Vidyasagar, MV Ramakrishna and A Chandra Mouli. Non-static plane symmetric bulk viscous dark energy cosmological model. Int. J. Phys. Math. 2024;6(1):29-33. DOI: 10.33545/26648636.2024.v6.i1a.76

Vol. 6, Issue 1, Part A (2024)

Non-static plane symmetric bulk viscous dark energy cosmological model

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