Interacting Holographic Dark Energy in Bianchi Type-V Universe with Variable Deceleration Parameter - Open Access Library Journal

OALibJ > Vol.6 No.6, June 2019

Open Access Library Journal

Volume 6, Issue 6 (June 2019)

ISSN Print: 2333-9705 ISSN Online: 2333-9721

Google-based Impact Factor: 0.73 Citations

Interacting Holographic Dark Energy in Bianchi Type-V Universe with Variable Deceleration Parameter ()

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DOI: 10.4236/oalib.1105498 464 Downloads 1,282 Views Citations

Author(s)

Vijay G. Mete¹, Vaibhav D. Bokey², Vasant S. Bawane³

Affiliation(s)

¹R.D.I.K. & K.D. College, Badnera, India.
²Nehru Mahavidyalaya, Ner Parsopant, India.
³M. F. Arts, Comm. & S. C. Science Mahavidyalaya, Warud, India.

ABSTRACT

The present study deals with spatially homogeneous and anisotropic Bianchi Type-V universe filled with interacting dark matter and holographic dark energy. The exact solutions of Einstein’s equations are obtained by using the variable deceleration parameter in the form a(t)=(sinh(at))^1/n (Chawla et al. [1]). The physical properties of the model are obtained and discussed in details.

KEYWORDS

Bianchi Type-V Universe, Holographic Dark Energy, Interacting Dark Fluids, Variable Deceleration Parameter

Share and Cite:

Mete, V. , Bokey, V. and Bawane, V. (2019) Interacting Holographic Dark Energy in Bianchi Type-V Universe with Variable Deceleration Parameter. Open Access Library Journal, 6, 1-5. doi: 10.4236/oalib.1105498.

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