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.
Cite this paper
Mete, V. G. , Bokey, V. D. and Bawane, V. S. (2019). Interacting Holographic Dark Energy in Bianchi Type-V Universe with Variable Deceleration Parameter. Open Access Library Journal, 6, e5498. doi: http://dx.doi.org/10.4236/oalib.1105498.
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