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Chang, Z., Wu, F.-Q. and Zhang, X. (2006) Constraints on Holographic Dark Energy from X-Ray Gas Mass Fraction of Galaxy Clusters. Physics Letters B, 633, 14-18. https://doi.org/10.1016/j.physletb.2005.10.095

has been cited by the following article:

• TITLE: Interacting Holographic Dark Energy in Bianchi Type-V Universe with Variable Deceleration Parameter

  AUTHORS: Vijay G. Mete, Vaibhav D. Bokey, Vasant S. Bawane

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

  JOURNAL NAME: Open Access Library Journal, Vol.6 No.6, June 14, 2019

  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.