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Nojiri, S. and Odintsov, S.D. (2006) Unifying Phantom Inflation with Late-Time Acceleration: Scalar Phan-tom-Non-Phantom Transition Model and Generalized Holographic Dark Energy. General Relativity and Gravitation, 38, 1285-1304.
https://doi.org/10.1007/s10714-006-0301-6

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.