V. G. Mete, Pratiksha Brahmadeo Murade, A. S. Bansod,
At the present paper, Locally Rotationally Symmetric (LRS) Bianchi type-II cosmological model with interacting dark matter (DM) and holographic dark energy (DE) have been discussed.In order to obtain solutions of the field equations, it is assume that the shear scalar ( σ ) is proportional to expansion scalar ( θ ).To have a general description of holographic dark energy and dark matter, a phenomenological parameterization of dark energy in terms of its equation of state (EoS) has been taken.Statefinder diagnostic ...
Tópico(s): Dark Matter and Cosmic Phenomena
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