Interacting holographic dark energy in Bianchi type-V and IX universes with variable deceleration parameter
Articles > Article ยท 2020
Authors: H. Eser, C. B. Kilinc
International Journal of Geometric Methods in Modern Physics, International, WoS, 2020, vol 17, pp 2050160-2050160
DOI: 10.1142/s0219887820501601
Summary
In this paper, we study spatially homogeneous and anisotropic Bianchi type-V and IX universes filled with interacting dark matter and holographic dark energy. We obtained the solution of the field equations by using the variable deceleration parameter in the form [Formula: see text]. The cosmological parameters of the models like deceleration and equation of state are obtained. We observe that the deceleration parameter tends to [Formula: see text] which shows an accelerated universe, and the equation of state tends to [Formula: see text] which belongs to [Formula: see text]CDM model. Moreover, we establish the correspondence between holographic dark energy model and quintessence scalar field.