Abstract
In the most of existing cosmological investigations, the isotropic space–time models have been considered. In the present work, we focus on beyond this limitation and discuss the influence of anisotropy from thermodynamical perspective. The main goal of this study is to discuss the first and the generalized second laws of thermodynamics in an expanding anisotropic inhomogeneous model of the cosmos from the teleparallel gravity perspective, which is filled with the baryonic matter (BM) interacting with the dark energy (DE) and the cold dark matter (CDM) by assuming the cosmos as a thermodynamical system, which is bounded by a dynamical horizon.
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