Anisotropic Dark Energy and the Generalized Second Law of Thermodynamics
M. Sharif, Farida Khanum
TL;DR
This paper explores how anisotropic dark energy interacting with dark matter and radiation affects the validity of the generalized second law of thermodynamics in a Bianchi type I universe, highlighting the dependence on shear, skewness, and equation of state.
Contribution
It investigates the impact of anisotropic dark energy interactions on thermodynamic law validity within a Bianchi type I cosmological model.
Findings
Validity depends on shear, skewness, and equation of state parameters.
The law holds under specific conditions related to anisotropy.
Results provide insights into thermodynamics in anisotropic cosmologies.
Abstract
We consider a Bianchi type model in which anisotropic dark energy is interacting with dark matter and anisotropic radiation. With this scenario, we investigate the validity of the generalized second law of thermodynamics. It is concluded that the validity of this law depends on different parameters like shear, skewness and equation of state.
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