Orateur
Description
We examine the cosmic evolution of an accelerating universe within the framework of the Einstein–Cartan–Sciama–Kibble theory, employing a flat, homogeneous and isotropic model. In this context, various parameterizations of the equation of state parameter, denoted as w (omega), are considered with respect to the redshift function. We analyze the behavior of cosmological parameters such as deceleration, Om-diagnostic, statefinder and squared speed of sound. It is found that these cosmological parameters are consistent with the current cosmic scenario and recent Planck data from 2018. Additionally, we examine the validity of the generalized second law of thermodynamics at the apparent horizon, taking into account the Bekenstein–Hawking entropy and find it valid for specific choices of constants.
