I explored dark energy models (Barrow holographic, New Barrow Agegraphic, and Barrow Agegraphic) and their connections to modified gravity theories. This contributes to understanding cosmic acceleration and gravity modifications.
Study of the k-essence Scalar Field in the context of inhomogeneous cosmology
This research explores the dynamics of the inhomogeneous k-essence scalar field. It establishes connections between dark energy components and the universe’s scale factor, enhancing our comprehension of cosmic evolution.
Here, we are studying the stability and viability of two of the most recent dark energy models MCAG and MCJG. We are theoretically modelling the behavior of those models in the evolutionary stages of the universe using several thermodynamical parameters.