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.
We study the stability, field theory origin, and viability of two recent dark energy fluid models, analyzing their thermodynamics, temperature evolution, energy conditions, and GSL, to model their behavior through cosmic evolution.
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.