Orateur
David A López Magaña
(Universidad Nacional Autónoma de México)
Description
Within the standard understanding of cosmology, the existence of Dark Matter and Dark Energy is considered. Together, these constitute approximately 95% of the Universe; however, their behavior is not fully understood. Through reconstructions, the phenomenological behavior of both Dark Energy and Dark Matter can be inferred from astronomical observations. This work addresses the interpolation method for reconstructing the Equation of State $\omega(z)$ and the normalized energy density $f(z)=\frac{\rho(z)}{\rho_0}$, which is used to study Dark Energy on its own and the Dark Sector (Dark Energy and Dark Matter) as a whole.
Auteur
David A López Magaña
(Universidad Nacional Autónoma de México)