Study of Dark Energy Stars in a Buchdahl Spacetime

Citation: Manuel Malaver, "Study of Dark Energy Stars in a Buchdahl Spacetime", Universal Library of Innovative Research and Studies, Volume 01, Issue 02.

Copyright: This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Abstract

In this paper we obtained some spherically stellar configurations that represent new models of dark energy stars specifying particular forms for gravitational potential and the electric field intensity which allows solve the Einstein-Maxwell field equations. We have chosen the metric potential proposed by Buchdahl (1959) with the equation of state pr = wp where pr is the radial pressure, p is the dark energy density and w is the dark energy parameter. We found that the radial pressure, the anisotropy factor, energy density, metric coefficients, mass function, charge density are regular and well behaved in the stellar interior but the causality conditions and of strong energy are not satisfied. These models have great application in physics and cosmology due to the fact that several independent observations indicate that the universe is in a phase of accelerated expansion which can be explained by the presence of dark energy that has not been detected.

Keywords: Dark Energy Stars, Metric Potential, Causality Condition, Strong Energy Condition, Accelerated Expansion.

https://doi.org/10.70315/uloap.ulirs.2024.0102001