Charged Gravastar in a Dark Energy Universe

TL;DR

This paper models charged gravastars within a dark energy universe, highlighting how charge influences their stability, potential to form black holes or naked singularities, and challenging the gravastar-black hole alternative hypothesis.

Contribution

It introduces a charged gravastar model with a thin shell and analyzes how charge affects stability and the formation of black holes or naked singularities.

Findings

Charge can stabilize or destabilize gravastars.

Presence of charge can lead to black hole or naked singularity formation.

Naked singularities can emerge from gravastar instabilities.

Abstract

Here we constructed a charged gravastar model formed by an interior de Sitter spacetime, a charged dynamical infinitely thin shell with an equation of state and an exterior de Sitter-Reissner-Nordstr\"om spacetime. We find that the presence of the charge is crucial to the stability of these structures. It can as much favor the stability of a bounded excursion gravastar, and still converting it in a stable gravastar, as make disappear a stable gravastar, depending on the range of the charge considered. There is also formation of black holes and, above certain values, the presence of the charge allows the formation of naked singularity . This is an important example in which a naked singularity emerges as a consequence of unstabilities of a gravastar model, which reinforces that gravastar is not an alternative model to black hole.