New bound of the mass-to-radius ratio for electrically charged stars
Cristian Stelea, Marina-Aura Dariescu, Ciprian Dariescu

TL;DR
This paper derives a new theoretical bound on the mass-to-radius ratio for electrically charged stars, extending existing bounds for uncharged stars to include electric charge effects.
Contribution
It introduces a novel bound on the mass-radius ratio for charged stars, generalizing previous uncharged bounds using a solution-generating technique.
Findings
Derived a new bound on the mass-radius ratio for charged stars.
Extended uncharged star bounds to include electric charge effects.
Provides a theoretical framework for analyzing charged compact objects.
Abstract
Using a general solution-generating technique for electrically charged relativistic stars with spherical symmetry, we derive a new bound on the mass-radius ratio. This compactness bound is based on the already established bounds for uncharged interior solutions and it will provide the corresponding generalizations in presence of the electric charge.
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