Compact stars with a small electric charge: the limiting radius to mass relation and the maximum mass for incompressible matter
Jos\'e P. S. Lemos, Francisco J. Lopes, Gon\c{c}alo Quinta, Vilson T., Zanchin

TL;DR
This paper analytically investigates how a small electric charge in incompressible relativistic stars affects their limiting radius-to-mass relation and maximum mass, revealing that charge increases maximum mass and decreases minimum radius.
Contribution
It introduces an analytical scheme to assess the impact of tiny electric charges on the structure of relativistic stars with incompressible matter, extending classical models.
Findings
Maximum mass increases with small electric charge.
Minimum radius decreases when electric charge is present.
Analytical first-order approximation in charge used for the study.
Abstract
One of the stiffest equations of state for matter in a compact star is constant energy density and this generates the interior Schwarzschild radius to mass relation and the Misner maximum mass for relativistic compact stars. If dark matter populates the interior of stars, and this matter is supersymmetric or of some other type, some of it possessing a tiny electric charge, there is the possibility that highly compact stars can trap a small but non-negligible electric charge. In this case the radius to mass relation for such compact stars should get modifications. We use an analytical scheme to investigate the limiting radius to mass relation and the maximum mass of relativistic stars made of an incompressible fluid with a small electric charge. The investigation is carried out by using the hydrostatic equilibrium equation, i.e., the Tolman-Oppenheimer-Volkoff (TOV) equation, together…
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