New bound of the mass-to-radius ratio for electrically charged stars
arXiv:1810.03008 · doi:10.1103/PhysRevD.98.124022
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.
9 pages, 1 figure
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