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تسجيل مستخدم جديدElectrically charged supermassive twin stars
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We assume that ultra dense neutron stars are endowed with a distribution of electric charge and study the twin star solutions and their properties resulting from a first order transition from confined hadronic to deconfined quark phases. Two distinct phenomenological treatments for the phase transition are considered and the values for the maximum gravitational masses of the hadronic and hybrid configurations are estimated for different values of the total electric charge. We demonstrate that stable compact charged twin stars exist, with charged stars being more massive than their neutral counterparts, and that the standard ${2.2}{M_{odot}}$ constraint is surpassed for large values of the electric charge. In particular, our results suggest that the unknown compact object of $approx {2.6}{M_{odot}}$ measured in the GW190814 event might be a charged star.
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