Signatures of strangeness in neutron star merger remnants

Abstract

Neutron star (NS) mergers provide us with information rich in physics using multi-messenger astrophysical observations. One of the probable remnants of such a merger is a differentially rotating hot hypermassive neutron star. The stability of the merger remnant depends crucially on the underlying Equation of State (EoS) and thus provides a method to probe the nature of dense matter in NSs. In this work, we search for possible signatures of strangeness containing matter in the NS interior on the secular stability of the merger remnant. We also use recently proposed methods to make a rough estimate the collapse time of the merger remnant and the threshold mass above which the merger promptly collapses to a black hole.

arXiv comment4 figures

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• Investigating the role of nuclear parameters on oscillation modes in hot Neutron Stars
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• Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
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