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Effects of a strong phase transition on supernova explosions, compact stars and their mergers

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arxiv 2203.17188 v1 pith:PWKW3X2O submitted 2022-03-31 nucl-th astro-ph.HE

Andreas Bauswein , David Blaschke , Tobias Fischer This is my paper · ORCID
classification nucl-thastro-ph.HE
keywords compactphasestrongmattermergersstarsupernovatransition
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We outline a theoretical approach supporting strong phase transitions from normal nuclear matter to the deconfined quark-gluon plasma, in the equation of state (EOS) for compact star matter. Implications of this hypothesis are discussed for astrophysical applications. Special emphasis is devoted to potentially detectable signatures, which can be directly related with the occurrence of a sufficiently strong phase transition. Therefore, simulations of core-collapse supernovae and binary compact star mergers are considered, including the subsequent emission of gravitational waves and, in the case of supernova, in addition the neutrinos play the role of messengers.

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Cited by 1 Pith paper

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  1. Individual Neutrino Masses From a Supernova

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    Using time-of-flight delays of the three neutrino mass eigenstates across sharp supernova features, a galactic supernova at 10 kpc could individually constrain or measure neutrino masses at JUNO, with precision that d...

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