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Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers
C. Mondal, M. Antonelli, F. Gulminelli +3
Possible strong first-order hadron-quark phase transitions in neutron star interiors leave an imprint on gravitational waves, which could be detected with planned third-generation…
CompOSE Reference Manual
S. Typel, M. Oertel, T. Klähn +10
CompOSE (CompStar Online Supernovae Equations of State) is an online repository of equations of state (EoS) for use in nuclear physics and astrophysics, e.g., in the description of…
What can be learned from a proto-neutron star's mass and radius?
Edwan Preau, Aurélien Pascal, Jérôme Novak +1
We make extensive numerical studies of masses and radii of proto-neutron stars during the first second after their birth in core-collapse supernova events. We use a quasi-static ap…
Maximum mass of compact stars from gravitational wave events with finite-temperature equations of state
Sanika Khadkikar, Adriana R. Raduta, Micaela Oertel +1
We conjecture and verify a set of universal relations between global parameters of hot and fast-rotating compact stars, including a relation connecting the masses of the mass-shedd…
Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations
Sebastian Blacker, Niels-Uwe F. Bastian, Andreas Bauswein +5
We study the possible occurrence of the hadron-quark phase transition (PT) during the merging of neutron star binaries by hydrodynamical simulations employing a set of temperature…
Improved neutrino-nucleon interactions in dense and hot matter for numerical simulations
Micaela Oertel, Aurélien Pascal, Marco Mancini +1
Neutrinos play an important role in compact star astrophysics: neutrino-heating is one of the main ingredients in core-collapse supernovae, neutrino-matter interactions determine t…