no code implementations • 11 Feb 2021 • Edwan Preau, Aurélien Pascal, Jérôme Novak, Micaela Oertel
We show that if masses and radii of a proto-neutron star can be determined in the first second after the birth, e. g. from gravitational wave emission, no information could be obtained on the corresponding cold neutron star and therefore on the cold nuclear equation of state.
High Energy Astrophysical Phenomena
