By Ting Ting Sun and others

We investigate radial oscillations of proto-neutron stars, employing equations of state described by the Brueckner-Hartree-Fock theory or the relativistic mean field model, and assuming isentropy and fixed lepton fractions for the internal structure. We calculate the eigenfrequencies and corresponding oscillation functions, which show different characteristics in different mass regions. In... Show more

August 13, 2024

Loading full text...

Similar articles

Loading recommendations...

x1

Radial oscillations of proto-neutron stars

Click on play to start listening