Using the numerical simulation data for two-dimensional core-collapse supernova, we
examine the protoneutron star (PNS) asteroseismology with the relativistic Cowling …

Gravitational waves (GWs) provide unobscured insight into the birthplace of neutron stars
and black holes in core-collapse supernovae (CCSNe). The nuclear equation of state (EOS) …

The future detection of gravitational waves (GWs) from a Galactic core-collapse supernova
will provide information on the physics inside protoneutron stars (PNS). In this work, we …

Context. The growth of hydrodynamical instabilities is key to triggering a core-collapse
supernova explosion during the phase of stalled accretion shock, immediately after the birth …

Gravitational waves (GWs) can provide crucial information about the central engines of core-
collapse supernovae (CCSNe). In order to unveil the nature of GW emission in CCSNe, we …

Three-dimensional modeling has reached a level of maturity to provide detailed predictions
of the gravitational wave emission in neutrino-driven core collapse supernovae. We review …

The equation of state (EOS) of nuclear dense matter plays a crucial role in many
astrophysical phenomena associated with neutron stars (NSs). Fluid oscillations are one of …

Gravitational waves (GWs) hold great potential for an unobscured view of protoneutron stars
(PNSs) formed as a result of stellar collapses. While waiting for discovery, deepening the …

We investigate the oscillations of neutron stars using a purely Newtonian approach and
three other pseudo-Newtonian formulations. Our work is motivated by the fact that pseudo …