We report on the gravitational-wave signal computed in the context of a three-dimensional
simulation of a core-collapse supernova explosion of a 15 M⊙ star. The simulation was …

Neutron stars close to the Galactic center are expected to swim in a dense background of
dark matter. For models in which the dark matter has efficient interactions with neutrons, they …

With the advent of modern neutrino and gravitational wave (GW) detectors, the promise of
multimessenger detections of the next galactic core-collapse supernova (CCSN) has …

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) …

We use an asteroseismology method to calculate the frequencies of gravitational waves
(GWs) in a long-term core-collapse supernova simulation, with a mass of 9.6 solar mass …

The eventual detection of gravitational waves from core-collapse supernovae (CCSNe) will
help improve our current understanding of the explosion mechanism of massive stars. The …

Stellar Mass Black Hole Formation and Multimessenger Signals from Three-dimensional
Rotating Core-collapse Supernova Simulations - IOPscience This site uses cookies. By …

Neutrinos are unique probes of core-collapse supernova dynamics, especially in the case of
black hole (BH-) forming stellar collapses, where the electromagnetic emission may be faint …

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 …