We calculate the gravitational-wave (GW) signatures of detailed three-dimensional (3D) core-
collapse supernova simulations spanning a range of massive stars. Most of the simulations …

One of the active debates in core-collapse supernova (CCSN) theory is how significantly
neutrino flavor conversions induced by neutrino-neutrino self-interactions change the …

Neutrinos are known to undergo flavor conversion processes among the three flavors. The
fast flavor conversion (FFC) has been the central piece of flavor conversions taking place in …

Gravitational waveform predictions from 3D simulations of explosions of non-rotating
massive stars with no magnetic fields have been extensively studied. However, the impact of …

Core-collapse supernovae (CCSNe) are predicted to produce gravitational waves (GWs)
that may be detectable by Advanced LIGO/Virgo. These GW signals carry information from …

Using relativistic supernova simulations of massive progenitor stars with a quark-hadron
equation of state (EOS) and a purely hadronic EOS, we identify a distinctive feature in the …

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 …

We present a methodology based on the implementation of a fully connected neural network
algorithm to estimate the temporal evolution of the high-frequency gravitational wave …

Hydrodynamical instabilities, such as the standing accretion shock instability (SASI), play an
essential role in the dynamics of core-collapse supernovae, with observable imprints in the …

Neutron stars (NSs) are observed with high space velocities and elliptical orbits in binaries.
The magnitude of these effects points to natal kicks that originate from asymmetries during …