We have simulated the collapse and evolution of the core of a solar-metallicity 40 M⊙ star
and find that it explodes vigorously by the neutrino mechanism, despite its very high" …

The radioactive isotopes 44 Ti and 56 Ni are important products of explosive
nucleosynthesis, which play a key role in supernova (SN) diagnostics and have been …

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 …

Using 20 long-term 3D core-collapse supernova simulations, we find that lower
compactness progenitors that explode quasi-spherically due to the short delay to explosion …

We study in detail the ejecta conditions and theoretical nucleosynthetic results for 18 three-
dimensional core-collapse supernova (CCSN) simulations done by F ornax. Most of the …

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 …

We present the first numerical study of gravitational waves (GWs) from collapsar disks, using
state-of-the-art 3D general relativistic magnetohydrodynamic simulations of collapsing stars …

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 …