Neutrinos are known to play important roles in many astrophysical scenarios from the early
period of the big bang to current stellar evolution being a unique messenger of the fusion …

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 …

Magnetorotational supernovae are a rare type of core-collapse supernovae where the
magnetic field and rotation play a central role in the dynamics of the explosion. We present …

We perform three-dimensional simulations of magnetorotational supernovae using a
progenitor star with two different initial magnetic field strengths of 1010 and 1012 G in the …

We investigate observable signatures of a first-order quantum chromodynamics (QCD)
phase transition in the context of core-collapse supernovae. To this end, we conduct axially …

The gravitational collapse of rapidly rotating massive stars can lead to the onset of the low
T/| W| instability within the central proto-neutron star (PNS), which leaves strong signatures …

We investigate the final collapse of rotating and non-rotating pulsational pair-instability
supernova progenitors with zero-age-main-sequence masses of 60, 80, and 115 M⊙ and …

We present a simple criterion to predict the explodability of massive stars based on the
density and entropy profiles before collapse. If a pronounced density jump is present near …

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 …

Magnetars are isolated young neutron stars characterised by the most intense magnetic
fields known in the Universe, which power a wide variety of high-energy emissions from …