The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …

In a previously presented proof-of-principle study, we established a parameterized
spherically symmetric explosion method (PUSH) that can reproduce many features of core …

In a previously presented proof-of-principle study, we established a parameterized
spherically symmetric explosion method (PUSH) that can reproduce many features of core …

We propose a simple model to explain the velocity of young neutron stars. We attempt to
confirm a relationship between the amount of mass ejected in the formation of the neutron …

The accurate description of neutrino opacities is central to both the core-collapse supernova
(CCSN) phenomenon and the validity of the explosion mechanism itself. In this work, we …

Recent developments in multi-dimensional simulations of core-collapse supernovae have
considerably improved our understanding of this complex phenomenon. In addition to that …

Core-collapse supernovae (CCSNe) are the first polluters of heavy elements in the galactic
history. As such, it is important to study the nuclear compositions of their ejecta, and …

We investigate the precision with which the supernova neutrino spectra can be
reconstructed in water Cherenkov detectors, in particular the large scale Hyper-Kamiokande …

Context. Tracing unstable isotopes produced in supernova nucleosynthesis provides a
direct diagnostic of supernova explosion physics. Theoretical models predict an extensive …

In order to investigate the impact of collective neutrino oscillations (CNOs) on the neutrino
signal from a nearby supernova, we perform three-flavor neutrino oscillation simulations …