Neutrino–neutrino refraction dominates the flavor evolution in core-collapse supernovae,
neutron star mergers, and the early Universe. Ordinary neutrino flavor conversions develop …

Nonspherical mass motions are a generic feature of core-collapse supernovae, and
hydrodynamic instabilities play a crucial role in the explosion mechanism. The first …

To reach a deeper understanding of the origin of elements in the periodic table, we construct
Galactic chemical evolution (GCE) models for all stable elements from C (A= 12) to U (A …

Double neutron star (DNS) systems represent extreme physical objects and the endpoint of
an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems …

We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a
broad range of progenitor masses. This is the largest collection of sophisticated 3D …

To date, modern three-dimensional (3D) supernova (SN) simulations have not demonstrated
that explosion energies of 10 51 erg (= 1 bethe= 1 B) or more are possible for neutrino …

Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …

Light curves, explosion energies, and remnant masses are calculated for a grid of
supernovae resulting from massive helium stars that have been evolved including mass …

We present a suite of seven 3D supernova simulations of non-rotating low-mass progenitors
using multigroup neutrino transport. Our simulations cover single star progenitors with zero …

We study the impact of large-scale perturbations from convective shell burning on the core-
collapse supernova explosion mechanism using 3D multigroup neutrino hydrodynamics …