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 …

Abstract The Einstein Telescope (ET), a proposed European ground-based gravitational-
wave detector of third-generation, is an evolution of second-generation detectors such as …

We present a new moment-based energy-integrated neutrino transport code for neutron star
merger simulations in general relativity. In the merger context, ours is the first code to include …

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 …

The details of the physical mechanism that drives core-collapse supernovae (CCSNe)
remain uncertain. While there is an emerging consensus on the qualitative outcome of …

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 …

We present in this paper a public data release of an unprecedentedly large set of core-
collapse supernova (CCSN) neutrino emission models, comprising 100 detailed 2D …

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 …

Multi-messenger astrophysics has produced a wealth of data with much more to come in the
future. This enormous data set will reveal new insights into the physics of core-collapse …