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

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 …

Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …

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 …

Thus far, judging the fate of a massive star (either a neutron star [NS] or a black hole) solely
by its structure prior to core collapse has been ambiguous. Our work and previous attempts …

We present a detailed report of the connection between long‐duration gamma‐ray bursts
(GRBs) and their accompanying supernovae (SNe). The discussion presented here places …

We examine the effect of neutrino flavor transformation by the fast flavor instability (FFI) on
long-term mass ejection from accretion disks formed after neutron star mergers. Neutrino …

We have performed ab initio neutrino radiation hydrodynamics simulations in three and two
spatial dimensions (3D and 2D) of core-collapse supernovae from the same 15 M☉ …

In this paper, we present the results of our three-dimensional, multigroup, multineutrino-
species radiation/hydrodynamic simulation using the state-of-the-art code fornax of the …

Models of neutrino-driven core-collapse supernova explosions have matured considerably
in recent years. Explosions of low-mass progenitors can routinely be simulated in 1D, 2D …