We review the ensemble of anticipated gravitational-wave (GW) emission processes in
stellar core collapse and postbounce core-collapse supernova evolution. We discuss recent …

Gravitational-wave emission from stellar collapse has been studied for nearly four decades.
Current state-of-the-art numerical investigations of collapse include those that use …

We present results of a systematic study of failing core-collapse supernovae and the
formation of stellar-mass black holes (BHs). Using our open-source general-relativistic 1.5 D …

We study gravitational waves (GWs) from a set of 2D multigroup neutrino radiation
hydrodynamic simulations of core-collapse supernovae (CCSNe). Our goal is to systematize …

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 present gravitational wave (GW) signal predictions from four 3D multigroup neutrino
hydrodynamics simulations of core-collapse supernovae of progenitors with 11.2, 20 and 27 …

We present the first two-dimensional general relativistic (GR) simulations of stellar core
collapse and explosion with the CoCoNuT hydrodynamics code in combination with the …

Magnetic fields can play a major role in the dynamics of outstanding explosions associated
to violent events such as gamma-ray bursts and hypernovae, since they provide a natural …

Astrophysical observations originate from matter that interacts with radiation or transported
particles. We develop a pragmatic approximation in order to enable multidimensional …

We investigate axisymmetric black hole (BH) formation and its gravitational wave (GW) and
neutrino signals with self-consistent core-collapse supernova simulations of a non-rotating …