We present a gravitational wave (GW) analysis of an extensive series of three-dimensional
magnetohydrodynamical core-collapse simulations. Our 25 models are based on a 15$ M …

We present results from detailed general relativistic simulations of stellar core collapse to a
proto-neutron star, using two different microphysical nonzero-temperature nuclear equations …

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

Aims. We have performed a comprehensive parameter study of the collapse of rotating,
strongly magnetized stellar cores in axisymmetry to determine their gravitational wave …

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 general relativistic (GR) simulations of stellar core collapse to a protoneutron
star, using a microphysical equation of state (EOS) and an approximation of deleptonization …

We have carried out an extensive set of two-dimensional, axisymmetric, purely
hydrodynamic calculations of rotational stellar core collapse with a realistic, finite …

We present results from full general relativistic 3D hydrodynamics simulations of stellar core
collapse of a 70 M⊙ star with spectral neutrino transport. To investigate the impact of …

We have computed the gravitational wave signal from supernova core collapse by using the
most realistic input physics available at present. We start from state-of-the-art progenitor …

We present the gravitational wave analyses from rotating (model s15g) and nearly non-
rotating (model s15h) 3D MHD core collapse supernova simulations at bounce and during …