Supernova theory, numerical and analytic, has made remarkable progress in the past
decade. This progress was made possible by more sophisticated simulation tools, especially …

Rotating relativistic stars have been studied extensively in recent years, both theoretically
and observationally, because of the information they might yield about the equation of state …

We present here the first 2D rotating, multigroup, radiation magnetohydrodynamics (RMHD)
simulations of supernova core collapse, bounce, and explosion. In the context of rapid …

Supernova models with a full spectral treatment of the neutrino transport are presented,
employing the prometheus/vertex neutrino-hydrodynamics code with a variable Eddington …

Core-collapse supernovae are among the most energetic explosions in the universe
marking the catastrophic end of massive stars. In spite of rigorous studies for several …

We explore the influence of non-axisymmetric modes on the dynamics of the collapsed core
of rotating, magnetized high-mass stars in three-dimensional simulations of a rapidly rotating …

We study hydrodynamic instabilities during the first seconds of core-collapse supernovae by
means of 2D simulations with approximative neutrino transport and boundary conditions that …

We investigate the explosion of stars with zero-age main-sequence masses between 20 and
35 M⊙ and varying degrees of rotation and magnetic fields including ones commonly …

Spherically symmetric (1D) and two-dimensional (2D) supernova simulations for progenitor
stars between 11 and 25 are presented, making use of the Prometheus/Vertex neutrino …

We study the evolution of a supernova core from the beginning of the gravitational collapse
of a 15 M☉ star up to 1 s after core bounce. We present results of spherically symmetric …