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 …

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 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 report on the gravitational-wave signal computed in the context of a three-dimensional
simulation of a core-collapse supernova explosion of a 15 M⊙ star. The simulation was …

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 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 …

The next galactic core-collapse supernova (CCSN) has already exploded, and its
electromagnetic (EM) waves, neutrinos, and gravitational waves (GWs) may arrive at any …

We present a detailed theoretical analysis of the gravitational wave (GW) signal of the post-
bounce evolution of core-collapse supernovae (SNe), employing for the first time relativistic …

We study the three-dimensional (3D) hydrodynamics of the post-core-bounce phase of the
collapse of a 27 M☉ star and pay special attention to the development of the standing …

We present predictions for the gravitational wave (GW) emission of 3D supernova
simulations performed for a 15 solar-mass progenitor with the prometheus–vertex code …