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 …

In the last decade, enormous progress has been achieved in the understanding of the
various facets of coalescing double neutron star and neutron black hole binary systems. One …

We present a detailed, three-dimensional hydrodynamic study of the neutrino-driven winds
emerging from the remnant of a neutron star merger. Our simulations are performed with the …

We examine magnetorotationally driven supernovae as sources of r-process elements in the
early Galaxy. On the basis of thermodynamic histories of tracer particles from a three …

We present a comprehensive nucleosynthesis study of the neutrino-driven wind in the
aftermath of a binary neutron star merger. Our focus is the initial remnant phase when a …

Entropy solutions have been widely accepted as the suitable solution framework for systems
of conservation laws in several space dimensions. However, recent results in De Lellis and …

A standard paradigm for the existence of solutions in fluid dynamics is based on the
construction of sequences of approximate solutions or approximate minimizers. This …

Context. Many problems in astrophysics feature flows which are close to hydrostatic
equilibrium. However, standard numerical schemes for compressible hydrodynamics may …

ABSTRACT We present an Advanced Spectral Leakage (ASL) scheme to model neutrinos in
the context of core-collapse supernovae (CCSNe) and compact binary mergers. Based on …

Context. Modeling core-collapse supernovae (SNe) with neutrino transport in three
dimensions (3D) requires tremendous computing resources and some level of …