We consider multiphysics applications from algorithmic and architectural perspectives,
where “algorithmic” includes both mathematical analysis and computational complexity, and …

Over the last decade block-structured adaptive mesh refinement (SAMR) has found
increasing use in large, publicly available codes and frameworks. SAMR frameworks have …

Laser plasma-based particle accelerators attract great interest in fields where conventional
accelerators reach limits based on size, cost or beam parameters. Despite the fact that …

The details of the physical mechanism that drives core-collapse supernovae (CCSNe)
remain uncertain. While there is an emerging consensus on the qualitative outcome of …

Mergers of binary neutron stars usually result in the formation of a hypermassive neutron
star (HMNS). Whether and when this remnant collapses to a black hole (BH) depends …

We study the radioactively powered transients produced by accretion disc winds following a
compact object merger. Based on the outflows found in two-dimensional hydrodynamical …

The detonation of a sub-Chandrasekhar-mass white dwarf (WD) has emerged as one of the
most promising Type Ia supernova (SN Ia) progenitor scenarios. Recent studies have …

We present simulations of the multiphase interstellar medium (ISM) at solar neighbourhood
conditions including thermal and non-thermal ISM processes, star cluster formation, and …

We examine the effect of neutrino flavor transformation by the fast flavor instability (FFI) on
long-term mass ejection from accretion disks formed after neutron star mergers. Neutrino …

We investigate the nucleosynthesis of heavy elements in the winds ejected by accretion
discs formed in neutron star mergers. We compute the element formation in disc outflows …