In this paper, we analyze the neutrino-driven winds that emerge in 12 unprecedentedly long-
duration 3D core-collapse supernova simulations done using the code F ornax. The 12 …

The radioactive isotopes 44 Ti and 56 Ni are important products of explosive
nucleosynthesis, which play a key role in supernova (SN) diagnostics and have been …

We study in detail the ejecta conditions and theoretical nucleosynthetic results for 18 three-
dimensional core-collapse supernova (CCSN) simulations done by F ornax. Most of the …

We present the state-of-the-art single-zone nuclear reaction network WinNet, which is
capable of calculating the nucleosynthetic yields of a large variety of astrophysical …

We present core-collapse supernova simulations including nuclear reaction networks that
impact explosion dynamics and nucleosynthesis. The different composition treatment can …

The production of heavy elements is one of the main by-products of the explosive end of
massive stars. A long sought goal is finding differentiated patterns in the nucleosynthesis …

Material expelled from binary neutron star (BNS) mergers can harbour r-process
nucleosynthesis and power a kilonova (KN), both intimately related to the astrophysical …

We perform a set of two-dimensional, non-relativistic, hydrodynamics simulations for
supernova-like explosions associated with stellar core collapse of rotating massive stars into …

Abstract We report C, N, Si, and Al–Mg isotope data for 39 presolar X silicon carbide (SiC)
and four silicon nitride grains—a group of presolar grains that condensed in the remnants of …

Core-collapse supernovae (CCSNe) are the violent explosions of massive stars. Yet, their
detailed explosion mechanism is still a matter of intense research. By performing three …