We have performed ab initio neutrino radiation hydrodynamics simulations in three and two
spatial dimensions (3D and 2D) of core-collapse supernovae from the same 15 M☉ …

Beyond iron, a small fraction of the total abundances in the Solar System is made of proton-
rich isotopes, the p-nuclei. The clear understanding of their production is a fundamental …

We provide a set of stellar evolution and nucleosynthesis calculations that applies
established physics assumptions simultaneously to low-and intermediate-mass and massive …

For the origin of heavy rapid neutron capture process (r-process) elements, different sources
have been proposed, eg core-collapse supernovae or neutron star mergers. Old metal-poor …

We have derived new, very accurate abundances of the Fe-group elements Sc through Zn
(Z= 21− 30) in the bright main-sequence turnoff star HD 84937 based on high-resolution …

I study the flavor evolution of a dense neutrino gas by considering vacuum contributions,
matter effects, and neutrino self-interactions. Assuming a system of two flavors in a uniform …

Connecting observations of core-collapse supernova explosions to the properties of their
massive star progenitors is a long-sought, and challenging, goal of supernova science …

Neutrino–matter interactions play an important role in core-collapse supernova (CCSN)
explosions, as they contribute to both lepton number and/or four-momentum exchange …

We use a simple one-zone galactic chemical evolution model to quantify the uncertainties
generated by the input parameters in numerical predictions for a galaxy with properties …

Thermal bombs are a widely used method to artificially trigger explosions of core-collapse
supernovae (CCSNe) to determine their nucleosynthesis or ejecta and remnant properties …