2 papers
astro-ph.SR2026
Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates
Nobuya Nishimura, Carla Froehlich, Thomas Rauscher
Core-collapse supernovae, occurring at the end of massive star evolution, produce heavy elements, including those in the iron peak. Although the explosion mechanism is not yet full…
nucl-th2026
Astrophysical Reaction Rates for Charged-Particle Induced Reactions on Proton-Rich Nuclides
Thomas Rauscher
Astrophysical reaction rates for reactions with proton-rich isotopes of Ne to Bi from stability to the proton dripline were calculated with an updated version of the SMARAGD statis…