5 papers
Nuclear physics uncertainties in neutrino-driven, neutron-rich supernova ejecta
J. Bliss, A. Arcones, F. Montes +1
Neutrino-driven ejecta in core collapse supernovae (CCSNe) offer an interesting astrophysical scenario where lighter heavy elements between Sr and Ag can be synthesized. Previous s…
Nucleosynthesis of "Light" Heavy Nuclei in Neutrino-driven Winds. Role of () reactions
Jorge Pereira, Almudena Arcones, Julia Bliss +1
Neutrino-driven winds following core collapse supernovae have been proposed as a suitable site where the so-called light heavy elements (between Sr to Ag) can be synthetized. For m…
r-Process Nucleosynthesis: Connecting Rare-Isotope Beam Facilities with the Cosmos
C. J. Horowitz, A. Arcones, B. Côté +35
This is an exciting time for the study of r-process nucleosynthesis. Recently, a neutron star merger GW170817 was observed in extraordinary detail with gravitational waves and elec…
Production of Mo and Ru isotopes in neutrino-driven winds: implications for solar abundances and presolar grains
Julia Bliss, Almudena Arcones, Yong-Zhong Qian
The origin of the so-called -isotopes and in the solar system remains a mystery as several astrophysical scenarios fail to account fo…
Survey of astrophysical conditions in neutrino-driven supernova ejecta nucleosynthesis
Julia Bliss, Maximilian Witt, Almudena Arcones +2
Core-collapse supernovae produce elements between Fe and Ag depending on the properties of the ejected matter. Despite the fast progress in supernova simulations in the last decade…