168 citations · 383 across the 9 of their papers we have counts for
9 papers
The nuclear reaction network WinNet
M. Reichert, C. Winteler, O. Korobkin +13
We present the state-of-the-art single-zone nuclear reaction network WinNet that is capable of calculating the nucleosynthetic yields of a large variety of astrophysical environmen…
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…
Impact of reactions on weak r-process in neutrino-driven winds
Julia Bliss, Almudena Arcones, Fernando Montes +1
After a successful core-collapse supernova, a neutrino-driven wind develops where it is possible to synthesize lighter heavy elements (). In the early galaxy, the origin o…
Nucleosynthesis of molybdenum in neutrino-driven winds
Julia Bliss, Almudena Arcones
Neutrino-driven winds that follow core-collapse supernovae are an exciting astrophysical site for the production of heavy elements. Although hydrodynamical simulations show that th…
Nucleosynthesis of elements between Sr and Ag in neutron- and proton-rich neutrino-driven winds
A. Arcones, J. Bliss
Neutrino-driven winds that follow core collapse supernovae were thought to be the site where half of the heavy elements are produced by the r-process. Although recent hydrodynamic…