Julia Bliss
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View article: The Nuclear Reaction Network WinNet
The Nuclear Reaction Network WinNet Open
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 environments and conditions. This ranges from the calculation of t…
View article: The nuclear reaction network WinNet
The nuclear reaction network WinNet Open
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 environments and conditions. This ranges from the calculation of the …
View article: Nuclear physics uncertainties in neutrino-driven, neutron-rich supernova ejecta
Nuclear physics uncertainties in neutrino-driven, neutron-rich supernova ejecta Open
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 studies emphasized the important role that ($\alpha,n$) reac…
View article: Nucleosynthesis of lighter heavy elements in neutrino-driven winds
Nucleosynthesis of lighter heavy elements in neutrino-driven winds Open
Neutrino-driven winds following core-collapse supernova explosions are an exciting astrophysical site for the formation of the lighter heavy elements between strontium up to (possibly) silver. Observations of very old stars, so-called ultr…
View article: Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds
Nucleosynthesis of Mo and Ru isotopes in neutrino-driven winds Open
The solar system origin of the p-isotopes ⁹²,⁹⁴Mo and ⁹⁶,⁹⁸Ru is a long-lasting mystery. Several astrophysical scenarios failed to explain their formation. Moreover, SiC X grains show a different abundance ratio of ⁹⁵,⁹⁷Mo than in the sola…