C. Winteler
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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: The Impact of Fission on R-Process Calculations
The Impact of Fission on R-Process Calculations Open
We have performed r-process calculations in neutron star mergers (NSM) and jets of magnetohydrodynamically driven (MHD) supernovae. In these very neutron-rich environments the fission model of heavy nuclei has an impact on the shape of the…
View article: The influence of fission on neutron star merger r-process and the position of the third r-process peak
The influence of fission on neutron star merger r-process and the position of the third r-process peak Open
The comparison between observational abundance features and those obtained from nucleosynthesis predictions of stellar evolution and/or explosion simulations can scrutinize two aspects: (a) the conditions in the astrophysical production si…
View article: THE ROLE OF FISSION IN NEUTRON STAR MERGERS AND ITS IMPACT ON THE<i>r</i>-PROCESS PEAKS
THE ROLE OF FISSION IN NEUTRON STAR MERGERS AND ITS IMPACT ON THE<i>r</i>-PROCESS PEAKS Open
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or explosion simulations, we can scrutinize two aspects: (a) the conditions in the astrophysical production site and (b) the quality of the nu…