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after freeze-out, the abundance features can still be changed by several processes (e.g., neutron captures, fission) ● in our NSM calculations, the third peak is shifted towards heavier nuclei due to neutron captures after the r-process freeze-out – fission neutrons from last fission cycle ● β-decays have a large influence on the global abundance distribution (also indirectly, i.e., by influencing the timing of the release of fission neutrons) Fission reactions are fundamental in shaping the r-process abundance pattern from the second peak onwards
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Arcones, A.; Feldmeier, H.; Martínez-Pinedo, G.; Neff, T.; Roth, R.; Schwenk, A., E-mail: sekretariat-theorie@gsi.de, E-mail: hirschegg@gsi.de; Technical University Darmstadt (Germany); vp; 2017; 19 p; Hirschegg 2017: 45. International Workshop on Gross Properties of Nuclei and Nuclear Excitations; Hirschegg (Austria); 15-21 Jan 2017; INIS-AT--1701505; Also available in electronic form from: https://theory.gsi.de/hirschegg/2017/
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