Challenge on the Astrophysical R-process Calculation with Nuclear Mass Models

Details Challenge on the Astrophysical R-process Calculation with Nuclear Mass Models Challenge on the Astrophysical R-process Calculation with Nuclear Mass Models

2008-07-16

arxiv.org/abs/0807.2509v1

Chin.Phys.Lett.25:2429,2008

Physics

Nuclear Physics

Nuclear Theory

3 pages, 3 figures

Scientific paper

10.1088/0256-307X/25/7/027

Our understanding of the rapid neutron capture nucleosynthesis process in universe depends on the reliability of nuclear mass predictions. Initiated by the newly developed mass table in the relativistic mean field theory (RMF), in this paper the influence of mass models on the $r$-process calculations is investigated assuming the same astrophysical conditions. The different model predictions on the so far unreachable nuclei lead to significant deviations in the calculated r-process abundances.

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