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New fission fragment distributions and r-process origin of the rare-earth elements.
Physical review letters, no. 24 (2013): 242502-242502
Neutron star (NS) merger ejecta offer a viable site for the production of heavy r-process elements with nuclear mass numbers A≳140. The crucial role of fission recycling is responsible for the robustness of this site against many astrophysical uncertainties, but calculations sensitively depend on nuclear physics. In particular, the fissio...More
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