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arxiv: astro-ph/9907274 · v1 · submitted 1999-07-20 · 🌌 astro-ph · nucl-ex· nucl-th

Shell-model half-lives for the N=82 nuclei and their implications for the r-process

classification 🌌 astro-ph nucl-exnucl-th
keywords half-livesr-processshell-modelnucleiadoptedagreementbeta-flowcalculation
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We have performed large-scale shell-model calculations of the half-lives and neutron-branching probabilties of the r-process waiting point nuclei at the magic neutron number N=82. We find good agreement with the measured half-lives of 129Ag and 130Cd. Our shell-model half-lives are noticeably shorter than those currently adopted in r-process simulations. Our calculation suggests that 130Cd is not produced in beta-flow equilibrium with the other N=82 isotones on the r-process path.

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