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arxiv: nucl-ex/9607001 · v1 · submitted 1996-07-05 · ⚛️ nucl-ex · astro-ph

The rp-process and new measurements of beta-delayed proton decay of light Ag and Cd isotopes

classification ⚛️ nucl-ex astro-ph
keywords protonbetadecayisotopesnetworkcalculationsdelayedlight
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Recent network calculations suggest that a high temperature rp-process could explain the abundances of light Mo and Ru isotopes, which have long challenged models of p-process nuclide production. Important ingredients to network calculations involving unstable nuclei near and at the proton drip line are $\beta$-halflives and decay modes, i.e., whether or not $\beta$-delayed proton decay takes place. Of particular importance to these network calculation are the proton-rich isotopes $^{96}$Ag, $^{98}$Ag, $^{96}$Cd and $^{98}$Cd. We report on recent measurements of $\beta$-delayed proton branching ratios for $^{96}$Ag, $^{98}$Ag, and $^{98}$Cd at the on-line mass separator at GSI.

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