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Constraints for stellar electron-capture rates on \(^{86}\)Kr via the \(^{86}\)Kr(\(t\),\(^{3}\)He\(+\gamma\))\(^{86}\)Br reaction and the implications for core-collapse supernovae
Titus, R; Ney, E M; Zegers, R G T; Bazin, D; Belarge, J; et al. arXiv.org, Aug 12, 2019.You might have access to this document
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