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• W2078126784 abstract "Supernova simulations to date have assumed that during core collapse electron captures occur dominantly on free protons, while captures on heavy nuclei are Pauli blocked and are ignored. We have calculated rates for electron capture on nuclei with mass numbers A=65-112 for the temperatures and densities appropriate for core collapse. We find that these rates are large enough so that, in contrast to previous assumptions, electron capture on nuclei dominates over capture on free protons. This leads to significant changes in core collapse simulations." @default.
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• W2078126784 date "2003-06-19" @default.
• W2078126784 modified "2023-10-18" @default.
• W2078126784 title "Electron Capture Rates on Nuclei and Implications for Stellar Core Collapse" @default.
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• W2078126784 doi "https://doi.org/10.1103/physrevlett.90.241102" @default.
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