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- W1588821034 abstract "We argue that the standard derivation of the Gamow-Teller contribution to the $^{37}mathrm{Cl}$ solar neutrino capture cross section from the $^{37}mathrm{Ca}$ delayed proton spectrum yields a B(GT) distribution that is too weak and shifted to lower excitation energies. Because the redistribution of Gamow-Teller strength occurs primarily above the analog state, where the neutrino reaction phase space is small, it has only a small effect (4%) on the solar neutrino cross section. However, our observations help resolve the discrepancy between the $^{37}mathrm{Ca}$ ensuremath{beta}-decay and $^{37}mathrm{Cl}$(p,n) Gamow-Teller mappings." @default.
- W1588821034 created "2016-06-24" @default.
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- W1588821034 date "1987-09-01" @default.
- W1588821034 modified "2023-09-26" @default.
- W1588821034 title "Cl37solar neutrino capture cross section" @default.
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- W1588821034 doi "https://doi.org/10.1103/physrevc.36.879" @default.
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