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• W3009795241 abstract "Assuming the universality of weak interactions, we have studied the weak processes such as β-decay and electron capture using the nuclear gross theory of beta decay (GTBD). We evaluate the β± and electron capture decay rates and the neutrino–nucleus cross sections as a function of the energy of the incident neutrino, for Eν < 250 MeV. The evaluation performed some years ago for the electron neutrino–nucleus reactions in the mass region A < 70 is extended to the heavy one A < 220 for a set of 965 nuclear species of astrophysical interest. The nuclei are separated according to its parity in even–even, even–odd, odd–odd, and odd–even nuclei, both for β±-decay and electron capture. The obtained cross sections are interpolated by means of a fourth-degree polynomial function in Eν. The coefficients in these polynomials are obtained and later fitted as a function of A and Z. The fitting procedure is described in detail paying special attention to the root mean square deviations in the adjustment. These polynomial functions provide a tool for the systematic evaluation of the cross sections needed in astrophysical processes like the r-process during the nucleosynthesis of supernovae." @default.
• W3009795241 created "2020-03-13" @default.
• W3009795241 creator A5032909371 @default.
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• W3009795241 date "2020-03-03" @default.
• W3009795241 modified "2023-10-07" @default.
• W3009795241 title "Systematic Calculation of Neutrino–Nucleus Cross Section Available for Astrophysical Applications" @default.
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• W3009795241 doi "https://doi.org/10.1007/s13538-020-00737-y" @default.
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