Astrophysical weak-interaction rates for selected $A=20$ and $A=24$ nuclei

Abstract

We have evaluated the electron capture rates on ${}^{20}$Ne, ${}^{20}$F, ${}^{24}$Mg, ${}^{24}$Na and the ${\hat{I}}^2$ decay rates for ${}^{20}$F and ${}^{24}$Na at temperature and density conditions relevant for the late-evolution stages of stars with $M=8$-12 M${}_{\odot }$. The rates are based on recent experimental data and large-scale shell model calculations. We show that the electron capture rates on ${}^{20}$Ne, ${}^{24}$Mg and the ${}^{20}$F, ${}^{24}$Na ${\hat{I}}^2$-decay rates are based on data in this astrophysical range, except for the capture rate on ${}^{20}$Ne, which we predict to have a dominating contribution from the second-forbidden transition between the ${}^{20}$Ne and ${}^{20}$F ground states in the density range $\log \ddot{I}Y_e({\mathrm{g}\mathrm{cm}}^{-3})=9.3$-9.6. The dominance of a few individual transitions allows us to present the various rates by analytical expressions at the relevant astrophysical conditions. We also derive the screening corrections to the rates.

21 pages, 12 figures