Isospin Mixing Reveals ${}^{30}$P($p,\gamma$)${}^{31}$S Resonance Influencing Nova Nucleosynthesis

M. B. Bennett, C. Wrede, B. A. Brown +21

The thermonuclear ${}^{30}$P($p,\gamma$)${}^{31}$S reaction rate is critical for modeling the final elemental and isotopic abundances of ONe nova nucleosynthesis, which affect the calibrati…