A Gamow shell model calculation gives a 19F(p,gamma)20Ne rate at 0.1 GK that is 2.2 times the NACRE value and close to the JUNA measurement, reviving the CNO breakout explanation for calcium in metal-poor stars.
Kious, Determination of nuclear reaction rates lead- ing to the stellar nucleosynthesis of fluorine
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$^{19}$F$(p,\gamma)$$^{20}$Ne reaction rate and the puzzling calcium abundance in metal poor stars
A Gamow shell model calculation gives a 19F(p,gamma)20Ne rate at 0.1 GK that is 2.2 times the NACRE value and close to the JUNA measurement, reviving the CNO breakout explanation for calcium in metal-poor stars.