N. Michel

activity

20242026

most cited

^{19}

(p, γ)

^{20}

Ne reaction rate and the puzzling calcium abundance in metal poor stars

3 citations · 3 across the 3 of their papers we have counts for

collaborators

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2 papers · 1 filter

nucl-th2026

$^{14}$ N(p, $γ)^{15}$ O $S$ factor and the puzzling solar composition problem

G. X. Dong, X. B. Wang, N. Michel +1

In stellar hydrogen burning, the CNO cycle dominates, with the $^{14}$ N(p, $γ)^{15}$ O reaction being the slowest process. Consequently, this reaction critically influences the solar…

nucl-th2024★ 3 cited

$^{19}$ F $(p, γ)$ $^{20}$ Ne reaction rate and the puzzling calcium abundance in metal poor stars

G. X. Dong, X. B. Wang, N. Michel +1

The $^{19}$ F $(p, γ)$ $^{20}$ Ne reaction is the only process to break out of the CNO cycle at temperature below 0.1 GK and may serve as the origin of calcium in first generation of st…

14N(p,γ)15O S factor and the puzzling solar composition problem

19F(p,γ)20Ne reaction rate and the puzzling calcium abundance in metal poor stars

$^{14}$ N(p, $γ)^{15}$ O $S$ factor and the puzzling solar composition problem

$^{19}$ F $(p, γ)$ $^{20}$ Ne reaction rate and the puzzling calcium abundance in metal poor stars