X. B. Wang

collaborators

2 papers

nucl-th2026

$^{14}$ N(p, $I^^{3})^{15}$ 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, $I^^{3})^{15}$ O reaction being the slowest process. Consequently, this reaction critically influences the sola…

nucl-th2024

$^{19}$ F $(p, I^^{3})$ $^{20}$ Ne reaction rate and the puzzling calcium abundance in metal poor stars

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

The $^{19}$ F $(p, I^^{3})$ $^{20}$ 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 s…

14N(p,I^3)15O S factor and the puzzling solar composition problem

19F(p,I^3)20Ne reaction rate and the puzzling calcium abundance in metal poor stars

$^{14}$ N(p, $I^^{3})^{15}$ O $S$ factor and the puzzling solar composition problem

$^{19}$ F $(p, I^^{3})$ $^{20}$ Ne reaction rate and the puzzling calcium abundance in metal poor stars