3 papers
nucl-th2026
N(p,O 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 N(p,O reaction being the slowest process. Consequently, this reaction critically influences the sola…
nucl-ex2025
Unbound neutron strength in C and the N=16 shell gap
J. Lois-Fuentes, B. Fernández-DomÃnguez, F. Delaunay +61
Significant continuum strength has been observed to be populated in C produced in the d(C,p) reaction at a beam energy of 17.2~MeV/nucleon. The strength appears at gr…
nucl-th2024
FNe reaction rate and the puzzling calcium abundance in metal poor stars
G. X. Dong, X. B. Wang, N. Michel +1
The FNe 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…