30 citations · 42 across the 5 of their papers we have counts for
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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 solar…
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 st…
Gamow shell model description of the radiative capture reaction BC
G. X. Dong, X. B. Wang, N. Michel +1
In low metallicity supermassive stars, the hot chain can serve as an alternative way to produce the CNO nuclei. In the astrophysical environment of high temperature, the proto…
Gamow shell model description of the radiative capture reaction LiLi
G. X. Dong, X. B. Wang, N. Michel +1
The LiLi reaction plays a critical role in several reaction chains leading to the nucleosynthesis of nuclei. Due to unstable nature of Li and the unavaila…
Comparison between Variational Monte Carlo and Shell Model Calculations of Neutrinoless Double Beta Decay Matrix Elements in Light Nuclei
X. B. Wang, A. C. Hayes, J. Carlson +4
Benchmark comparisons between many-body methods are performed to assess the ingredients necessary for an accurate calculation of neutrinoless double beta decay matrix elements. She…