17O(p,a)14N
Rapagnani et al. 2025
R-matrix cross section calculations based on available measurements of the relevant nuclear parameters (energies, widths, strengths of known resonances, interference patterns, etc.), coupled to a Monte Carlo to evaluate the global reaction rate error. For the 65 keV resonance, two opposite interference patterns were investigated, which cannot be constrained by experimental data. The difference between the two rates vanishes above 20 MK.
Link to the paper.
Nuclear reaction rates in the MESA format:
Bruno et al. 2016
Thermonuclear reaction rate based on a new direct determination of the ER=64.5 keV resonance strength performed at the Laboratory for Underground Nuclear Astrophysics (LUNA).
Link to the paper.