¹³C(p,g)¹⁴N

Skowronski et al. 2023

Re-evaluated thermonuclear rate based on cross section measurements performed at the Laboratory for Underground Nuclear Astrophysics, down to the lowest energies to date (Ec.m.=60  keV)., hence reaching for the first time the high energy tail of hydrogen burning in the shell of giant stars. Compared with most of the previous literature, these results are systematically lower by 30% on average.

Link to the paper.

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Nuclear reaction rate in the MESA format:

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