23Na(p,g)24Mg
Boeltzig et al. 2019
Evaluation of the nuclear reaction rate based on measurements of the resonance strengths at Ep = 140 and 251keV, which are the main contributors to the reaction rate at 50 ≲ T ≲ 110MK, performed at the Laboratory for Underground Nuclear Astrophysics (LUNA). Two complementary detection approaches were used: high efficiency with a 4π BGO detector for the 140 keV resonance, and high resolution with a HPGe detector for the 251 keV resonance.
Link to the paper.
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Thermonuclear reaction rate obtained using a method based on Monte Carlo techniques. Low rate, median rate and high rate correspond to the 0.16, 0.50 and 0.84 quantiles, respectively, of the cumulative reaction rate distribution.
Link to publication: Nuclear Physics A 841 (2010) 31–250
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