13C(a,n)16O

13C(a,n)16O Ciani et al. 2021 This rate comes after the 13C(a,n)16O LUNA measurement, which is the first direct measurement reaching the high energy edge of the Gamow Window (130<E<240 keV). LUNA data cover the energy range 230<Ecm<305 keV corresponding to alpha energy 305<Ea<400 keV. All the points have overall uncertainty lower than 20%. The S… Continue reading 13C(a,n)16O

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22Ne(a,g)26Mg

22Ne(a,g)26Mg Adsley et al. 2021 A reevaluation of both 22Ne(a,n)25Mg and 22Ne(a,g)26Mg reaction rates using updated nuclear data from a number of sources, including the nuclear data from Ota et al. 2021and updating spin and parity assignments. Link to the publication: PHYSICAL REVIEW C 103, 015805 (2021) Wiescher et al. 2023 Evaluation of both 22Ne(a,n)25Mg and 22Ne(a,g)26Mg reaction rates… Continue reading 22Ne(a,g)26Mg

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22Ne(p,g)23Na

22Ne(p,g)23Na Iliadis et al. 2010 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 the publication: Nuclear Physics A 841 (2010) 31–250 Williams et al. 2020 This study… Continue reading 22Ne(p,g)23Na

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22Ne(a,n)25Mg

22Ne(a,n)25Mg Adsley et al. 2021 A reevaluation of both 22Ne(a,n)25Mg and 22Ne(a,g)26Mg reaction rates using updated nuclear data from a number of sources, including the nuclear data from Ota et al. 2021and updating spin and parity assignments. Link to the publication: PHYSICAL REVIEW C 103, 015805 (2021) Longland et al. 2012 Evaluation of both 22Ne(a,n)25Mg… Continue reading 22Ne(a,n)25Mg

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