In the nova temperature range, 0.1 GK < T < 0.4 GK, several low-energy resonances dominate the Ne-21(p,gamma)Na-22 reaction rate, which is currently affected by large uncertainties. We present a high-precision study of the resonances at E-r(lab) = 127.3, 271.4, 272.3, 291.5, and 352.6 keV, measured directly at the Laboratory for Underground Nuclear Astrophysics in Italy. The strengths of the 127.3-, 271.4-, and 291.5-keV resonances are consistent with previous measurements within 1 sigma. However, for the 272.3- and 352.6-keV resonances, we report strength values of (129.9 +/- 5.8) meV and (14.9 +/- 0.8) meV, respectively, more than a factor of 1.5 higher than literature values. In addition, we report on new branching ratios for the 127.3-, 272.3-, and 352.6-keV resonances, leading to updated decay schemes. Finally, we present a revised thermonuclear reaction rate and investigate its impact on the NeNa nucleosynthesis.

Improved direct measurement of low-energy resonances in the 21Ne(p, γ) 22Na reaction

Biasissi R.;Caciolli A.;Marigo P.;Piatti D.;Skowronski J.;Turkat S.;
2025

Abstract

In the nova temperature range, 0.1 GK < T < 0.4 GK, several low-energy resonances dominate the Ne-21(p,gamma)Na-22 reaction rate, which is currently affected by large uncertainties. We present a high-precision study of the resonances at E-r(lab) = 127.3, 271.4, 272.3, 291.5, and 352.6 keV, measured directly at the Laboratory for Underground Nuclear Astrophysics in Italy. The strengths of the 127.3-, 271.4-, and 291.5-keV resonances are consistent with previous measurements within 1 sigma. However, for the 272.3- and 352.6-keV resonances, we report strength values of (129.9 +/- 5.8) meV and (14.9 +/- 0.8) meV, respectively, more than a factor of 1.5 higher than literature values. In addition, we report on new branching ratios for the 127.3-, 272.3-, and 352.6-keV resonances, leading to updated decay schemes. Finally, we present a revised thermonuclear reaction rate and investigate its impact on the NeNa nucleosynthesis.
2025
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/3574381
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