First measurement of the low-energy direct capture in 20Ne(p, {\gamma})21Na and improved energy and strength of the Ecm = 368 keV resonance
E. Masha🇩🇪 · L. Barbieri · J. Skowronski🇮🇹 · M. Aliotta🇬🇧 · C. Ananna🇮🇹 · F. Barile · D. Bemmerer🇩🇪 · A. Best🇮🇹 · A. Boeltzig🇮🇹 · C. Broggini🇮🇹 · C.G. Bruno🇬🇧 · A. Caciolli🇮🇹 and 39 other authors
The reaction is the slowest in the NeNa cycle and directly affects the abundances of the Ne and Na isotopes in a variety of astrophysical sites. Here we report the measurement of its direct capture contribution, for the first time below ~keV, and of the contribution from the ~keV resonance, which dominates the reaction rate at ~GK. The experiment was performed deep underground at the Laboratory for Underground Nuclear Astrophysics, using a high-intensity proton beam and a windowless neon gas target. Prompt rays from the reaction were detected with two high-purity germanium detectors. We obtain a resonance strength ~meV, with an uncertainty a factor of smaller than previous values. Our revised reaction rate is 20\% lower than previously adopted at ~GK and agrees with previous estimates at temperatures ~GK. Initial astrophysical implications are presented.