Direct capture cross section and the = 71 and 105 keV resonances in the Ne()Na reaction
F. Ferraro🇮🇹 · M. P. Takács🇩🇪 · D. Piatti🇮🇹 · F. Cavanna🇮🇹 · R. Depalo🇮🇹 · M. Aliotta · D. Bemmerer🇩🇪 · A. Best🇮🇹 · A. Boeltzig🇮🇹 · C. Broggini🇮🇹 · C. G. Bruno🇬🇧 · A. Caciolli🇮🇹 and 32 other authors
The Ne()Na reaction, part of the neon-sodium cycle of hydrogen burning, may explain the observed anticorrelation between sodium and oxygen abundances in globular cluster stars. Its rate is controlled by a number of low-energy resonances and a slowly varying non-resonant component. Three new resonances at = 156.2, 189.5, and 259.7 keV have recently been observed and confirmed. However, significant uncertainty on the reaction rate remains due to the non-resonant process and to two suggested resonances at = 71 and 105 keV. Here, new Ne()Na data with high statistics and low background are reported. Stringent upper limits of 610 and 710\,eV (90\% confidence level), respectively, are placed on the two suggested resonances. In addition, the off-resonant S-factor has been measured at unprecedented low energy, constraining the contributions from a subthreshold resonance and the direct capture process. As a result, at a temperature of 0.1 GK the error bar of the Ne()Na rate is now reduced by three orders of magnitude.