A new study of the 22Ne(p, γ)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance

LUNA Collaboration, F. Cavanna, R. Depalo, M-L Menzel, M. Aliotta, M. Anders, D. Bemmerer*, C. Broggini, C. G. Bruno, A. Caciolli, P. Corvisiero, T. Davinson, A. di Leva, Z. Elekes, F. Ferraro, A. Formicola, Zs. Fueloep, G. Gervino, A. Guglielmetti, C. GustavinoGy. Gyuerky, G. Imbriani, M. Junker, R. Menegazzo, P. Prati, C. Rossi Alvarez, D. A. Scott, E. Somorjai, O. Straniero, F. Strieder, T. Szuecs, D. Trezzi

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

The Ne-22(p, gamma)Na-23 reaction takes part in the neon-sodium cycle of hydrogen burning. This cycle is active in asymptotic giant branch stars as well as in novae and contributes to the nucleosythesis of neon and sodium isotopes. In order to reduce the uncertainties in the predicted nucleosynthesis yields, new experimental efforts to measure the Ne-22(p, gamma)Na-23 cross section directly at the astrophysically relevant energies are needed. In the present work, a feasibility study for a Ne-22(p, gamma)Na-23 experiment at the Laboratory for Underground Nuclear Astrophysics (LUNA) 400 kV accelerator deep underground in the Gran Sasso laboratory, Italy, is reported. The ion-beam-induced.-ray background has been studied. The feasibility study led to the first observation of the E-p = 186 keV resonance in a direct experiment. An experimental lower limit of 0.12 x 10(-6) eV has been obtained for the resonance strength. Informed by the feasibility study, a dedicated experimental setup for the Ne-22(p, gamma)Na-23 experiment has been developed. The new setup has been characterized by a study of the temperature and pressure profiles. The beam heating effect that reduces the effective neon gas density due to the heating by the incident proton beam has been studied using the resonance scan technique, and the size of this effect has been determined for a neon gas target.

Original languageEnglish
Article number179
Number of pages10
JournalEuropean Physical Journal A: Hadrons and Nuclei
Volume50
Issue number11
DOIs
Publication statusPublished - 27 Nov 2014

Keywords

  • THERMONUCLEAR REACTION-RATES
  • LOW-ENERGY RESONANCES
  • NUCLEAR ASTROPHYSICS
  • NOVA NUCLEOSYNTHESIS
  • GAS-TARGET
  • AGB STARS
  • LUNA
  • CAPTURE
  • BEAM
  • ACCELERATOR

Fingerprint Dive into the research topics of 'A new study of the 22Ne(p, γ)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance'. Together they form a unique fingerprint.

Cite this