https://doi.org/10.1140/epja/i2014-14179-5
Regular Article - Experimental Physics
A new study of the 22Ne(p, γ)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance
1
Dipartimento di Fisica, Università di Genova, and INFN, Sezione di Genova, Genova, Italy
2
Sezione di Padova, INFN, Padova, Italy
3
Dipartimento di Fisica e Astronomia, Università di Padova, Padova, Italy
4
Helmholtz-Zentrum Dresden-Rossendorf (HZDR), Dresden, Germany
5
Technische Universität Dresden, Dresden, Germany
6
SUPA, School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
7
Dipartimento di Fisica, Università degli Studi di Napoli Federico II, and INFN, Sezione di Napoli, Napoli, Italy
8
Institute of Nuclear Research of the Hungarian Academy of Sciences (MTA ATOMKI), Debrecen, Hungary
9
Laboratori Nazionali del Gran Sasso, INFN, Assergi, Italy
10
Dipartimento di Fisica Sperimentale, Università di Torino, and INFN, Sezione di Torino, Torino, Italy
11
Università degli Studi di Milano, and INFN, Sezione di Milano, Milano, Italy
12
Sezione di Roma “La Sapienza”, INFN, Roma, Italy
13
Osservatorio Astronomico di Collurania, Teramo, Italy
15
Sezione di Napoli, INFN, Napoli, Italy
14
Ruhr-Universität Bochum, Bochum, Germany
* e-mail: d.bemmerer@hzdr.de
Received:
2
August
2014
Revised:
4
November
2014
Accepted:
11
November
2014
Published online:
27
November
2014
The 22Ne(p,γ)23Na 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 22Ne(p,γ)23Na cross section directly at the astrophysically relevant energies are needed. In the present work, a feasibility study for a 22Ne(p,γ)23Na 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 γ-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 × 10−6 eV has been obtained for the resonance strength. Informed by the feasibility study, a dedicated experimental setup for the 22Ne(p,γ)23Na 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.
© SIF, Springer-Verlag Berlin Heidelberg, 2014