The 22Ne(p,γ)23Na reaction is a part of the hydrogen burning NeNa cycle. In second-generation stars hydrogen burning may proceed via this cycle. The rate of the 22Ne(p,γ) 23Na reaction depends on the strength of several resonances in the energy range of the LUNA 400 kV accelerator which have never been observed in direct experiments. A related study is under preparation at LUNA.
Towards a Study of the Ne-22(p,gamma)Na-23 Reaction at LUNA / F. Cavanna, R. Depalo, M.-. Menzel (AIP CONFERENCE PROCEEDINGS). - In: EXOTIC NUCLEI AND NUCLEAR/PARTICLE ASTROPHYSICS (IV). FROM NUCLEI TO STARS: Carpathian Summer School of Physics 2012 / [a cura di] L. Trache, P.G. Isar. - [s.l] : AMER INST PHYSICS, 2012. - ISBN 978-0-7354-1112-8. - pp. 314-318 (( convegno Carpathian Summer School of Physics 2012: Exotic Nuclei and Nuclear/Particle Astrophysics (IV). From Nuclei to Stars, CSSP 2012 tenutosi a Sinaia nel 2012 [10.1063/1.4768510].
Towards a Study of the Ne-22(p,gamma)Na-23 Reaction at LUNA
R. DepaloSecondo
;
2012
Abstract
The 22Ne(p,γ)23Na reaction is a part of the hydrogen burning NeNa cycle. In second-generation stars hydrogen burning may proceed via this cycle. The rate of the 22Ne(p,γ) 23Na reaction depends on the strength of several resonances in the energy range of the LUNA 400 kV accelerator which have never been observed in direct experiments. A related study is under preparation at LUNA.
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