Study of the 12C+12C fusion reactions near the Gamow energy

Phys.Rev.Lett.98:122501,2007 The fusion reactions 12C(12C,a)20Ne and 12C(12C,p)23Na have been studied from E = 2.10 to 4.75 MeV by gamma-ray spectroscopy using a C target with ultra-low hydrogen contamination. The deduced astrophysical S(E)* factor exhibits new resonances at E

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Hauptverfasser: Spillane, T, Raiola, F, Zeng, S, Becker, H. -W, Bordeanu, C, Gialanella, L, Rolfs, C, Romano, M, Sch"urmann, D, Schweitzer, J, Strieder, F
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Zusammenfassung:Phys.Rev.Lett.98:122501,2007 The fusion reactions 12C(12C,a)20Ne and 12C(12C,p)23Na have been studied from E = 2.10 to 4.75 MeV by gamma-ray spectroscopy using a C target with ultra-low hydrogen contamination. The deduced astrophysical S(E)* factor exhibits new resonances at E
DOI:10.48550/arxiv.nucl-ex/0702023