Constraining the 12C+12C astrophysical S-factors with the 12C+13C measurements at very low energies

We use an underground counting lab with an extremely low background to perform an activity measurement for the C12+13C system with energies down to Ec.m.=2.323 MeV, at which the 12C(13C,p)24Na cross section is found to be 0.22(7) nb. The C12+13C fusion cross section is derived with a statistical mod...

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Principais autores:	N.T. Zhang, X.Y. Wang, D. Tudor, B. Bucher, I. Burducea, H. Chen, Z.J. Chen, D. Chesneanu, A.I. Chilug, L.R. Gasques, D.G. Ghita, C. Gomoiu, K. Hagino, S. Kubono, Y.J. Li, C.J. Lin, W.P. Lin, R. Margineanu, A. Pantelica, I.C. Stefanescu, M. Straticiuc, X.D. Tang, L. Trache, A.S. Umar, W.Y. Xin, S.W. Xu, Y. Xu
פורמט:	Artigo
שפה:	Inglês
יצא לאור:	Elsevier 2020-02-01
סדרה:	Physics Letters B
גישה מקוונת:	http://www.sciencedirect.com/science/article/pii/S0370269319308925
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