Asymptotic normalization coefficient from the 12C(7Li,6He)13N reaction and the astrophysical 12C(p,g)13N reaction rate

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dc.creatorLi, Z. H.
dc.creatorSu, J.
dc.creatorGuo, B.
dc.creatorLi, Z. C.
dc.creatorBai, X. X.
dc.creatorLiu, J. C.
dc.creatorLi, Y. J.
dc.creatorYan, S. Q.
dc.creatorWang, B. X.
dc.creatorWang, Y. B.
dc.creatorLian, G.
dc.creatorZeng, S.
dc.creatorLi, E. T.
dc.creatorFang, X.
dc.creatorLiu, W. P.
dc.creatorChen, Y. S.
dc.creatorShu, N. C.
dc.creatorFan, Q. W.
dc.date2009-05-11
dc.date.accessioned2026-07-07T13:13:37Z
dc.date.available2026-07-07T13:13:37Z
dc.descriptionAngular distribution of the 12C(7Li,6He)13N reaction at E(7Li) = 44.0 MeV was measured at the HI-13 tandem accelerator of Beijing, China. Asymptotic normalization coefficient (ANC) of 13N = 12C + p was derived to be 1.64 $\pm$ 0.11 fm$^{-1/2}$ through distorted wave Born approximation (DWBA) analysis. The ANC was then used to deduce the astrophysical $S(E)$ factors and reaction rates for direct capture in 12C(p,g)13N at energies of astrophysical relevance.
dc.description13 pages, 4 figues, submitted to Nucl. Phys. A
dc.identifierhttps://arxiv.org/abs/0905.1530
dc.identifierhttp://arxiv.org/abs/0905.1530
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229950
dc.subjectNuclear Experiment
dc.titleAsymptotic normalization coefficient from the 12C(7Li,6He)13N reaction and the astrophysical 12C(p,g)13N reaction rate
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