Astrophysical SE2 factor of the 12C(α, γ)16O reaction through the 12C(11B, 7Li)16O transfer reaction

Astrophysical SE2 factor of the 12C(α, γ)16O reaction through the 12C(11B, 7Li)16O transfer reaction

The 12C(α, γ)16O reaction plays a key role in the evolution of stars with masses of M > 0.55 M⊙. At the Gamow peak (Ec.m. = 300 ke V, T9 = 0.2), the cross section of the 12C(α, γ)16O reaction is so small (about 10−17 barn) that the direct measurement in ground laboratory is not feasible with the...

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Bibliographic Details
Main Authors: Guo B., Du X.C., Li Z.H., Li Y.J., Pang D.Y., Su J., Yan S.Q., Fan Q.W., Gan L., Han Z.Y., Li E.T., Li X.Y., Lian G., Liu J.C., Pei C.J., Qiao L.H., Shen Y.P., Su Y., Wang Y.B., Zeng S., Zhou Y., Liu W.P.
Format: Article
Language:English
Published: EDP Sciences 2016-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201610904003

Internet

http://dx.doi.org/10.1051/epjconf/201610904003

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