Publication Date:
2015-04-17
Description:
Author(s): M. L. Avila, G. V. Rogachev, E. Koshchiy, L. T. Baby, J. Belarge, K. W. Kemper, A. N. Kuchera, and D. Santiago-Gonzalez Background: Accurate knowledge of the 13 C(α,n) 16 O reaction cross section is important for the understanding of the s process in asymptotic giant branch stars, since it is considered to be the main source of neutrons. The subthreshold 1/2 + state at excitation energy of 6.356 MeV in 17 O has a strong i... [Phys. Rev. C 91, 048801] Published Thu Apr 16, 2015
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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