Publication Date:
2012-11-06
Description:
Author(s): U. Hager, L. Buchmann, B. Davids, J. Fallis, U. Greife, D. A. Hutcheon, D. Irvine, D. Ottewell, A. Rojas, S. Reeve, and C. Ruiz In stars, 16 O represents the endpoint of the helium burning sequence due to the low rate of 16 O( α , γ ) 20 Ne. We present a new direct measurement of the total cross section of 16 O( α , γ ) 20 Ne at E c.m. =1.69 MeV employing the DRAGON recoil separator. In addition, the branching ratios and strength of the E c.m... [Phys. Rev. C 86, 055802] Published Mon Nov 05, 2012
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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