Publication Date:
2017-10-28
Description:
Author(s): S. A. Kuvin, J. Belarge, L. T. Baby, J. Baker, I. Wiedenhöver, P. Höflich, A. Volya, J. C. Blackmon, C. M. Deibel, H. E. Gardiner, J. Lai, L. E. Linhardt, K. T. Macon, B. C. Rasco, N. Quails, K. Colbert, D. L. Gay, and N. Keeley Background: The F 17 ( p , γ ) Ne 18 reaction is part of the astrophysical “hot CNO” cycles that are important in astrophysical environments like novas. Its thermal reaction rate is low owing to the relatively high energy of the resonances and therefore is dominated by direct, nonresonant capture in stellar... [Phys. Rev. C 96, 045812] Published Fri Oct 27, 2017
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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