Phys. Rev. C 66, 048801 (2002) [4 pages]Indirect study of the astrophysically important 15O(α,γ)19Ne reaction through 2H(18Ne,19Ne)1HReceived 3 July 2002; published 29 October 2002 The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO cycle. Under nova conditions, the reaction rate is dominated by a single sub-Coulomb resonance at Ec.m.=504keV which corresponds to a 19Ne excitation energy of ER=4.033MeV. Results from a d(18Ne,19Ne)p experiment show that states of astrophysical interest are populated in this reaction. An upper limit for the α-branching ratio of the 4.033 MeV state was identified and branching ratios for other states in 19Ne were found to be in good agreement with stable beam based results. © 2002 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevC.66.048801
DOI:
10.1103/PhysRevC.66.048801
PACS:
25.60.Je, 26.30.+k
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