Journal
PHYSICS LETTERS B
Volume 579, Issue 3-4, Pages 265-270Publisher
ELSEVIER
DOI: 10.1016/j.physletb.2003.11.024
Keywords
Coulomb excitation; CNO cycle; radiative width; radioactive beam
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The radiative width of the 3/2(+) state at 6.793 MeV in O-15 has been experimentally determined to be Gammagamma = 0.95(-0.95)(+0.60) eV by intermediate-energy Coulomb excitation. Our result independently supports the recent studies which point to a minor contribution of this state to the astrophysical rate of the N-14(p,gamma)O-15 reaction in the CNO-cycle hydrogen burning in massive stars. (C) 2003 Elsevier B.V. All rights reserved.
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