Phys. Rev. C 57, 2731 - 2739 (1998)Breakout from the hot CNO cycle: The 18F(p,γ) vs 18F(p,α) branching ratio
S. Utku1 *, J. G. Ross2 †, N. P. T. Bateman1 ‡, D. W. Bardayan1, A. A. Chen1, J. Görres2, A. J. Howard3, C. Iliadis2 §, P. D. Parker1, M. S. Smith4, R. B. Vogelaar5, M. Wiescher2, and K. Yildiz1 See Also: Erratum Received 30 October 1997 We have studied the properties of low-lying 18F+p resonances as excited states in 19Ne. Three new levels have been found in the range 0<~Ec.m.<~1 MeV just above the 18F+p threshold, and partial decay widths and isospin-mirror connections are suggested to known states in 19F for each of the nine states in this energy range. The properties of these resonances have been used to calculate the reaction rate NA〈σv〉 for the 18F(p,γ)19Ne and 18F(p,α)15O reactions in the temperature range 108<T<109. A comparison of these rates indicates that in this temperature range, the 14O(α,p)17F(p,γ)18Ne(e+ν)18F(p,γ)19Ne reaction sequence is not as fast as the 15O(α,γ)19Ne reaction. ©1998 The American Physical Society
URL: http://link.aps.org/doi/10.1103/PhysRevC.57.2731
* Present address: Columbia University Law School, Columbia University, New York, NY 10027.
See AlsoErratum: S. Utku, J. G. Ross, N. P. Bateman, D. W. Bardayan, A. A. Chen, J. Görres, A. J. Howard, C. Iliadis, P. D. Parker, M. S. Smith, R. B. Vogelaar, M. Wiescher, and K. Yildiz, Erratum: Breakout from the hot CNO cycle: The 18F(p,γ) vs 18F(p,α) branching ratio [Phys. Rev. C 57, 2731 (1998)], Phys. Rev. C 58, 1354 (1998) [ Abstract | Previous article | Next article | Issue 5 ] |
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