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Phys. Rev. Lett. 89, 262501 (2002) [4 pages]

Strength of the 18F(p,α)15O Resonance at Ec.m.=330  keV

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D. W. Bardayan1, J. C. Batchelder2, J. C. Blackmon1, A. E. Champagne3, T. Davinson4, R. Fitzgerald3, W. R. Hix1,5,6, C. Iliadis3, R. L. Kozub7, Z. Ma5, S. Parete-Koon1,5, P. D. Parker8, N. Shu1,9, M. S. Smith1, and P. J. Woods4
1Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831
2UNIRIB, Oak Ridge Associated Universities, Oak Ridge, Tennessee 37831
3Department of Physics and Astronomy, University of North Carolina, Chapel Hill, North Carolina 27599
4Department of Physics and Astronomy, University of Edinburgh, Edinburgh EH9 3JZ, United Kingdom
5Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996
6Joint Institute for Heavy Ion Research, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831-6374
7Physics Department, Tennessee Technological University, Cookeville, Tennessee 38505
8A. W. Wright Nuclear Structure Laboratory, Yale University, New Haven, Connecticut 06520
9Chinese Institute for Atomic Energy, Beijing, 102413, People’s Republic of China

Received 1 July 2002; published 10 December 2002

Production of the radioisotope 18F in novae is severely constrained by the rate of the 18F(p,α)15O reaction. A resonance at Ec.m.=330   keV may strongly enhance the 18F(p,α)15O reaction rate, but its strength has been very uncertain. We have determined the strength of this important resonance by measuring the 18F(p,α)15O cross section on and off resonance using a radioactive 18F beam at the ORNL Holifield Radioactive Ion Beam Facility. We find that its resonance strength is 1.48±0.46  eV, and that it dominates the 18F(p,α)15O reaction rate over a significant range of temperatures characteristic of ONeMg novae.

© 2002 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.89.262501
DOI:
10.1103/PhysRevLett.89.262501
PACS:
27.20.+n, 25.60.Dz, 25.60.Je, 26.30.+k