Phys. Rev. C 62, 055804 (2000) [14 pages]The astrophysically important 3+ state in 18Ne and the 17F(p,γ)18Ne stellar rateReceived 19 June 2000; published 19 October 2000 Knowledge of the 17F(p,γ)18Ne reaction rate is important for understanding stellar explosions, but it was uncertain because the properties of an expected but previously unobserved 3+ state in 18Ne were not known. This state would provide a strong s-wave resonance for the 17F+p system and, depending on its excitation energy, could dominate the stellar reaction rate at temperatures above 0.2 GK. We have observed this missing 3+ state by measuring the 1H(17F,p)17F excitation function with a radioactive 17F beam at the ORNL Holifield Radioactive Ion Beam Facility (HRIBF). We find that the state lies at a center-of-mass energy of Er=599.8±1.5stat±2.0sys keV (Ex=4523.7±2.9keV) and has a width of Γ=18±2stat±1syskeV. The measured properties of the resonance are only consistent with a Jπ=3+ assignment. © 2000 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevC.62.055804
DOI:
10.1103/PhysRevC.62.055804
PACS:
26.30.+k, 25.40.Cm, 25.60.Bx, 27.20.+n
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