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The hot CNO cycle'' [sup 13]N([ital p],[gamma]) resonance energy and the [sup 18]Ne mass

Journal Article · · Physical Review, C (Nuclear Physics); (United States)
;  [1];  [2]
  1. Nuclear Physics Laboratory GL-10, University of Washington, Seattle, Washington 98195 (United States)
  2. Lawrence Berkeley Laboratory, Berkeley, California 94720 (United States)
The masses of [sup 18]Ne, and of the [sup 14]O first excited state that dominates the astrophysical [sup 13]N([ital p],[gamma]) reaction rate, were measured using the [sup 16]O([sup 3]He,[ital n]) and [sup 12]C([sup 3]He,[ital n]) reactions. We found mass excesses of 5316.8[plus minus]1.5 keV for the [sup 18]Ne ground state and 13163.4[plus minus]2.0 keV for the first excited state of [sup 14]O. The [sup 14]O mass corresponds to an [sup 13]N([ital p],[gamma]) resonance energy of 528.8[plus minus]2.0 keV. This is consistent with the result from a recent [sup 13]N+[ital p] study, but disagrees with the previously accepted value. Implications for the thermonuclear [sup 13]N([ital p],[gamma]) rate are discussed.
OSTI ID:
5016858
Journal Information:
Physical Review, C (Nuclear Physics); (United States), Journal Name: Physical Review, C (Nuclear Physics); (United States) Vol. 49:4; ISSN 0556-2813; ISSN PRVCAN
Country of Publication:
United States
Language:
English