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sup 17 O( sup 3 He, d ) sup 18 F reaction and its implication in the sup 17 O destruction in the CNO cycle in stars

Journal Article · · Physical Review (Section) C: Nuclear Physics; (USA)
; ; ; ;  [1]; ; ;  [2]
  1. Centre de Spectrometrie Nucleaire et de Spectrometrie de Masse, 91405 Orsay, France (FR)
  2. Institut de Physique Nucleaire, 91406 Orsay, France (FR)
The proton stripping reaction {sup 17}O({sup 3}He,{ital d}){sup 18}F has been used to reinvestigate the proton widths of the states in {sup 18}F near the proton threshold. Distorted-wave angular distributions were calculated using appropriate methods for stripping to unbound states. The deduced proton width for the level at {ital E}{sub {ital x}}=5.673 MeV ({ital J}{sup {pi}}=1{sup {minus}}) is significantly larger than a previous value obtained from a direct radiative capture experiment. A subthreshold state at {ital E}{sub {ital x}}=5.603 MeV ({ital J}{sup {pi}}=1{sup +}) was found to have a rather large proton reduced width so that this state contributes significantly to the astrophysical {ital S} factor at low energy. These measurements lead to substantial changes in the stellar reaction rate for the {sup 17}O({ital p},{alpha}){sup 14}N reaction. This result is discussed in relation to recent observation of the isotopic abundance ratio {sup 16}O/{sup 17}O in red giant stars. In addition, the nuclear structure of {sup 18}F is studied via the measurement of spectroscopic factors for most of the levels in {sup 18}F bound against proton decay.
OSTI ID:
5003271
Journal Information:
Physical Review (Section) C: Nuclear Physics; (USA), Journal Name: Physical Review (Section) C: Nuclear Physics; (USA) Vol. 40:5; ISSN 0556-2813; ISSN PRVCA
Country of Publication:
United States
Language:
English

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