Accurate energy determination of the 5673-keV state in 18F and implications in the 17O nucleosynthesis

Details Accurate energy determination of the 5673-keV state in 18F and implications in the 17O nucleosynthesis Accurate energy determination of the 5673-keV state in 18F and implications in the 17O nucleosynthesis

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvc..39..265b&link_type=abstract

Physical Review C (Nuclear Physics), Volume 39, Issue 1, January 1989, pp.265-268

Physics

Nuclear Physics

8

3H-, 3He-, And 4He-Induced Reactions, 6<=A<=19, Abundances, Chemical Composition

Scientific paper

The energy of the first level above the proton threshold in 18F has been determined to be 5672.57+/-0.32 keV by γ-ray measurements using the 14N(α,γ)18F reaction. The change in the excitation energy of this level previously measured at 5668+/-2 keV affects significantly the calculated reaction rate for 17O destruction during hydrogen burning in stars.

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