The F17(p,γ)Ne18 resonant cross section

Details The F17(p,γ)Ne18 resonant cross section The F17(p,γ)Ne18 resonant cross section

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009phrvc..80f5810c&link_type=abstract

Physical Review C, vol. 80, Issue 6, id. 065810

Physics

Nuclear Physics

Resonance Reactions, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, 6<=A<=19

Scientific paper

We directly measure the F17(p,γ)Ne18 resonant reaction using a mixed beam of F17 and O17 at the Holifield Radioactive Ion Beam Facility at Oak Ridge National Laboratory (ORNL). The astrophysically important 3+ resonance at ~600 keV above the proton threshold in Ne18 is found to have a partial width Γγ=56±24(stat)±30(sys) meV, in reasonable agreement with the theoretically predicted width. A 2σ upper limit on the direct capture of S(E)⩽65 keV b is determined at an energy of 800 keV. Experimental techniques and astrophysical implications are discussed.

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