Measurement of the 17 O(p,γ)18F reaction rate at astrophysically relevant energies

Details Measurement of the 17 O(p,γ)18F reaction rate at astrophysically relevant energies Measurement of the 17 O(p,γ)18F reaction rate at astrophysically relevant energies

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012phrvc..85c5803h&link_type=abstract

Physical Review C, vol. 85, Issue 3, id. 035803

Physics

Nuclear Physics

Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, Origin, Formation, And Abundances Of The Elements, Direct Reactions

Scientific paper

The 17O(p,γ)18F reaction plays an important role in hydrogen-burning nucleosynthesis. Conflicting values for the low-energy behavior of its cross section exist in the literature. We present direct measurements of the astrophysical S factor of the 17O(p,γ)18F reaction at center-of-mass energies between 250 and 500 keV. These measurements were conducted in inverse kinematics at the DRAGON recoil separator.

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