Widths of astrophysically important resonances in 18Ne

Details Widths of astrophysically important resonances in 18Ne Widths of astrophysically important resonances in 18Ne

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002phrvc..65c5803h&link_type=abstract

Physical Review C, vol. 65, Issue 3, id. 035803

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17

Elastic Scattering, Transfer Reactions, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments

Scientific paper

The astrophysically important reaction 14O(α,p)17F has been studied through a measurement of the time-inverse p(17F,α)14O reaction using a radioactive 17F beam. Resonance parameters for several states above an excitation energy of 7 MeV in 18Ne have been obtained. Through a measurement of the partial widths for elastic and inelastic proton scattering, it was determined that for these resonances the contribution of the 14O(α,p)17F* branch populating the first excited state in 17F is small. The results indicate that the contribution of resonances above Ex=7 MeV to the astrophysical (α,p) reaction rate is smaller than was previously assumed.

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