Astrophysical reaction rate for the 18F(p,α)15O reaction

Details Astrophysical reaction rate for the 18F(p,α)15O reaction Astrophysical reaction rate for the 18F(p,α)15O reaction

Apr 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvc..53.1950r&link_type=abstract

Physical Review C (Nuclear Physics), Volume 53, Issue 4, April 1996, pp.1950-1954

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33

Transfer Reactions, Resonances, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, 6<=A<=19

Scientific paper

An excitation function for the 18F(p,α)15O reaction has been measured in the energy range Ec.m.=600-800 keV using a radioactive 18F beam. A resonant state with a spin value of 3/2+ has been found at an energy of 652 keV above threshold. This lp=0 resonance is found to dominate the astrophysical reaction rate at temperatures T9>~0.5.

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