Study of the 18F(p,α)15O reaction at astrophysical energies using a 18F beam

Details Study of the 18F(p,α)15O reaction at astrophysical energies using a 18F beam Study of the 18F(p,α)15O reaction at astrophysical energies using a 18F beam

Aug 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995phrvc..52..460r&link_type=abstract

Physical Review C (Nuclear Physics), Volume 52, Issue 2, August 1995, pp.R460-R463

Physics

Nuclear Physics

32

Transfer Reactions, Transfer Reactions, Elementary Particle Processes

Scientific paper

For the first time the 18F(p,α)15O reaction has been studied with a 18F beam at energies which are of interest to explosive nucleosynthesis. Utilizing the gas-filled magnet technique a clean identification of the reaction products was achieved. A resonance with spin 3/2+ at an equivalent c.m. energy of 660 keV dominates the yield.

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