Measurement of the strength of the ^18F(p,α)^15O resonance at E_c.m. = 330 keV

Details Measurement of the strength of the ^18F(p,α)^15O resonance at E_c.m. = 330 keV Measurement of the strength of the ^18F(p,α)^15O resonance at E_c.m. = 330 keV

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apr.x7013b&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

Knowledge of the astrophysical ^18F(p,α)^15O rate is important for understanding gamma-ray emission from novae and heavy-element production in x-ray bursts. A resonance at E_c.m.=330 keV in the ^18F(p,α)^15O reaction is believed to dominate the rate at nova temperatures. We report on the first precise determination of the strength of this important resonance. We measured the ^18F(p,α)^15O cross section on and off resonance using a radioactive ^18F beam at the ORNL Holifield Radioactive Ion Beam Facility and detecting the reaction products in the Silicon Detector Array (SIDAR). Our experimental method and results will be discussed.

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