The Astrophysical S-factor and Cross-Section for the ^9Be(p,γ)^10B reaction.

Details The Astrophysical S-factor and Cross-Section for the ^9Be(p,γ)^10B reaction. The Astrophysical S-factor and Cross-Section for the ^9Be(p,γ)^10B reaction.

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..osfdo1003w&link_type=abstract

American Physical Society, Ohio Section Fall Meeting, October 13-14, 2000 Toledo, OH, abstract #DO1.003

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have studied the ^9Be(p,γ)^10B reaction for proton bombarding energies from 35 keV to 150 keV and obtained the cross section and astrophysical S-factor. We have detected the gamma rays produced from this capture reaction in a high purity, germanium detector. A maximum of 0.80 mA of proton beam current was used on a water cooled target (natural beryllium) and the detector front face was kept within 2 cm from the target. The astrophysical significance of the results obtained will be discussed.

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