Physics – Nuclear Physics
Scientific paper
Oct 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phrvc..58.2174k&link_type=abstract
Physical Review C (Nuclear Physics), Volume 58, Issue 4, October 1998, pp.2174-2179
Physics
Nuclear Physics
6
Inelastic Proton Scattering, Angular Distribution And Correlation Measurements, Cosmic Ray Nucleosynthesis
Scientific paper
Excitation functions for the production of the 2.74, 6.13, 6.92, and 7.12 MeV γ rays by inelastic proton scattering on 16O have been measured in steps of 200-500 keV for proton energies Ep=8.4-20 MeV. For the 4.44 MeV γ rays of 12C produced by inelastic proton scattering on 12C data have been obtained for proton energies Ep=8.4-14 MeV and at Ep=17.25, 18.25, and 19.75 MeV. Eight high efficiency Ge detectors with anti-Compton shielding for the γ-ray detection were used to obtain the laboratory γ-angular distributions. The results of Legendre polynom fits to these distributions are discussed and presented in suitable form for use in γ-ray astronomy.
Achouri N. L.
Berheide M.
Boughrara A.
Coc Alain
de Oliveira Santos F.
No associations
LandOfFree
γ-ray production by inelastic proton scattering on 16O and 12C does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with γ-ray production by inelastic proton scattering on 16O and 12C, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and γ-ray production by inelastic proton scattering on 16O and 12C will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1100668