Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003omeg.conf..130i&link_type=abstract
ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2000. Proceedings of the International Symposium. Held 19-21 January 2000 in Universi
Astronomy and Astrophysics
Astrophysics
Scientific paper
The Coulomb dissociation of 8B into 7Be and a proton was measured at E(8B) = 254 MeV/u. The astrophysical S17-factors for the 7Be(p,γ)8B reaction were extracted at Ecm = 0.25 - 2.78 MeV yielding the zero-energy S17-factor relevant to the solar neutrino problem to be S17(0) = 20.6 ± 1.2 ± 1.0 eV-b. Our results agree with the direct measurement results of Vaughn et al., Filippone et al., and Hammache et al. as well as the Coulomb dissociation results of Motobayashi et al. and Kikuchi et al. at E(8B) ≈ 50 MeV/u.
Baumann Thomas
Bertulani Carlos A.
Blank Basil
Boué François
Czajkowski S.
No associations
LandOfFree
Coulomb Dissociation of 8B at 254 MeV/u for 7Be(p,γ)8B 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 Coulomb Dissociation of 8B at 254 MeV/u for 7Be(p,γ)8B, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coulomb Dissociation of 8B at 254 MeV/u for 7Be(p,γ)8B will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1324847