Physics – Nuclear Physics – Nuclear Experiment
Scientific paper
2007-02-05
Phys.Rev.C75:035805,2007
Physics
Nuclear Physics
Nuclear Experiment
Accepted for publication in PRC
Scientific paper
10.1103/PhysRevC.75.035805
The flux of 7Be and 8B neutrinos from the Sun and the production of 7Li via primordial nucleosynthesis depend on the rate of the 3He(alpha,gamma)7Be reaction. In extension of a previous study showing cross section data at 127 - 167 keV center of mass energy, the present work reports on a measurement of the 3He(alpha,gamma)7Be cross section at 106 keV performed at Italy's Gran Sasso underground laboratory by the activation method. This energy is closer to the solar Gamow energy than ever reached before. The result is sigma = 0.567 +- 0.029(stat) +- 0.016(syst) nbarn. The data are compared with previous activation studies at high energy, and a recommended S(0) value for all 3He(alpha,gamma)7Be activation studies, including the present work, is given.
Alvarez Rossi C.
Bemmerer Daniel
Bonetti Roberto
Broggini Carlo
Confortola Fulvia
No associations
LandOfFree
3He(alpha,gamma)7Be cross section at low energies 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 3He(alpha,gamma)7Be cross section at low energies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and 3He(alpha,gamma)7Be cross section at low energies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-714512