2000/11/20 by M. Hussonois, Hussonois, M., L. Brillard +3
Physics and Astronomy · #FOS: Physical sciences #Gamma-ray bursts and supernovae #Nuclear Experiment (nucl-ex) #Nuclear Physics and Applications #Nuclear physics research studies #nucl-ex
paper · pdf · doi:10.48550/arxiv.nucl-ex/0011014
5 pages, 1 figure
arxiv created 2000/11/20 · openalex publication_date 2000/11/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The interpretation of the most recent solar neutrinos experiments requires a good knowledge of the cross section of the reaction 7Be(p,gamma)8B at very small energy (Ecm=18 keV). We have recently measured this cross section for Ecm=0.35-1.4 MeV and for Ecm=0.112-0.190 MeV. We report here on the description of the preparation of the radioactive targets of 7Be used in these experiments.