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AbstractAbstract
[en] We have measured the cross section for radiative capture of thermal neutrons on 3He. The measured cross section of 54±6 μb is used to estimate the astrophysical S factor for the reaction 3He(p,e+ν)4He which gives rise to high-energy neutrinos from the Sun
Primary Subject
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Journal Article
Literature Type
Numerical Data
Journal
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BARYON REACTIONS, BOSONS, DATA, ELEMENTARY PARTICLES, ENERGY RANGE, EVEN-EVEN NUCLEI, FERMIONS, HADRON REACTIONS, HELIUM ISOTOPES, INFORMATION, ISOTOPES, LEPTONS, LIGHT NUCLEI, MASSLESS PARTICLES, MEV RANGE, NUCLEAR REACTIONS, NUCLEI, NUCLEON REACTIONS, NUMERICAL DATA, PARTIAL WAVES, SPECTRA, STABLE ISOTOPES, TARGETS
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