Feasibility of a Br-81(nu, e/-/)Kr-81 solar neutrino experiment

Details Feasibility of a Br-81(nu, e/-/)Kr-81 solar neutrino experiment Feasibility of a Br-81(nu, e/-/)Kr-81 solar neutrino experiment

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phrvl..53.1116h&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 53, Sept. 10, 1984, p. 1116-1119.

Physics

28

Bromine Isotopes, Krypton Isotopes, Mass Spectroscopy, Solar Neutrinos, Capture Effect, Feasibility Analysis, Nuclear Reactions, Solar Interior, Solar Physics, Stellar Models

Scientific paper

A solar neutrino experiment utilizing the interaction of Br-81(nu, e/-/)Kr-81 to study the Be-7 neutrino source in the interior of the sun is shown to be feasible. Resonance ionization spectroscopy was used to count less than 1000 atoms of 200,000-yr Kr-81, making the bromine experiment possible. Except for the method of counting product atoms, the bromine experiment would be very similar to the successful chlorine detector C2-37(nu, e/-/)Ar-37, and thus it is a natural sequel to the only solar neutrino experiment to date.

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