ABSTRACT

A solar neutrino experiment utilizing the interaction of 81Br(v,e )81Kr to study the 7Be 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 2 × 105-yr 81Kr, 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 37Cl(v,e )37Ar, and thus it is a natural sequel to the only solar neutrino experiment to date.