Nuclear physics and detection of solar neutrinos and dark matter

Details Nuclear physics and detection of solar neutrinos and dark matter Nuclear physics and detection of solar neutrinos and dark matter

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993nuphs..31..149v&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 31, p. 149-155.

Physics

Nuclear Physics

Scientific paper

Nuclear physics of a solar neutrino detector based on 127I is described first. It is shown that an iodine detector could be a relatively high-statistics 8B ve detector, and possibly an excellent detector of 7Be neutrinos. The nuclear physics issues of direct detection of neutralinos are discussed next. For light nuclei and/or relatively light neutralinos the nuclear structure aspects can be handled easily, and quite accurately. For heavier targets and heavier neutralinos, the momentum transfer dependence of the scalar and axial-vector structure functions must be evaluated. This is a nontrivial problem, particularly for the spin-dependent (axial-vector) scattering. Examples of different approaches are discussed.

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