Detection of low energy solar neutrinos with HPGermanium

Details Detection of low energy solar neutrinos with HPGermanium Detection of low energy solar neutrinos with HPGermanium

1999-06-30

arxiv.org/abs/hep-ex/9906044v1

Eur.Phys.J. A5 (1999) 441-443

Physics

High Energy Physics

High Energy Physics - Experiment

5 pages (latex) including 1 postscript figure and one table. to appear in Eur. Phys. J. A

Scientific paper

10.1007/s100500050307

The potential of the GENIUS proposal to measure the spectrum of low energy solar neutrinos in real time is studied. The detection reaction is elastic neutrino-electron scattering. The energy resolution for detecting the recoil electrons is about 0.3 %, the energy threshold is a few keV. The expected number of events for a target of one ton of natural germanium is 3.6 events/day for pp-neutrinos and 1.3 events/day for 7Be-neutrinos, calculated in the standard solar model (BP98). It should be feasible to achieve a background low enough to measure the low energy solar neutrino spectrum.

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