Limits on sensitivity of large silicon bolometers for solar neutrino detection

Details Limits on sensitivity of large silicon bolometers for solar neutrino detection Limits on sensitivity of large silicon bolometers for solar neutrino detection

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sci...237..507m&link_type=abstract

Science (ISSN 0036-8075), vol. 237, July 31, 1987, p. 507-509. Research supported by the Research Corp.

Physics

15

Bolometers, Signal To Noise Ratios, Silicon Radiation Detectors, Solar Neutrinos, Background Noise, Cosmic Rays, Sensitivity, Single Crystals, Spallation

Scientific paper

Estimates are given for ultimate limits on background in proposed direct-counting measurements of neutrino scattering from large silicon crystals. Methods of background reduction are discussed. In the best case, the limiting backgrounds due to activities from cosmic-ray spallation of silicon would be less than the expected true event rate for reactor neutrino measurements of coherent neutral-current scattering from silicon nuclei. Considerable reduction of the estimated high-energy backgrounds would be required for a good signal-to-noise ratio in solar neutrino detection.

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