Limits on Sensitivity of Large Silicon Bolometers for Solar Neutrino Detection

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 b...

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Published inScience (American Association for the Advancement of Science) Vol. 237; no. 4814; pp. 507 - 509
Main Author Martoff, C. J.
Format Journal Article
LanguageEnglish
Published United States The American Association for the Advancement of Science 31.07.1987
American Association for the Advancement of Science
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Summary: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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ISSN:0036-8075
1095-9203
DOI:10.1126/science.237.4814.507