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 in | Science (American Association for the Advancement of Science) Vol. 237; no. 4814; pp. 507 - 509 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
United States
The American Association for the Advancement of Science
31.07.1987
American Association for the Advancement of Science |
Subjects | |
Online Access | Get full text |
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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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Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 ObjectType-Article-1 ObjectType-Feature-2 |
ISSN: | 0036-8075 1095-9203 |
DOI: | 10.1126/science.237.4814.507 |