Published July 22, 1991
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Journal Article
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Response of 127I to solar neutrinos
- Creators
- Engel, J.
- Pittel, S.
- Vogel, P.
Abstract
We use a configuration-mixing quasiparticle Tamm-Dancoff approximation to calculate the expected event rate for an 127I solar neutrino detector. Our cross section for 8B solar neutrinos is 2.2×10-42 cm2 [corresponding to about 13 solar neutrino units (SNU) in the standard solar model], a factor of more than 3 below an estimate by Haxton. This value may increase by about 30% when quadrupole correlations are included. The cross section for ''Be neutrinos is 2.0×10-45 cm2 (9.4 SNU), in agreement with a calculation by Dellagiacoma and Iachello. The total event rate per nucleus from all solar neutrinos is about 3 times that in 37Cl.
Additional Information
©1991 The American Physical Society Received 11 January 1991 This work was supported in part by the National Science Foundation under Grant No. PHY-8901558 and the U.S. Department of Energy under Contract No. DE-F603-88ER-40397. The numerical calculations were carried out in part on the Cray Y-MP computer at the San Diego Supercomputer Center; its support is gratefully acknowledged.Files
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- Resolver ID
- CaltechAUTHORS:ENGprl91
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