Engel, J. and Pittel, S. and Vogel, P. (1991) Response of 127I to solar neutrinos. Physical Review Letters, 67 (4). pp. 426-429. ISSN 0031-9007. doi:10.1103/PhysRevLett.67.426. https://resolver.caltech.edu/CaltechAUTHORS:ENGprl91
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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.
| Item Type: | Article | ||||||
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| 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. | ||||||
| Issue or Number: | 4 | ||||||
| DOI: | 10.1103/PhysRevLett.67.426 | ||||||
| Record Number: | CaltechAUTHORS:ENGprl91 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:ENGprl91 | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 3579 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Archive Administrator | ||||||
| Deposited On: | 16 Jun 2006 | ||||||
| Last Modified: | 08 Nov 2021 19:57 |
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