Response of I-127 to solar neutrinos

Details Response of I-127 to solar neutrinos Response of I-127 to solar neutrinos

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvl..67..426e&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 67, July 22, 1991, p. 426-429.

Physics

18

Configuration Interaction, Iodine, Radiation Counters, Solar Neutrinos, Beryllium Isotopes, Boron Isotopes, Cross Sections

Scientific paper

Haxton (1988) proposed the use of I-127 as the active element in s a solar neutrino detector, and estimated the cross section of B-8 neutrinos on I-127 to be between 7.2 x 10 to the -42nd and 8.9 x 10 to the -42nd sq cm, considerably larger value than the cross section on Cl-37. Here, a configuration-mixing quasi-particle Tamm-Dancoff approximation is used to calculate the expected event rate for an I-127 solar neutrino detector. The resulting cross section for B-8 solar neutrinos is 2.2 x 10 to the -42nd sq cm. Furthermore, the Be-7 cross section is so large that the Be-7/Be-8 ratio is very different from that in Cl-37.

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