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Solar neutrinos and the MSW effect for three-neutrino mixingResearchers considered three-neutrino Mikheyev-Smirnov-Wolfenstein (MSW) mixing, assuming m sub 3 is much greater than m sub 2 is greater than m sub 1 as expected from theoretical consideration if neutrinos have mass. They calculated the corresponding mixing parameter space allowed by the Cl-37 and Kamiokande 2 experiments. They also calculated the expected depletion for the Ga-71 experiment. They explored a range of theoretical uncertainty due to possible astrophysical effects by varying the B-8 neutrino flux and redoing the MSW mixing calculation.
Document ID
19910021746
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Shi, X.
(Chicago Univ. Chicago, IL, United States)
Schramm, David N.
(Chicago Univ. Chicago, IL, United States)
Date Acquired
September 6, 2013
Publication Date
June 1, 1991
Subject Category
Solar Physics
Report/Patent Number
NAS 1.26:188706
NASA-CR-188706
FERMILAB-PUB-91/178-A
Accession Number
91N31060
Funding Number(s)
CONTRACT_GRANT: NAGW-1340
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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