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Solar models, neutrino experiments, and helioseismologyThe event rates and their recognized uncertainties are calculated for 11 solar neutrino experiments using accurate solar models. These models are also used to evaluate the frequency spectrum of the p and g oscillations modes of the sun. It is shown that the discrepancy between the predicted and observed event rates in the Cl-37 and Kamiokande II experiments cannot be explained by a 'likely' fluctuation in input parameters with the best estimates and uncertainties given in the present study. It is suggested that, whatever the correct solution to the solar neutrino problem, it is unlikely to be a 'trival' error.
Document ID
19880059023
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bahcall, John N.
(Institute for Advanced Study Princeton, NJ, United States)
Ulrich, Roger K.
(California, University Los Angeles, United States)
Date Acquired
August 13, 2013
Publication Date
April 1, 1988
Publication Information
Publication: Reviews of Modern Physics
Volume: 60
ISSN: 0034-6861
Subject Category
Solar Physics
Accession Number
88A46250
Funding Number(s)
CONTRACT_GRANT: NAGW-472
CONTRACT_GRANT: NSF PHY-82-17352
Distribution Limits
Public
Copyright
Other

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