Is bi-maximal mixing compatible with the large angle MSW solution of the
  solar neutrino problem?

A.J. Baltz; B.T. Cleveland; C. Caso; C. Giunti; G. Altarelli; H. Fritzsch; H. Fritzsch; J.N. Abdurashitov; J.N. Bahcall; J.N. Bahcall; K.S. Kang; L. Wolfenstein; L. Wolfenstein; N. Haba; R. Becker-Szendy; S.M. Bilenky; S.M. Bilenky; S.M. Bilenky; S.P. Mikheyev; S.P. Mikheyev; T.K. Kuo; V. Barger; W. Hampel; W.W.M. Allison; Y. Fukuda; Y. Fukuda; Y. Fukuda; Y. Nomura

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Is bi-maximal mixing compatible with the large angle MSW solution of the solar neutrino problem?

Authors: A.J. Baltz
B.T. Cleveland
C. Caso
C. Giunti
G. Altarelli
H. Fritzsch
H. Fritzsch
J.N. Abdurashitov
J.N. Bahcall
J.N. Bahcall
K.S. Kang
L. Wolfenstein
L. Wolfenstein
N. Haba
R. Becker-Szendy
S.M. Bilenky
S.M. Bilenky
S.M. Bilenky
S.P. Mikheyev
S.P. Mikheyev
T.K. Kuo
V. Barger
W. Hampel
W.W.M. Allison
Y. Fukuda
Y. Fukuda
Y. Fukuda
Y. Nomura
Publication date: 7 October 1998
Publisher: 'American Physical Society (APS)'
Doi

Abstract

It is shown that the large angle MSW solution of the solar neutrino problem with a bi-maximal neutrino mixing matrix implies an energy-independent suppression of the solar nu_e flux. The present solar neutrino data exclude this solution of the solar neutrino problem at 99.6% CL.Comment: 6 pages. No figure

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