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Implications of the GALLEX determination of the solar neutrino flux

✍ Scribed by P. Anselmann; W. Hampel; G. Heusser; J. Kiko; T. Kirsten; E. Pernicka; R. Plaga; U. Rönn; M. Sann; C. Schlosser; R. Wink; M. Wójcik; R. von Ammon; K.H. Ebert; E. Henrich; M. Balata; E. Bellotti; N. Ferrari; H. Lalla; T. Stolarczyk; C. Cattadori; O. Cremonesi; E. Fiorini; S. Pezzoni; L. Zanotti; F. von Feilitzsch; R. Mößbauer; U. Schanda; G. Berthomieu; E. Schatzman; I. Carmi; I. Dostrovsky; C. Bacci; P. Belli; R. Bernabei; S. d'Angelo; L. Paoluzi; S. Charbit; M. Cribier; G. Dupont; L. Gosset; J. Rich; M. Spiro; C. Tao; D. Vignaud; R.L. Hahn; F.X. Hartmann; J.K. Rowley; R.W. Stoenner; J. Weneser

Book ID
113361153
Publisher
Elsevier Science
Year
1992
Tongue
English
Weight
536 KB
Volume
285
Category
Article
ISSN
0370-2693

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Analyses of the Cl and Ga solar neutrino data yield statistically compelling evidence for rotational (and related) modulations of the solar neutrino flux. While a neutrino transition magnetic moment and the Resonant-Spin-Flavor-Precession (RSFP) process have given at least as good a fit to time-aver