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[en] The analysis described in this paper, made on the bases of two a priori assumptions derived from the results of the authors' work, shows that the Kamioka data support the previously found correlation between the g.w. data and the Mont Blanc data. The probability that this support be accidental is of the order of 3.3 x 10-4 or 4.7 x 10-4 and, in all cases, it is smaller than 5.1 x 10-3. To this, it should be added the fact that the Kamioka contribution is due to events concentrated near the 5νMont Blanc event
Source
Fenyves, E.J. (Dept. of Physics, Univ. of Texas at Dallas, Richardson, TX (USA)); Annals of the New York Academy of Sciences; 698 p; ISBN 0-89766-526-0; 
; 1989; p. 561-576; The New York Academy of Sciences; New York, NY (USA); 14. Texas symposium on relativistic astrophysics; Dallas, TX (USA); 11-16 Dec 1988; CONF-881268--; The New York Academy of Sciences, 2 East 63 St., New York, NY 10021 (USA)
; 1989; p. 561-576; The New York Academy of Sciences; New York, NY (USA); 14. Texas symposium on relativistic astrophysics; Dallas, TX (USA); 11-16 Dec 1988; CONF-881268--; The New York Academy of Sciences, 2 East 63 St., New York, NY 10021 (USA)