Correlations among gravitational wave and neutrino detector data during SN 1987A.

Details Correlations among gravitational wave and neutrino detector data during SN 1987A. Correlations among gravitational wave and neutrino detector data during SN 1987A.

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ncimb.105..993p&link_type=abstract

Nuovo Cimento B, Vol. 105, No. 8/9, p. 993 - 1007

Mathematics

Probability

Supernova 1987A In Lmc, Neutrinos: Supernovae, Neutrinos: Gravitational Radiation

Scientific paper

The data recorded with the neutrino detectors at Mont Blanc, Kamioka, Baksan and with the graviational wave detectors at Maryland and Rome have been analysed during the period of SN 1987A without presuming nor excluding that they are really due to neutrions and to gravitational waves (g.w.). Correlations are found during a period of one or two hours roughly centred at 2:45 hour U.T. of 23 February 1987. The strongest correlations are between g.w. and Mont Blanc with a probability to be accidental of about p ≍ 10-5, g.w. and Kamioka with p ≍ 10-3, and Mont Blanc and Baksan with p ≍ 4×10-3. All "neutrino" signals follow the g.w. signals by a time of the order of 1 second. The basic physical problems connected with these correlations are indicated but no physical explanation of the observed phenomenon is proposed.

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