Correlation between gravitational-wave detectors and particle detectors during SN1987A

Details Correlation between gravitational-wave detectors and particle detectors during SN1987A Correlation between gravitational-wave detectors and particle detectors during SN1987A

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ncimc..15..931p&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 15 C, no. 6, p. 931-941.

Physics

2

Gravitational Waves, Neutrinos, Radiation Detectors, Statistical Analysis, Supernova 1987A, Algorithms, Correlation, Data Processing, Photoelectrons

Scientific paper

A correlation is established between the data recorded during the supernova SN1987A by the gravitational wave antennas of Maryland and Rome and by the neutrino detectors of Mont Blanc, Kamioka, IMB, and Baksan. The correlation exists during a period of 1-2 hrs centered at about 2 h 24 m that includes the time of the 5nu burst detected by the Mont Blanc detector on 23 February, 1987. The correlation is such that the gravitational wave signal precede the neutrino signals by a 1.1 +/- 0.5 s. The physical mechanisms of the correlation are not yet known.

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