Other
Scientific paper
Aug 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nciml..31..499f&link_type=abstract
Nuovo Cimento, Lettere, Serie 2, vol. 31, Aug. 8, 1981, p. 499, 500.
Other
9
Gravitational Waves, Neutrinos, Particle Mass, Supernovae, Time Lag, Gravitational Collapse, Stellar Flares
Scientific paper
It is proposed that the time delay between the reception of a gravitational wave signal and a neutrino pulse from a supernova explosion may be used as an indicator of neutrino mass. It is shown that if the neutrino is truly a massless particle, the gravitational waves and neutrinos emitted from a stellar gravitational collapse should arrive within 0.1 sec of each other, while if the neutrino has a mass, the delay of the neutrino signal will be proportional to the distance of the supernova and neutrino emission energy and mass. It is noted that present neutrino detectors and gravitational wave antennas are sufficiently sensitive to allow an accurate measurement of the time delay for galactic supernova explosions.
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