Detection of gravitational collapse

Details Detection of gravitational collapse Detection of gravitational collapse

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aipc...96..214w&link_type=abstract

AIP Conference Proceedings, Volume 96, pp. 214-224 (1983).

Physics

Supernovae, Elementary Particle Processes

Scientific paper

At least one kind of supernova is expected to emit a large flux of neutrinos and gravitational radiation because of the collapse of a core to form a neutron star. Such collapse events may in addition occur in the absence of any optical display. The corresponding neutrino bursts can be detected via Cerenkov events in the same water used in proton decay experiments. Dedicated equipment is under construction to detect the gravitational radiation. Events throughout the Galaxy could be detectable, but are expected only at intervals exceeding a decade. Nevertheless, the next event could come tomorrow, so every attempt should be made to make the monitoring for such events routine.

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