Estimate of the background of a gravitational-wave detector due to cosmic rays View Full Text


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Article Info

DATE

1986-03

AUTHORS

E. Amaldi, G. Pizzella

ABSTRACT

The authors examine once more the effect of cosmic rays on a resonating gravitational-wave antenna in view of the very high sensitivities that are required for detecting the supernovae of the Virgo Cluster. They show that, at sea-level, the secondaries generated in the bar by the electromagnetic interaction of high-energy muons produce signals with rates much larger than that expected from supernovae. This inconvenience is eliminated in an underground laboratory. More... »

PAGES

612-620

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/bf02514879

DOI

http://dx.doi.org/10.1007/bf02514879

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1010231595


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