Detecting a non-Gaussian stochastic background of gravitational radiation

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dc.creatorDrasco, Steve
dc.creatorFlanagan, Eanna E.
dc.date2001-01-15
dc.date.accessioned2026-07-07T03:25:36Z
dc.date.available2026-07-07T03:25:36Z
dc.descriptionWe derive a detection method for a stochastic background of gravitational waves produced by events where the ratio of the average time between events to the average duration of an event is large. Such a signal would sound something like popcorn popping. Our derivation is based on the somewhat unrealistic assumption that the duration of an event is smaller than the detector time resolution.
dc.description2 pages, submitted to the Proceedings of the 9th Marcel Grossmann Meeting, Rome, 2-8 July, 2000
dc.identifierhttps://arxiv.org/abs/gr-qc/0101051
dc.identifierhttp://arxiv.org/abs/gr-qc/0101051
dc.identifierProceedings of the Ninth Marcel Grossmann Meeting on General Relativity, edited by V.G. Gurzadyan, R.T. Jantzen and R. Ruffini,World Scientific, Singapore, p. 1913 (2002)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33770
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleDetecting a non-Gaussian stochastic background of gravitational radiation
dc.typetext

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