Detecting a non-Gaussian stochastic background of gravitational radiation

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We 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.
2 pages, submitted to the Proceedings of the 9th Marcel Grossmann Meeting, Rome, 2-8 July, 2000

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General Relativity and Quantum Cosmology, Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/33770

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/gr-qc/0101051
 http://arxiv.org/abs/gr-qc/0101051
 Proceedings 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)

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arXiv