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Detecting a non-Gaussian stochastic background of gravitational radiation

Steve Drasco·Eanna E. Flanagan
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Abstract

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.

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Steve Drasco, Eanna E. Flanagan. 2001-01-15. Detecting a non-Gaussian stochastic background of gravitational radiation. https://arxiv.org/abs/gr-qc/0101051

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