Document Type

Article

Publication Date

1999

Abstract

If γ-ray bursts (GRBs) are accompanied by gravitational wave bursts (GWBs) the correlated output of two gravitational wave detectors evaluated in the moments just prior to a GRB will differ from that evaluated at other times. We can test for this difference without prior knowledge of either the GWB wave form or the detector noise spectrum. With a model for the GRB source population and GWB spectrum we can put a limit on the in-band rms GWB signal amplitude. Laser-Interferometer Gravitational Wave Observatory I detector observations coincident with 1000 GRB observations could lead us to exclude with 95% confidence associated GWBs with hRMS≳1.7×10−22.

Comments

© 1999 American Physical Society. Original published version available at https://doi.org/10.1103/PhysRevD.60.121101

Publication Title

Physical Review D

DOI

10.1103/PhysRevD.60.121101

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