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Detection of gravitational waves from coalescing binaries in the time domain

L Milano-+,++, F Barone-+,++ and M Milano§

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We propose a multistep procedure for the on-line detection and analysis of gravitational wave signals emitted during the coalescence of compact binaries. This procedure, based on a hierarchical strategy, consists of a rough analysis of the gravitational wave signal using adaptive line enhancers (ALE) filters and the controlled random search (CRS) optimization algorithm followed by a refined analysis using the classic matched-filtering technique. The results of simulations for the rough analysis are quite promising both for the relatively small computational power needed and for the robustness of the algorithms used, so that it could be very helpful for gravitational wave detection with very large baseline interferometric detectors like LIGO and VIRGO.


PACS

04.80.Nn Gravitational wave detectors and experiments

97.80.-d Binary and multiple stars

MSC

83C35 Gravitational waves

Subjects

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 6 (June 1997)

Received 16 August 1996, in final form 22 January 1997



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