Using Resonant Bars and Interferometers to Search for Stochastic Gravitational Waves

Details Using Resonant Bars and Interferometers to Search for Stochastic Gravitational Waves Using Resonant Bars and Interferometers to Search for Stochastic Gravitational Waves

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..tsf.c1009w&link_type=abstract

American Physical Society, Joint Fall Meeting of the Texas Sections of the , abstract #C1.009

Astronomy and Astrophysics

Astrophysics

Scientific paper

A stochastic background of gravitational waves (SBGW) may result from gravitational waves emitted in the early universe (e.g., during inflation) or from a superposition of many unresolved astrophysical sources. Pairs of resonant bar detectors, as well as pairs of prototype interferometers, have been used to set limits on SBGW strength by looking for correlations between the random signals in the two detectors, and data from the two LIGO interferometers are being analyzed right now for this purpose. I will describe a parallel analysis being carried out to look for SBGW-induced correlations between the LIGO detector in Livingston, LA and the ALLEGRO resonant bar detector in Baton Rouge, LA.

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