Wide-band measurement of gravitational waves - The VIRGO project

Details Wide-band measurement of gravitational waves - The VIRGO project Wide-band measurement of gravitational waves - The VIRGO project

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ncimc..15..955g&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 15 C, no. 6, p. 955-971.

Computer Science

4

Background Noise, Calibrating, Gravitational Wave Antennas, Sensitivity, Broadband, Michelson Interferometers, Noise Spectra, Resonant Frequencies

Scientific paper

To detect gravitational waves (GW) in a frequency range between 10 Hz and few kHz a ground-based antenna was designed by the French-Italian collaboration VIRGO. The antenna is a 3 km long interferometer with special suspensions for the optical components, planned to reduce the seismic noise in order to reach the low-frequency region. Results on the seismic isolation devices are given together with some preliminary results on the use of permanent magnets on the VIRGO suspensions.

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