Plane parallel mirrors Fabry-Perot cavity to improve Virgo superattenuators

Details Plane parallel mirrors Fabry-Perot cavity to improve Virgo superattenuators Plane parallel mirrors Fabry-Perot cavity to improve Virgo superattenuators

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phla..243..187b&link_type=abstract

Physics Letters A, Volume 243, Issue 4, p. 187-194.

Physics

7

Scientific paper

The measurement of the finesse and the longitudinal locking of a 100 μm long plane mirrors Fabry-Perot cavity is described. a finesse of up to 5400 has been found. If attached to the Virgo antenna suspension (SA), a similar device is sensitive enough to detect the thermal displacement noise of the SA test mass, which is expected to limit the Virgo antenna sensitivity between 10 and 600 Hz. Reducing the Virgo noise floor is a challenge for future antenna development, as this region is the most promising one for coalescing binary stars and pulsar signals.

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