Measurements of Superattenuator seismic isolation by Virgo interferometer

F. Acernese, H.J. Bulten, D.S. Rabeling, J.F.J. van den Brand, Th. S. Bauer, M.G. Beker, T.G.F. Li, S. van der Putten

Research output: Contribution to JournalArticleAcademicpeer-review

Abstract

Each mirror of the interferometric gravitational wave antenna Virgo is attached to a Superattenuator, a chain of mechanical filters designed to suppress seismic vibrations, starting from a few Hz. The filter chain attenuation has been measured by exciting its suspension point with sinuisodal forces and using the interferometer as sensor. The attenuation, measured at different frequencies, is compliant with the requirements of the next generation antenna Advanced Virgo. In the third generation detector Einstein Telescope, the attenuation is sufficient above 3 Hz, independently of the underground site choice. © 2010 Elsevier B.V. All rights reserved.
Original languageEnglish
Pages (from-to)182-189
JournalAstroparticle Physics
Volume33
Issue number3
DOIs
Publication statusPublished - 2010

Fingerprint

Dive into the research topics of 'Measurements of Superattenuator seismic isolation by Virgo interferometer'. Together they form a unique fingerprint.

Cite this