Relevance of Newtonian seismic noise for the VIRGO interferometer sensitivity

Details Relevance of Newtonian seismic noise for the VIRGO interferometer sensitivity Relevance of Newtonian seismic noise for the VIRGO interferometer sensitivity

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cqgra..15.3339b&link_type=abstract

Classical and Quantum Gravity, Volume 15, Issue 11, pp. 3339-3362 (1998).

Physics

26

Scientific paper

In this paper we analyse the noise level induced by changes in the mass density distribution around the Virgo interferometric antenna. These stochastic mass density fluctuations generate a gravitational field which couples directly to the mirrors of the optical apparatus, and it could be relevant if the planned final sensitivity of the Virgo interferometer is to be reached.

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