作者: A Pasqualetti , R Poggiani , F Frasconi , S Rapisarda , P Popolizio
DOI: 10.1088/0264-9381/15/11/004
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摘要: In this paper we analyse the noise level induced by changes in mass density distribution around Virgo interferometric antenna. These stochastic fluctuations generate a gravitational field which couples directly to mirrors of optical apparatus, and it could be relevant if planned final sensitivity interferometer is reached.