Title of article
Thermal noise reduction for present and future gravitational wave detectors
Author/Authors
Amico، نويسنده , , P and Bosi، نويسنده , , L and Gammaitoni، نويسنده , , L and Losurdo، نويسنده , , G and Marchesoni، نويسنده , , F and Mazzoni، نويسنده , , M and Punturo، نويسنده , , M and Stanga، نويسنده , , R and Toncelli، نويسنده , , A and Tonelli، نويسنده , , M and Travasso، نويسنده , , F and Vetrano، نويسنده , , F and Vocca، نويسنده , , H، نويسنده ,
Pages
4
From page
240
To page
243
Abstract
Thermal noise in mirror suspension is and will be the most severe fundamental limit to the low-frequency sensitivity of interferometric gravitational wave detectors currently under construction. The technical solutions, adopted in the Virgo detector, optimize the current suspension scheme, but new materials and new designs are needed to further reduce the suspension thermal noise. Silicon fibers are promising candidates both for room temperature advanced detectors and for future cryogenic interferometric detectors.
Keywords
thermal noise , Silicon , Gravitational wave detectors
Journal title
Astroparticle Physics
Record number
2022362
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