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Thermal noise reduction for present and future gravitational wave detectors

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TLDR
In this paper, the 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, and new materials and new designs are needed to further reduce the suspension thermal noise.
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.

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Citations
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Breaking strength tests on silicon and sapphire bondings for gravitational wave detectors

TL;DR: In this paper, the breaking strength of the silicate bonding that glues cylinders of silicon (Si) and sapphire (Al2O3) has been investigated, and all material combinations, flatness quality and orientations have been tested over time.
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First characterization of silicon crystalline fibers produced with the μ-pulling technique for future gravitational wave detectors

TL;DR: In this article, the design and fabrication of low thermal-noise suspensions made of a new material presently under investigation is reported. And the first measurements of the fiber mechanical and thermal properties at room temperature have been performed and interpreted.
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Molecular adsorbed layer formation on cooled mirrors and its impacts on cryogenic gravitational wave telescopes

TL;DR: In this article, the formation of a molecular adlayer on a cold mirror was investigated and the formation rate of the adlayer was shown to be $27.2 and $2.073, respectively.
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Orthogonal ribbons for suspending test masses in interferometric gravitational wave detectors

TL;DR: In this paper, a simple modification of ribbon suspensions for laser interferometric gravitational wave detectors can substantially reduce the amplitude of violin modes at the expense of a small deterioration of suspension thermal noise.
Journal ArticleDOI

Cryogenic vacuum considerations for future gravitational wave detectors

TL;DR: In this article, the consequences of hosting a cryogenically cooled mirror in a vacuum system and sets new limits for an acceptable operating pressure to avoid frost formation in a given period of continuous data taking.
References
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Journal ArticleDOI

Irreversibility and Generalized Noise

TL;DR: In this article, a relation between the generalized resistance and the generalized forces in linear dissipative systems is obtained, which forms the extension of the Nyquist relation for the voltage fluctuations in electrical impedances.
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On a Theorem of Irreversible Thermodynamics

TL;DR: In this paper, a relation between the parameter describing the irreversible response of a driven dissipative system and the spontaneous fluctuations of the thermodynamic extensive parameters of the system in equilibrium is obtained.
Book

The Detection of Gravitational Waves

TL;DR: Blair et al. as discussed by the authors presented an introduction to Gravitational Waves and methods for their detection, including the sources of gravitational waves, detectors, and sources of internal friction in high Q materials.
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Thermodynamical fluctuations and photo-thermal shot noise in gravitational wave antennae

TL;DR: In this article, thermal expansion coefficients of the temperature in mirrors of gravitational wave antennae are transformed through the thermal expansion coefficient into additional noise, which leads to the necessity to reexamine the choice of materials for the mirrors.
Journal ArticleDOI

Recommended Values for the Thermal Expansivity of Silicon from 0 to 1000 K

TL;DR: In this paper, various absolute determinations of the thermal expansivity of both single crystal and polycrystalline silicon are used to establish a smooth relationship from 90 to 850 K which is believed to be reliable to roughly 10−8 K−1, and which is extrapolated to 1000 K.
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