Progress in the measurement and reduction of thermal noise in optical coatings for gravitational-wave detectors
arXiv:1912.11394 · doi:10.1364/AO.377293
Abstract
Coating thermal noise is a fundamental limit for precision experiments based on optical and quantum transducers. In this review, after a brief overview of the techniques for coating thermal noise measurements, we present the latest world-wide research activity on low-noise coatings, with a focus on the results obtained at the Laboratoire des Matériaux Avancés. We report new updated values for the TaO, TaO-TiO and SiO coatings of the Advanced LIGO, Advanced Virgo and KAGRA detectors, and new results from sputtered NbO, TiO-NbO, TaO-ZrO, MgF, AlF and silicon nitride coatings. Amorphous silicon, crystalline coatings, high-temperature deposition, multi-material coatings and composite layers are also briefly discussed, together with the latest developments of structural analyses and models.
arXiv commentarXiv admin note: text overlap with arXiv:1909.03737
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Cited by in corpus (21)
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