Coating thermal noise is a fundamental limit for experiments involving optical and quantum transducers. We report on the latest research activity on low-noise coatings at the Laboratoire des Matériaux Avancés, from updated values for the current Ta2O5, Ta2O5-TiO2 and SiO2 coatings of the Advanced LIGO, Advanced Virgo and KAGRA detectors to recent results from sputtered Nb2O5, TiO2-Nb2O5, Ta2O5-ZrO2, MgF2, AlF3 and Si3N4 coatings. Some alternative options, like amorphous-silicon and AlGaAs crystalline coatings among others, are also briefly discussed.

Progress in the measurement and reduction of thermal noise in optical coatings for gravitational-wave detectors

Cagnoli G.;
2019

Abstract

Coating thermal noise is a fundamental limit for experiments involving optical and quantum transducers. We report on the latest research activity on low-noise coatings at the Laboratoire des Matériaux Avancés, from updated values for the current Ta2O5, Ta2O5-TiO2 and SiO2 coatings of the Advanced LIGO, Advanced Virgo and KAGRA detectors to recent results from sputtered Nb2O5, TiO2-Nb2O5, Ta2O5-ZrO2, MgF2, AlF3 and Si3N4 coatings. Some alternative options, like amorphous-silicon and AlGaAs crystalline coatings among others, are also briefly discussed.
2019
Optics InfoBase Conference Papers
Optical Interference Coatings, OIC 2019
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11577/3578092
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