We report on the optical, mechanical and structural characterization of the sputtered coating materials of Advanced LIGO, Advanced Virgo and KAGRA gravitational-waves detectors. We present the latest results of our research program aiming at decreasing coating thermal noise through doping, optimization of deposition parameters and post-deposition annealing. Finally, we propose sputtered Si3N4as a candidate material for the mirrors of future detectors
Thermal noise in the highly reflective mirror coatings is one of the main limitations to the sensiti...
Thermal noise in amorphous coatings is a limitation for a wide range of precision experiments such a...
In this Perspective, we summarize the status of technological development for large-area and low-noi...
International audienceWe report on the optical, mechanical and structural characterization of the sp...
Brownian thermal noise associated with highly reflective mirror coatings is a fundamental limit for ...
Coating thermal noise is a fundamental limit for experiments involving optical and quantum transduce...
4th August 2017, 12.30.43 Italian time: A gravitational wave crossed the Earth. To generate it, the ...
International audienceWe present the results of mechanical characterizations of many different high-...
Coating thermal noise is one of the dominant noise sources in current gravitational wave detectors a...
High-reflection interference mirrors for current gravitational wave detectors (aLIGO, Advanced Virgo...
Gravitational waves are detected by measuring length changes between mirrors in the arms of kilomet...
We report on the results of an extensive campaign of optical and mechanical characterization of the ...
Gravitational waves are a prediction of Einstein's General Theory of Relativity. Astrophysical event...
Brownian thermal noise associated with highly reflective coatings is a fundamental limit for several...
This study investigates a multilayer high reflector with new coating materials for next-generation l...
Thermal noise in the highly reflective mirror coatings is one of the main limitations to the sensiti...
Thermal noise in amorphous coatings is a limitation for a wide range of precision experiments such a...
In this Perspective, we summarize the status of technological development for large-area and low-noi...
International audienceWe report on the optical, mechanical and structural characterization of the sp...
Brownian thermal noise associated with highly reflective mirror coatings is a fundamental limit for ...
Coating thermal noise is a fundamental limit for experiments involving optical and quantum transduce...
4th August 2017, 12.30.43 Italian time: A gravitational wave crossed the Earth. To generate it, the ...
International audienceWe present the results of mechanical characterizations of many different high-...
Coating thermal noise is one of the dominant noise sources in current gravitational wave detectors a...
High-reflection interference mirrors for current gravitational wave detectors (aLIGO, Advanced Virgo...
Gravitational waves are detected by measuring length changes between mirrors in the arms of kilomet...
We report on the results of an extensive campaign of optical and mechanical characterization of the ...
Gravitational waves are a prediction of Einstein's General Theory of Relativity. Astrophysical event...
Brownian thermal noise associated with highly reflective coatings is a fundamental limit for several...
This study investigates a multilayer high reflector with new coating materials for next-generation l...
Thermal noise in the highly reflective mirror coatings is one of the main limitations to the sensiti...
Thermal noise in amorphous coatings is a limitation for a wide range of precision experiments such a...
In this Perspective, we summarize the status of technological development for large-area and low-noi...