Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz frequency range in the interferometric gravitational wave detectors. Ta2O5 losses were dominating compared to the SiO2 losses. We developed a model to calculate multilayer mechanical losses and we are working for low mechanical losses Ta2O5/SiO2 coatings
Thermal noise of the mirrors limits the sensitivity of interferometric gravitational-wave detectors ...
Future gravitational wave detectors (GWDs) such as Advanced LIGO upgrades and the Einstein Telescope...
A standard quarter-wavelength multilayer optical coating will produce the highest reflectivity for a...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next...
International audienceMirror coatings play a crucial role in the performance of laser interferometer...
International audienceWe estimate the loss angles of the materials currently used in the highly refl...
Current interferometric gravitational wave detectors use test masses with mirror coatings formed fro...
International audienceWe present the results of mechanical characterizations of many different high-...
International audienceThermal noise of the mirrors limits the sensitivity of interferometric gravita...
Coating thermal noise is a fundamental limit for experiments involving optical and quantum transduce...
Coating thermal noise is one of the dominant noise sources in current gravitational wave detectors a...
The interferometer mirrors of Gravitational-Wave Detectors (GWD) are Bragg reflectors made of altern...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
All current gravitational wave detectors use test masses coated with alternating layers of two diffe...
Thermal noise of the mirrors limits the sensitivity of interferometric gravitational-wave detectors ...
Future gravitational wave detectors (GWDs) such as Advanced LIGO upgrades and the Einstein Telescope...
A standard quarter-wavelength multilayer optical coating will produce the highest reflectivity for a...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next...
International audienceMirror coatings play a crucial role in the performance of laser interferometer...
International audienceWe estimate the loss angles of the materials currently used in the highly refl...
Current interferometric gravitational wave detectors use test masses with mirror coatings formed fro...
International audienceWe present the results of mechanical characterizations of many different high-...
International audienceThermal noise of the mirrors limits the sensitivity of interferometric gravita...
Coating thermal noise is a fundamental limit for experiments involving optical and quantum transduce...
Coating thermal noise is one of the dominant noise sources in current gravitational wave detectors a...
The interferometer mirrors of Gravitational-Wave Detectors (GWD) are Bragg reflectors made of altern...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
All current gravitational wave detectors use test masses coated with alternating layers of two diffe...
Thermal noise of the mirrors limits the sensitivity of interferometric gravitational-wave detectors ...
Future gravitational wave detectors (GWDs) such as Advanced LIGO upgrades and the Einstein Telescope...
A standard quarter-wavelength multilayer optical coating will produce the highest reflectivity for a...