Add to ORKGThe mechanical dissipation of ion-beam-sputtered optical coatings is expected to be a limiting source of thermal noise for future interferometric gravitational wave detectors. Presented here are measurements of the dissipation as a function of temperature between 85 K and 290 K in a single layer of Ta2O5 doped with TiO2
International audienceCoating thermal noise is a fundamental limit for precision experiments based o...
High finesse optical cavities of current interferometric gravitational-wave detectors are significan...
Predicted in 1916 by Einstein, then detected one hundred year later by the VIRGO and LIGO collaborat...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
Thermal noise arising from mechanical dissipation in dielectric reflective coatings is expected to c...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
Here we report the first results comparing the temperature dependence of the mechanical dissipation ...
Thermal noise arising from mechanical dissipation in dielectric reflective coatings is expected to c...
Previous studies have quantified the mechanical dissipation associated with dielectric thin films fo...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
International audienceMirror coatings play a crucial role in the performance of laser interferometer...
Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next...
All current gravitational wave detectors use test masses coated with alternating layers of two diffe...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...
International audienceCoating thermal noise is a fundamental limit for precision experiments based o...
High finesse optical cavities of current interferometric gravitational-wave detectors are significan...
Predicted in 1916 by Einstein, then detected one hundred year later by the VIRGO and LIGO collaborat...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
Thermal noise arising from mechanical dissipation in dielectric reflective coatings is expected to c...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
Here we report the first results comparing the temperature dependence of the mechanical dissipation ...
Thermal noise arising from mechanical dissipation in dielectric reflective coatings is expected to c...
Previous studies have quantified the mechanical dissipation associated with dielectric thin films fo...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
International audienceMirror coatings play a crucial role in the performance of laser interferometer...
Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next...
All current gravitational wave detectors use test masses coated with alternating layers of two diffe...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...
International audienceCoating thermal noise is a fundamental limit for precision experiments based o...
High finesse optical cavities of current interferometric gravitational-wave detectors are significan...
Predicted in 1916 by Einstein, then detected one hundred year later by the VIRGO and LIGO collaborat...