Add to ORKGThermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many precision measurement systems, including optical frequency standards, high-resolution optical spectroscopy and interferometric gravity wave detectors. Presented here are measurements of dissipation as a function of temperature between 7 K and 290 K in ion-beam-sputtered Ta2O5 doped with TiO2, showing a loss peak at 20 K. Analysis of the peak provides the first evidence of the source of dissipation in doped Ta2O5 coatings, leading to possibilities for the reduction of thermal noise effects
High finesse optical cavities of current interferometric gravitational-wave detectors are significan...
Coating thermal noise is a fundamental limit for experiments involving optical and quantum transduce...
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...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
The mechanical dissipation of ion-beam-sputtered optical coatings is expected to be a limiting sourc...
Thermal noise arising from mechanical dissipation in dielectric reflective coatings is expected to c...
Thermal noise arising from mechanical dissipation in dielectric reflective coatings is expected to c...
The exceptional stability required from high finesse optical cavities and high precision interferome...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...
Here we report the first results comparing the temperature dependence of the mechanical dissipation ...
Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next...
Predicted in 1916 by Einstein, then detected one hundred year later by the VIRGO and LIGO collaborat...
Previous studies have quantified the mechanical dissipation associated with dielectric thin films fo...
High finesse optical cavities of current interferometric gravitational-wave detectors are significan...
Coating thermal noise is a fundamental limit for experiments involving optical and quantum transduce...
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...
Thermal noise arising from mechanical dissipation in oxide coatings is a major limitation to many pr...
The mechanical dissipation of ion-beam-sputtered optical coatings is expected to be a limiting sourc...
Thermal noise arising from mechanical dissipation in dielectric reflective coatings is expected to c...
Thermal noise arising from mechanical dissipation in dielectric reflective coatings is expected to c...
The exceptional stability required from high finesse optical cavities and high precision interferome...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...
Here we report the first results comparing the temperature dependence of the mechanical dissipation ...
Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next...
Predicted in 1916 by Einstein, then detected one hundred year later by the VIRGO and LIGO collaborat...
Previous studies have quantified the mechanical dissipation associated with dielectric thin films fo...
High finesse optical cavities of current interferometric gravitational-wave detectors are significan...
Coating thermal noise is a fundamental limit for experiments involving optical and quantum transduce...
The interferometer mirrors of Gravitational-Wave Detectors (GWD) are Bragg reflectors made of altern...