Advanced generations of ground-based gravitational wave detectors will use ultra-low-loss amorphous dielectric multilayer mirror coatings in order to minimise thermal noise, a limiting factor in detector sensitivity. Transmission electron microscopy is a promising way to probe the atomic structure of these coatings in an effort to better understand the causes of the observed mechanical loss (internal friction) and hence thermal noise
International audienceWe report on the results of an extensive campaign of optical and mechanical ch...
<p>Highly reflective dielectric mirror coatings are critical components in a range of precisio...
Thermal noise associated with the mechanical loss of current highly reflective mirror coatings is a ...
Current interferometric gravitational wave detectors use test masses with mirror coatings formed fro...
Future advanced gravitational wave detectors will need to be constructed using ultra low loss materi...
International audienceMirror coatings play a crucial role in the performance of laser interferometer...
Amorphous tantala (a-Ta2O5) is an important technological material that has wide ranging application...
High finesse optical cavities of current interferometric gravitational-wave detectors are significan...
AbstractAmorphous tantala (a-Ta2O5) is an important technological material that has wide ranging app...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
All current gravitational wave detectors use test masses coated with alternating layers of two diffe...
Previous studies have quantified the mechanical dissipation associated with dielectric thin films fo...
2021 Summer.Includes bibliographical references.Amorphous thin films prepared from vapor deposition ...
Thermal noise arising from high-reflective mirror coatings limits the current ground-based gravitati...
International audienceThermal noise of the mirrors limits the sensitivity of interferometric gravita...
International audienceWe report on the results of an extensive campaign of optical and mechanical ch...
<p>Highly reflective dielectric mirror coatings are critical components in a range of precisio...
Thermal noise associated with the mechanical loss of current highly reflective mirror coatings is a ...
Current interferometric gravitational wave detectors use test masses with mirror coatings formed fro...
Future advanced gravitational wave detectors will need to be constructed using ultra low loss materi...
International audienceMirror coatings play a crucial role in the performance of laser interferometer...
Amorphous tantala (a-Ta2O5) is an important technological material that has wide ranging application...
High finesse optical cavities of current interferometric gravitational-wave detectors are significan...
AbstractAmorphous tantala (a-Ta2O5) is an important technological material that has wide ranging app...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
All current gravitational wave detectors use test masses coated with alternating layers of two diffe...
Previous studies have quantified the mechanical dissipation associated with dielectric thin films fo...
2021 Summer.Includes bibliographical references.Amorphous thin films prepared from vapor deposition ...
Thermal noise arising from high-reflective mirror coatings limits the current ground-based gravitati...
International audienceThermal noise of the mirrors limits the sensitivity of interferometric gravita...
International audienceWe report on the results of an extensive campaign of optical and mechanical ch...
<p>Highly reflective dielectric mirror coatings are critical components in a range of precisio...
Thermal noise associated with the mechanical loss of current highly reflective mirror coatings is a ...