The dominant noise source in aLIGO is Brownian thermal noise, due to mechanical losses in the atomic structure of the amorphous titania doped tantala end test-mass mirror coatings. This thesis investigates the structural source of these losses. The effect of titania doping and thermal annealing upon the atomic structure of amorphous tantalum pentoxide coating preparations are studied using advanced electron diffraction techniques. Significant differences between the coating atomic structures have been identified for the first time in detail. The tantala based coatings studied have been demonstrated as better described by a heterogeneous phase separated model, rather than the continuous random network model for covalently bonded amorp...
We estimate the loss angles of the materials currently used in the highly reflective test-mass coati...
© 2019 American Physical Society. Understanding the local atomic order in amorphous thin film coatin...
Advanced generations of ground-based gravitational wave detectors will use ultra-low-loss amorphous ...
The dominant noise source in aLIGO is Brownian thermal noise, due to mechanical losses in the atomic...
Amorphous tantala (a-Ta2O5) is an important technological material that has wide ranging application...
AbstractAmorphous tantala (a-Ta2O5) is an important technological material that has wide ranging app...
Amorphous tantala (a-Ta2O5) is an important technological material that has wide ranging application...
Understanding the local atomic order in amorphous thin film coatings and how it relates to macroscop...
<p>Highly reflective dielectric mirror coatings are critical components in a range of precisio...
We have investigated by spectroscopic ellipsometry (SE, 190-1700 nm) the optical properties of unifo...
International audienceWe present the results of mechanical characterizations of many different high-...
2021 Summer.Includes bibliographical references.Amorphous thin films prepared from vapor deposition ...
The exceptional stability required from high finesse optical cavities and high precision interferome...
The interferometer mirrors of Gravitational-Wave Detectors (GWD) are Bragg reflectors made of altern...
High-reflection interference mirrors for current gravitational wave detectors (aLIGO, Advanced Virgo...
We estimate the loss angles of the materials currently used in the highly reflective test-mass coati...
© 2019 American Physical Society. Understanding the local atomic order in amorphous thin film coatin...
Advanced generations of ground-based gravitational wave detectors will use ultra-low-loss amorphous ...
The dominant noise source in aLIGO is Brownian thermal noise, due to mechanical losses in the atomic...
Amorphous tantala (a-Ta2O5) is an important technological material that has wide ranging application...
AbstractAmorphous tantala (a-Ta2O5) is an important technological material that has wide ranging app...
Amorphous tantala (a-Ta2O5) is an important technological material that has wide ranging application...
Understanding the local atomic order in amorphous thin film coatings and how it relates to macroscop...
<p>Highly reflective dielectric mirror coatings are critical components in a range of precisio...
We have investigated by spectroscopic ellipsometry (SE, 190-1700 nm) the optical properties of unifo...
International audienceWe present the results of mechanical characterizations of many different high-...
2021 Summer.Includes bibliographical references.Amorphous thin films prepared from vapor deposition ...
The exceptional stability required from high finesse optical cavities and high precision interferome...
The interferometer mirrors of Gravitational-Wave Detectors (GWD) are Bragg reflectors made of altern...
High-reflection interference mirrors for current gravitational wave detectors (aLIGO, Advanced Virgo...
We estimate the loss angles of the materials currently used in the highly reflective test-mass coati...
© 2019 American Physical Society. Understanding the local atomic order in amorphous thin film coatin...
Advanced generations of ground-based gravitational wave detectors will use ultra-low-loss amorphous ...