We present mechanical Q-factors (quality factors) of a crystalline quartz test mass with a nano-structured surface, measured in the temperature regime from 5 to 300 K. The nano-structure was a grating with a period of 2 mu m and a depth of about 0.1 mu m. Comparative measurements were performed on the plain substrate and on the structured test mass with different numbers of SiO2/Ta2O5 coating layers. The measurements at different stages of the test mass fabrication process show that the surface distortion induced by the nanostructure does not severely lower the mechanical Q-factor of the substrate. Damping due to a multi-layer coating stack was found to be orders of magnitude higher. The results provide vital information concerning the pote...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
We performed noise measurements to obtain the quality factor (Q) and frequency shift of gold coated ...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...
We present mechanical Q-factors (quality factors) of a crystalline quartz test mass with a nano-stru...
doi:10.1088/1367-2630/9/7/225 Abstract. We present mechanical Q-factors (quality factors) of a cryst...
Current interferometric gravitational wave detectors (IGWDs) are operated at room temperature with t...
Future generations of gravitational wave interferometers are likely to be operated at cryogenic temp...
Thermal noise in the mirror substrates sets a most severe limit to the low-frequency sensitivity of ...
To minimize thermal noise in gravitational-wave detectors high mechanical quality factors are requir...
Future gravitational wave detectors will be limited by different kinds of noise. Thermal noise from ...
International audienceThermal noise of the mirrors limits the sensitivity of interferometric gravita...
Thermal noise of the mirrors limits the sensitivity of interferometric gravitational-wave detectors ...
Current interferometric gravitational wave detectors use the combination of quasi-monochromatic, con...
The successful detection of gravitational waves from astrophysical sources carried out by the laser ...
Materials with a high quality factor are used, for the test mass and suspension elements, in interfe...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
We performed noise measurements to obtain the quality factor (Q) and frequency shift of gold coated ...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...
We present mechanical Q-factors (quality factors) of a crystalline quartz test mass with a nano-stru...
doi:10.1088/1367-2630/9/7/225 Abstract. We present mechanical Q-factors (quality factors) of a cryst...
Current interferometric gravitational wave detectors (IGWDs) are operated at room temperature with t...
Future generations of gravitational wave interferometers are likely to be operated at cryogenic temp...
Thermal noise in the mirror substrates sets a most severe limit to the low-frequency sensitivity of ...
To minimize thermal noise in gravitational-wave detectors high mechanical quality factors are requir...
Future gravitational wave detectors will be limited by different kinds of noise. Thermal noise from ...
International audienceThermal noise of the mirrors limits the sensitivity of interferometric gravita...
Thermal noise of the mirrors limits the sensitivity of interferometric gravitational-wave detectors ...
Current interferometric gravitational wave detectors use the combination of quasi-monochromatic, con...
The successful detection of gravitational waves from astrophysical sources carried out by the laser ...
Materials with a high quality factor are used, for the test mass and suspension elements, in interfe...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
We performed noise measurements to obtain the quality factor (Q) and frequency shift of gold coated ...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...