Future gravitational-wave detectors operated at cryogenic temperatures are expected to be limited by thermal noise of the highly reflective mirror coatings. Silicon nitride is an interesting material for such coatings as it shows very low mechanical loss, a property related to low thermal noise, which is known to further decrease under stress. Low optical absorption is also required to maintain the low mirror temperature. Here, we investigate the effect of stress on the optical properties at 1,550 nm of silicon nitride membranes attached to a silicon frame. Our approach includes the measurement of the thermal expansion coefficient and the thermal conductivity of the membranes. The membrane and frame temperatures are varied, and translated i...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
Thermal noise of highly reflective mirror coatings is a major limit to the sensitivity of many preci...
Future gravitational wave detectors (GWDs) such as Advanced LIGO upgrades and the Einstein Telescope...
Future gravitational-wave detectors operated at cryogenic temperatures are expected to be limited by...
Future gravitational-wave detectors operated at cryogenic temperatures are expected to be limited by...
Because of a low mechanical loss, thin films made of silicon nitride (Si3N4) are interesting for fun...
This study investigates a multilayer high reflector with new coating materials for next-generation l...
International audienceWe have measured the thermal properties of suspended membranes from 10 K to 30...
Gravitational waves were predicted by Einstein’s General Theory of Relativity which described gravit...
We study the mechanical dissipation of the fundamental mode of millimeter-sized, high quality-factor...
Thermal noise in the highly reflective mirror coatings is one of the main limitations to the sensiti...
In this paper, we characterize the Thermo-optic properties of silicon nitride ring resonators betwee...
The successful detection of gravitational waves from astrophysical sources carried out by the laser ...
Optical interferometry offers a powerful tool for the study of the mechanical motion of micro- and n...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
Thermal noise of highly reflective mirror coatings is a major limit to the sensitivity of many preci...
Future gravitational wave detectors (GWDs) such as Advanced LIGO upgrades and the Einstein Telescope...
Future gravitational-wave detectors operated at cryogenic temperatures are expected to be limited by...
Future gravitational-wave detectors operated at cryogenic temperatures are expected to be limited by...
Because of a low mechanical loss, thin films made of silicon nitride (Si3N4) are interesting for fun...
This study investigates a multilayer high reflector with new coating materials for next-generation l...
International audienceWe have measured the thermal properties of suspended membranes from 10 K to 30...
Gravitational waves were predicted by Einstein’s General Theory of Relativity which described gravit...
We study the mechanical dissipation of the fundamental mode of millimeter-sized, high quality-factor...
Thermal noise in the highly reflective mirror coatings is one of the main limitations to the sensiti...
In this paper, we characterize the Thermo-optic properties of silicon nitride ring resonators betwee...
The successful detection of gravitational waves from astrophysical sources carried out by the laser ...
Optical interferometry offers a powerful tool for the study of the mechanical motion of micro- and n...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
Thermal noise of highly reflective mirror coatings is a major limit to the sensitivity of many preci...
Future gravitational wave detectors (GWDs) such as Advanced LIGO upgrades and the Einstein Telescope...