Studies of the mechanical loss of silicon flexures in a temperature region from 5 to 300 K are presented, where the flexures have been prepared by different fabrication techniques of interest for the construction of suspension elements of future interferometric gravitational wave detectors. A lowest mechanical loss of 3 × 10−8 was observed for a 130 μm thick flexure at around 10 K. While the mechanical loss follows the thermo-elastic predictions down to 50 K, at lower temperatures the observed loss is found to be a function of surface roughness. This surface loss is of interest for all applications using silicon-based oscillators at low temperatures. The extraction of a surface loss parameter using results from our measurements and those of...
Thermal noise of the mirrors limits the sensitivity of interferometric gravitational-wave detectors ...
The research work developed in the present PhD thesis deals with the measurement of mechanical dissi...
The design of next generation gravitational wave observatories considers operation at cryogenic temp...
Studies of the mechanical loss of silicon flexures in a temperature region from 5 to 300 K are prese...
The thermo-mechanical properties of silicon make it of significant interest as a possible material f...
Low mechanical loss materials are needed to further decrease thermal noise in upcoming gravitational...
Silicon optics suspended by silicon ribbons or silicon fibers and kept at low temperature are being ...
Some proposed interferometric gravitational wave detectors of the next generation are designed to us...
The paper summarises systematic studies of the mechanical loss of crystalline silicon at low tempera...
In order to reduce the thermal noise in future interferometers for gravitational wave (GW) detectors...
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...
In order to reduce the thermal noise in future interferometers for gravitational wave (GW) detectors...
The announcement of the direct detection of gravitational waves (GW) by the LIGO and Virgo collabora...
Current interferometric gravitational wave detectors (IGWDs) are operated at room temperature with t...
Thermal noise of the mirrors limits the sensitivity of interferometric gravitational-wave detectors ...
The research work developed in the present PhD thesis deals with the measurement of mechanical dissi...
The design of next generation gravitational wave observatories considers operation at cryogenic temp...
Studies of the mechanical loss of silicon flexures in a temperature region from 5 to 300 K are prese...
The thermo-mechanical properties of silicon make it of significant interest as a possible material f...
Low mechanical loss materials are needed to further decrease thermal noise in upcoming gravitational...
Silicon optics suspended by silicon ribbons or silicon fibers and kept at low temperature are being ...
Some proposed interferometric gravitational wave detectors of the next generation are designed to us...
The paper summarises systematic studies of the mechanical loss of crystalline silicon at low tempera...
In order to reduce the thermal noise in future interferometers for gravitational wave (GW) detectors...
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...
In order to reduce the thermal noise in future interferometers for gravitational wave (GW) detectors...
The announcement of the direct detection of gravitational waves (GW) by the LIGO and Virgo collabora...
Current interferometric gravitational wave detectors (IGWDs) are operated at room temperature with t...
Thermal noise of the mirrors limits the sensitivity of interferometric gravitational-wave detectors ...
The research work developed in the present PhD thesis deals with the measurement of mechanical dissi...
The design of next generation gravitational wave observatories considers operation at cryogenic temp...