Materials with a high quality factor are used, for the test mass and suspension elements, in interferometric gravitational wave detectors to reduce off resonance thermal displacement noise. An experiment to increase the quality factor of mechanically polished silica cantilevers by etching their surface is described. An estimation of the thickness of the damaged layer due to polishing is found and we estimate how lossy this layer is. This was achieved by repeatedly etching a cantilever in solution and measuring its mechanical loss in each instance. In this way mechanical loss as a function of etch depth can be determined. This layer was estimated to be 0.5 micron deep with a loss of Os=2.98 x 10-8 which is three times higher than the surface...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
The Glasgow group is involved in the construction of the GE0600 interferometer as well as in R&D act...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Materials with a high quality factor are used, for the test mass and suspension elements, in interfe...
The work of this thesis involves the analysis of mechanical losses associated with coated test masse...
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 ...
In his 1916 General Theory of Relativity, Einstein predicted the existence of gravitational waves. T...
Current interferometric gravitational wave detectors use test masses with mirror coatings formed fro...
Interferometric gravitational wave detectors use mirrors whose substrates are formed from materials ...
Mechanical and optical thermal noises play an important role in many precise opto-mechanical experim...
International audienceMechanical and optical thermal noises play an important role in many precise o...
Brownian thermal noise generated by mechanical losses in thin film coatings limits the sensitivity o...
Gravitational waves were predicted by Einstein’s General Theory of Relativity which described gravit...
International audienceWe present the results of mechanical characterizations of many different high-...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
The Glasgow group is involved in the construction of the GE0600 interferometer as well as in R&D act...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Materials with a high quality factor are used, for the test mass and suspension elements, in interfe...
The work of this thesis involves the analysis of mechanical losses associated with coated test masse...
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 ...
In his 1916 General Theory of Relativity, Einstein predicted the existence of gravitational waves. T...
Current interferometric gravitational wave detectors use test masses with mirror coatings formed fro...
Interferometric gravitational wave detectors use mirrors whose substrates are formed from materials ...
Mechanical and optical thermal noises play an important role in many precise opto-mechanical experim...
International audienceMechanical and optical thermal noises play an important role in many precise o...
Brownian thermal noise generated by mechanical losses in thin film coatings limits the sensitivity o...
Gravitational waves were predicted by Einstein’s General Theory of Relativity which described gravit...
International audienceWe present the results of mechanical characterizations of many different high-...
Mirror thermal noise in Ta2O5/SiO2 coatings is predicted to be the limiting noise in the 50-300 Hz f...
The Glasgow group is involved in the construction of the GE0600 interferometer as well as in R&D act...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...