Thermal noise associated with the dielectric optical coatings used to form the mirrors of interferometric gravitational wave detectors is expected to be an important limit to the sensitivity of future detectors. Improvements in detector performance are likely to require coating materials of lower mechanical dissipation. Typically, current coatings use multiple alternating layers of ion-beam-sputtered amorphous silica and tantalum pentoxide (doped with titania). We present here measurements of the mechanical dissipation of promising alternative crystalline coatings that use multi-layers of single crystal gallium phosphide (GaP) and aluminium gallium phosphide (AlGaP) that are epitaxially grown and lattice matched to a silicon substrate. Anal...
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...
We estimate the loss angles of the materials currently used in the highly reflective test-mass coati...
The first direct observations of gravitational waves have been made by the Advanced LIGO detectors. ...
The sensitivity of 2nd and 3rd generations of interferometric gravitational wave detectors will be l...
International audienceWe present the results of mechanical characterizations of many different high-...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...
The sensitivity of second and third generations of interferometric gravitational wave (GW) detectors...
All current gravitational wave detectors use test masses coated with alternating layers of two diffe...
The sensitivity of second and third generations of interferometric gravitational wave (GW) detectors...
In this Perspective, we summarize the status of technological development for large-area and low-noi...
Gravitational waves are detected by measuring length changes between mirrors in the arms of kilomet...
Interferometric gravitational wave detectors use mirrors whose substrates are formed from materials ...
Thermal noise arising from high-reflective mirror coatings limits the current ground-based gravitati...
Brownian thermal noise associated with highly reflective mirror coatings is a fundamental limit for ...
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...
We estimate the loss angles of the materials currently used in the highly reflective test-mass coati...
The first direct observations of gravitational waves have been made by the Advanced LIGO detectors. ...
The sensitivity of 2nd and 3rd generations of interferometric gravitational wave detectors will be l...
International audienceWe present the results of mechanical characterizations of many different high-...
Thermal noise arising from mechanical dissipation in oxide mirror coatings is an important limit to ...
The sensitivity of second and third generations of interferometric gravitational wave (GW) detectors...
All current gravitational wave detectors use test masses coated with alternating layers of two diffe...
The sensitivity of second and third generations of interferometric gravitational wave (GW) detectors...
In this Perspective, we summarize the status of technological development for large-area and low-noi...
Gravitational waves are detected by measuring length changes between mirrors in the arms of kilomet...
Interferometric gravitational wave detectors use mirrors whose substrates are formed from materials ...
Thermal noise arising from high-reflective mirror coatings limits the current ground-based gravitati...
Brownian thermal noise associated with highly reflective mirror coatings is a fundamental limit for ...
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...
We estimate the loss angles of the materials currently used in the highly reflective test-mass coati...