We present for the first time the results of very high Q factor measurements for a 2.8 kg fused silica mass suspended by two fused quartz fibers attached by a novel technique for joining fused silica or quartz. The Q for the pendulum mode at 0.93 Hz was (2.3+/-0. 2)x10(7), the highest value demonstrated to date for a mass of this size. By employing such a new suspension system the sensitivity of the gravitational wave detectors currently under construction can be increased up to 1 order of magnitude
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
We present for the first time the results of very high Q factor measurements for a 2.8 kg fused sili...
The results of a very high Q factor measurements for a 2.8 kg fused silica mass suspended by two fus...
The results of a very high Q factor measurements for a 2.8 kg fused silica mass suspended by two fus...
Thermal noise in mirror suspension wires is the most severe limit to the low frequency sensitivity o...
Thermal noise in mirror suspension wires is the most severe limit to the low frequency sensitivity o...
To minimize thermal noise in gravitational-wave detectors high mechanical quality factors are requir...
High purity fused silica has become the cornerstone choice for use in the final monolithic stage of ...
High purity fused silica has become the cornerstone choice for use in the final monolithic stage of ...
A series of measurements were undertaken to measure the quality factor of a full scale prototype of ...
High Q mirror suspensions are a key element of the advanced interferometric gravitational-wave detec...
Thermal noise from the suspension fibers used in the mirror pendulums in current gravitational-wave ...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
We present for the first time the results of very high Q factor measurements for a 2.8 kg fused sili...
The results of a very high Q factor measurements for a 2.8 kg fused silica mass suspended by two fus...
The results of a very high Q factor measurements for a 2.8 kg fused silica mass suspended by two fus...
Thermal noise in mirror suspension wires is the most severe limit to the low frequency sensitivity o...
Thermal noise in mirror suspension wires is the most severe limit to the low frequency sensitivity o...
To minimize thermal noise in gravitational-wave detectors high mechanical quality factors are requir...
High purity fused silica has become the cornerstone choice for use in the final monolithic stage of ...
High purity fused silica has become the cornerstone choice for use in the final monolithic stage of ...
A series of measurements were undertaken to measure the quality factor of a full scale prototype of ...
High Q mirror suspensions are a key element of the advanced interferometric gravitational-wave detec...
Thermal noise from the suspension fibers used in the mirror pendulums in current gravitational-wave ...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
Detection of gravitational waves from astrophysical sources remains one of the most challenging prob...