Mechanical loss in pendulums is a subject of great importance to gravitational waves detectors being built and being planned, as this determines the level of thermal noise associated with the detector suspensions. Relationships between the mechanical loss of the pendulum and the mechanical loss of the suspending fibres or wires can be derived in two apparently contradictory ways which give answers different by a factor of two. In this paper the differences are resolved and it is shown that both methods lead to the same answer
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
The thermal noise is expected to be one of the main limiting factors on the sensitivity of interfero...
The test masses of a large interferometric gravity wave detector (VIRGO project) will be controlled ...
For gravitational wave interferometers to work as planned, they must exhibit low levels of thermal n...
Detection of gravitational waves remains one of the most challenging problems faced by experimental ...
We present an analysis of the centrifugal coupling of a simple pendulum to a dissipative support. We...
The use of fused-silica ribbons as suspensions in gravitational wave interferometers can result in s...
The use of fused-silica ribbons as suspensions in gravitational wave interferometers can result in s...
From quality factor measurements we can estimate thermal noise using an analytical or numerical mo...
From quality factor measurements we can estimate thermal noise using an analytical or numerical mod...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
The displacement noise in the test-mass mirrors of interferometric gravitational wave detectors is p...
In this article we discuss theoretical and experimental investigations of the use of eddy-current da...
In this article we discuss theoretical and experimental investigations of the use of eddy-current da...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
The thermal noise is expected to be one of the main limiting factors on the sensitivity of interfero...
The test masses of a large interferometric gravity wave detector (VIRGO project) will be controlled ...
For gravitational wave interferometers to work as planned, they must exhibit low levels of thermal n...
Detection of gravitational waves remains one of the most challenging problems faced by experimental ...
We present an analysis of the centrifugal coupling of a simple pendulum to a dissipative support. We...
The use of fused-silica ribbons as suspensions in gravitational wave interferometers can result in s...
The use of fused-silica ribbons as suspensions in gravitational wave interferometers can result in s...
From quality factor measurements we can estimate thermal noise using an analytical or numerical mo...
From quality factor measurements we can estimate thermal noise using an analytical or numerical mod...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
The displacement noise in the test-mass mirrors of interferometric gravitational wave detectors is p...
In this article we discuss theoretical and experimental investigations of the use of eddy-current da...
In this article we discuss theoretical and experimental investigations of the use of eddy-current da...
Internal thermal noise is expected to be a limiting noise source in the most sensitive frequency ban...
The thermal noise is expected to be one of the main limiting factors on the sensitivity of interfero...
The test masses of a large interferometric gravity wave detector (VIRGO project) will be controlled ...