Seismic noise is the major source of noise at frequencies below 100 Hz in current LIGO detectors. Thus, the suspension systems of future detectors must isolate this noise in order to increase their sensitivity; the design for the final stage suspension systems that actively damp and isolate seismic noise is the focus of this research. The design of our suspension system is composed of a double-double pendulum suspended from cantilever springs supported by a flexure stage. This stage contains piezoelectric actuators arranged so that the stage can be shaken in all three dimensions independently which simulates seismic noise with a controlled, large amplitude suitable of testing the isolation abilities of our suspension system. Early tests hav...
Low-mass suspension systems with high-Q pendulum stages are used to enable quantum radiation pressur...
Seismic noise limits Earth based gravitational wave interferometric detectors at low frequencies. Th...
The VIRGO SuperAttenuator is a complex six-degrees of freedom remote-controlled mechanism that isola...
In this chapter we describe the designs used for the suspension systems for Advanced LIGO and Advanc...
Seismic noise will be the dominant source of noise at low frequencies for ground based gravitational...
A seismic isolation system for the proposed 'Advanced LIGO' detector upgrade is under development. I...
In this article we describe aspects of the suspension system for each of the main optics (test masse...
Multiple-stage seismic vibration isolation stacks, which consist of alternating layers of stiff mass...
Below a few tens of hertz interferometric detection of gravitational waves is masked by seismic vibr...
An investigation of the use of mass-loaded piezoelectric accelerometers for active damping of high Q...
L'étude présentée porte sur le contrôle actif des supensions pour Advanced LIGO. LIGO est un projet ...
[[abstract]]To improve the performance of conventional seismic isolation technology, a semi-active i...
The gravitational wave detector VIRGO aims at extending the detection band down to a few Hertz by is...
The gravitational wave detector VIRGO aims at extending the detection band down to a few Hertz by is...
Low-mass suspension systems with high-Q pendulum stages are used to enable quantum radiation pressur...
Seismic noise limits Earth based gravitational wave interferometric detectors at low frequencies. Th...
The VIRGO SuperAttenuator is a complex six-degrees of freedom remote-controlled mechanism that isola...
In this chapter we describe the designs used for the suspension systems for Advanced LIGO and Advanc...
Seismic noise will be the dominant source of noise at low frequencies for ground based gravitational...
A seismic isolation system for the proposed 'Advanced LIGO' detector upgrade is under development. I...
In this article we describe aspects of the suspension system for each of the main optics (test masse...
Multiple-stage seismic vibration isolation stacks, which consist of alternating layers of stiff mass...
Below a few tens of hertz interferometric detection of gravitational waves is masked by seismic vibr...
An investigation of the use of mass-loaded piezoelectric accelerometers for active damping of high Q...
L'étude présentée porte sur le contrôle actif des supensions pour Advanced LIGO. LIGO est un projet ...
[[abstract]]To improve the performance of conventional seismic isolation technology, a semi-active i...
The gravitational wave detector VIRGO aims at extending the detection band down to a few Hertz by is...
The gravitational wave detector VIRGO aims at extending the detection band down to a few Hertz by is...
Low-mass suspension systems with high-Q pendulum stages are used to enable quantum radiation pressur...
Seismic noise limits Earth based gravitational wave interferometric detectors at low frequencies. Th...
The VIRGO SuperAttenuator is a complex six-degrees of freedom remote-controlled mechanism that isola...