Add to ORKGThe seismic isolation needed for LIGO-II will require a dramatic technological change from the passive systems used in the initial LIGO detector. To take advantage of the improved thermal noise of a 30 kg test mass made of high-Q material and suspended with fused silica fibers, one must attenuate the ground motion by more than 10 orders of magnitude at 10 Hz
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Mechanical Engineering, 2007.Includes...
New generations of gravity wave detectors require unprecedented levels of vibration isolation. This ...
Abstract. Both present LIGO and advanced LIGO (Ad-LIGO) will need an output mode cleaner (OMC) to re...
The seismic isolation needed for LIGO-II will require a dramatic technological change from the passi...
A seismic isolation system for the proposed 'Advanced LIGO' detector upgrade is under development. I...
The new generation of gravitational waves detectors require unprecedented levels of isolation from s...
Multiple-stage seismic vibration isolation stacks, which consist of alternating layers of stiff mass...
A new passive seismic attenuation system is being developed to replace the current passive attenuati...
The new generation of gravitational waves detectors require unprecedented levels of isolation from s...
New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave int...
In this chapter we describe the designs used for the suspension systems for Advanced LIGO and Advanc...
This paper presents the results of the past seven years of experimental investigation and testing do...
We describe the design of the suspension systems for the major optics for Advanced LIGO, the upgrade...
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
The detection of gravitational waves remains one of the most challenging prospects faced by experime...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Mechanical Engineering, 2007.Includes...
New generations of gravity wave detectors require unprecedented levels of vibration isolation. This ...
Abstract. Both present LIGO and advanced LIGO (Ad-LIGO) will need an output mode cleaner (OMC) to re...
The seismic isolation needed for LIGO-II will require a dramatic technological change from the passi...
A seismic isolation system for the proposed 'Advanced LIGO' detector upgrade is under development. I...
The new generation of gravitational waves detectors require unprecedented levels of isolation from s...
Multiple-stage seismic vibration isolation stacks, which consist of alternating layers of stiff mass...
A new passive seismic attenuation system is being developed to replace the current passive attenuati...
The new generation of gravitational waves detectors require unprecedented levels of isolation from s...
New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave int...
In this chapter we describe the designs used for the suspension systems for Advanced LIGO and Advanc...
This paper presents the results of the past seven years of experimental investigation and testing do...
We describe the design of the suspension systems for the major optics for Advanced LIGO, the upgrade...
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
The detection of gravitational waves remains one of the most challenging prospects faced by experime...
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Mechanical Engineering, 2007.Includes...
New generations of gravity wave detectors require unprecedented levels of vibration isolation. This ...
Abstract. Both present LIGO and advanced LIGO (Ad-LIGO) will need an output mode cleaner (OMC) to re...