How to reduce suspension thermal noise in LIGO without improving theQof the pendulum and violin modes
- 1 January 1999
- journal article
- Published by IOP Publishing in Measurement Science and Technology
- Vol. 10 (7) , 598-606
- https://doi.org/10.1088/0957-0233/10/7/305
Abstract
No abstract availableKeywords
All Related Versions
This publication has 9 references indexed in Scilit:
- Internal thermal noise in the LIGO test masses: A direct approachPhysical Review D, 1998
- Estimation of thermal noise in the mirrors of laser interferometric gravitational wave detectors: Two point correlation functionReview of Scientific Instruments, 1997
- Optical bars in gravitational wave antennasPhysics Letters A, 1997
- Energy dissipation in the pendulum mode of the test mass suspension of a gravitational wave antennaPhysics Letters A, 1996
- Brownian motion of a mass suspended by an anelastic wireThe Journal of the Acoustical Society of America, 1994
- LIGO: The Laser Interferometer Gravitational-Wave ObservatoryScience, 1992
- Thermal noise in mechanical experimentsPhysical Review D, 1990
- The VIRGO Project: A wide band antenna for gravitational wave detectionNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1990
- Irreversibility and Generalized NoisePhysical Review B, 1951