This conference presentation was prepared for the Quantum Technology: Driving Commercialisation of an Enabling Science III conference at SPIE Photonex, 2022.
Norna Robertson, Benjamin Abbott, R. Abbott, R. Adhikari, Graham Allen, Helena Armandula, Stuart Aston, A. Baglino, Mark Barton, B. Bland, Rolf Bork, J. Bogenstahl, Gianpietro Cagnoli, C. Campbell, C. Cantley, K. Carter, D. Cook, D. Coyne, David Crooks, Edward Daw, Daniel DeBra, E. Elliffe, J. Faludi, Peter Fritschel, A. Ganguli, Joseph Giaime, S. Gossler, A. Grant, J. Greenhalgh, M. Hammond, Jonathan Hanson, C. Hardham, Gregory Harry, Alistair Heptonstall, Jay Heefner, James Hough, D. Hoyland, Wensheng Hua, L. Jones, R. Jones, Jonathan Kern, J. LaCour, Brian Lantz, K. Lilienkamp, N. Lockerbie, Harald Lueck, M. MacInnis, K. Mailand, Ken Mason, R. Mittleman, Samir Nayfeh, J. Nichol, David Ottaway, H. Overmier, M. Perreur-Lloyd, J. Phinney, M. Plissi, W. Rankin, D. Robertson, J. Romie, Sheila Rowan, R. Scheffler, David Shoemaker, P. Sarin, Peter Sneddon, Clive Speake, O. Spjeld, G. Stapfer, Kenneth Strain, C. Torrie, G. Traylor, J. van Niekerk, Alberto Vecchio, Shirong Wen, P. Willems, I. Wilmut, Harry Ward, M. Zucker, Lei Zuo
To meet the overall isolation and alignment requirements for the optics in Advanced LIGO, the planned upgrade to LIGO, the US laser interferometric gravitational wave observatory, we are developing three sub-systems: a hydraulic external pre-isolator for low frequency alignment and control, a two-stage active isolation platform designed to give a factor of ~1000 attenuation at 10 Hz, and a multiple pendulum suspension system that provides passive isolation above a few hertz. The hydraulic stage uses laminar-flow quiet hydraulic actuators with millimeter range, and provides isolation and alignment for the optics payload below 10 Hz, including correction for measured Earth tides and the microseism. This stage supports the in-vacuum two-stage active isolation platform, which reduces vibration using force feedback from inertial sensor signals in six degrees of freedom. The platform provides a quiet, controlled structure to mount the suspension system. This latter system has been developed from the triple pendulum suspension used in GEO 600, the German/UK gravitational wave detector. To meet the more stringent noise levels required in Advanced LIGO, the baseline design for the most sensitive optics calls for a quadruple pendulum, whose final stage consists of a 40 kg sapphire mirror suspended on fused silica ribbons to reduce suspension thermal noise.
William Hamilton, Marc Burgamy, Daniel Busby, Edward Daw, J. Duran, Joseph Giaime, Jonathan Hanson, Ik Heng, Warren Johnson, Martin McHugh, Phillip Miller, Damon Nettles, J. Whelan
Resonant gravitational wave detectors are described. Examples are given for signal improvement by combining signals from several independent detectors. The successful test run of Allegro in coincidence with LIGO Livingston during an engineering run (E7) is also described.
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