Seismic isolation enhancements for initial and Advanced LIGO

被引:51
作者
Abbott, R
Adhikari, R
Allen, G
Baglino, D
Campbell, C
Coyne, D
Daw, E
DeBra, D
Faludi, J
Fritschel, P
Ganguli, A
Giaime, J
Hammond, M
Hardham, C
Harry, G
Hua, W
Jones, L
Kern, J
Lantz, B
Lilienkamp, K
Mailand, K
Mason, K
Mittleman, R
Nayfeh, S
Ottaway, D
Phinney, J
Rankin, W
Robertson, N
Scheffler, R
Shoemaker, DH
Wen, S
Zucker, M
Zuo, L
机构
[1] CALTECH, LIGO Lab, Pasadena, CA 91125 USA
[2] MIT, LIGO Lab, Cambridge, MA 02139 USA
[3] Stanford Univ, Ginzton Lab, Stanford, CA 94305 USA
[4] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
[5] Stanford Univ, Dept Aeronaut & Astronaut, Stanford, CA 94305 USA
[6] LIGO Livingston Observ, Livingston, LA 70754 USA
关键词
D O I
10.1088/0264-9381/21/5/081
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A seismic isolation system for the proposed 'Advanced LIGO' detector upgrade is under development. It consists of a two-stage in-vacuum active isolation platform that is supported by an external hydraulic actuation stage. A full-scale preliminary-design technology demonstrator of the in-vacuum platform has been assembled and is being tested at Stanford's engineering test facility. Unanticipated excess ground motion from local human activity at LIGO Livingston has prompted accelerated development of the external stage for installation and use in the initial Livingston detector. As an interim measure, active external isolation in the laser beam direction is implemented using existing PZT external actuators.
引用
收藏
页码:S915 / S921
页数:7
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