Seismic isolation for Advanced LIGO

被引：54

作者：

Abbott, R

Adhikari, R

Allen, G

Cowley, S

Daw, E

DeBra, D

Giaime, J ^{[1
]}

Hammond, G

Hammond, M

Hardham, C

How, J

Hua, W

Johnson, W

Lantz, B

Mason, K

Mittleman, R

Nichol, J

Richman, S

Rollins, J

Shoemaker, D

Stapfer, G

Stebbins, R

机构：

[1] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA

[2] Stanford Univ, Ginzton Lab, Stanford, CA 94305 USA

[3] MIT, LIGO Lab, Cambridge, MA 02139 USA

[4] Stanford Univ, Dept Aeronaut & Astronaut, Stanford, CA 94305 USA

[5] Univ Colorado, JILA, Boulder, CO 80303 USA

[6] LIGO Livingston Observ, Livingston, LA 70754 USA

来源：

CLASSICAL AND QUANTUM GRAVITY | 2002年 / 19卷 / 07期

关键词：

D O I：

10.1088/0264-9381/19/7/349

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The baseline design concept for a seismic isolation component of the proposed 'Advanced LIGO' detector upgrade has been developed with proof-of-principle experiments and computer models. It consists of a two-stage in-vacuum active isolation platform that is supported by an external hydraulic actuation stage. Construction is underway for prototype testing of a full-scale preliminary design.

引用

页码：1591 / 1597

页数：7