The GEO 600 gravitational wave detector

被引：277

作者：

Willke, B

Aufmuth, P

Aulbert, C

Babak, S

Balasubramanian, R

Barr, BW

Berukoff, S

Bose, S

Cagnoli, G

Casey, MM

Churches, D

Clubley, D

Colacino, CN

Crooks, DRM

Cutler, C

Danzmann, K

Davies, R

Dupuis, R

Elliffe, E

Fallnich, C

Freise, A

Gossler, S

Grant, A

Grote, H

Heinzel, G

Heptonstall, A

Heurs, M

Hewitson, M

Hough, J

Jennrich, O

Kawabe, K

Kötter, K

Leonhardt, V

Lück, H

Malec, M

McNamara, PW

McIntosh, SA

Mossavi, K

Mohanty, S

Mukherjee, S

Nagano, S

Newton, GP

Owen, BJ

Palmer, D

Papa, MA

Plissi, MV

Quetschke, V

Robertson, DI

Robertson, NA

Rowan, S

机构：

[1] Leibniz Univ Hannover, Inst Atom & Mol Phys, D-30167 Hannover, Germany

[2] Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland

[3] Max Planck Inst Gravitat Phys, Albert Einstein Inst, Aussenstelle Hannover, D-30167 Hannover, Germany

[4] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany

[5] Cardiff Univ, Dept Phys & Astron, Cardiff CF2 3YB, S Glam, Wales

[6] Laser Zentrum Hannover eV, D-30419 Hannover, Germany

[7] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

来源：

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

关键词：

D O I：

10.1088/0264-9381/19/7/321

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The GEO 600 laser interferometer with 600 m armlength is part of a worldwide network of gravitational wave detectors. Due to the use of advanced technologies like multiple pendulum suspensions with a monolithic last stage and signal recycling, the anticipated sensitivity of GEO 600 is close to the initial sensitivity of detectors with several kilometres armlength. This paper describes the subsystems of GEO 600, the status of the detector by September 2001 and the plans towards the first science run.

引用

页码：1377 / 1387

页数：11

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