Status of GEO 600

被引：89

作者：

Willke, B

Aufmuth, P

Aulbert, C

Babak, S

Balasubramanian, R

Barr, BW

Berukoff, S

Cagnoli, G

Cantley, CA

Casey, MM

Chelkowski, S

Churches, D

Colacino, CN

Crooks, DRM

Cutler, C

Danzmann, K

Davies, R

Dupuis, RJ

Elliffe, E

Fallnich, C

Freise, A

Gossler, S

Grant, A

Grote, H

Grunewald, S

Harms, J

Heinzel, G

Heng, IS

Hepstonstall, A

Heurs, M

Hewitson, M

Hild, S

Hough, J

Ingley, R

Itoh, Y

Jennrich, O

Jones, R

Hutter, SH

Kawabe, K

Killow, C

Kötter, K

Krishnan, B

Leonhardt, V

Lück, H

Machenschalk, B

Malec, M

Mercer, RA

Messenger, C

Mohanty, S

Mossavi, K

机构：

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

[2] Leibniz Univ Hannover, D-30167 Hannover, Germany

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

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

[5] Univ Glasgow, Dept Phys & Astron, Glasgow G12 8QQ, Lanark, Scotland

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

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

[8] Univ Illes Balears, Dept Fis, E-07122 Palma de Mallorca, Spain

来源：

CLASSICAL AND QUANTUM GRAVITY | 2004年 / 21卷 / 05期

关键词：

D O I：

10.1088/0264-9381/21/5/006

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 currently being commissioned as a part of a worldwide network of gravitational wave detectors. Due to the use of advanced technologies such as signal recycling and multiple pendulum suspensions with a monolithic last stage the anticipated sensitivity of GEO 600 is close to the initial sensitivity of km baseline detectors. This paper describes the status of the detector as of November 2003 with special emphasis on its performance during the first serious data-taking periods and on the experimental challenges encountered during the commissioning of the dual-recycled detector.

引用

页码：S417 / S423

页数：7

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