The Geo 600 Gravitational Wave Detector: Pulsar Prospects

G Woan, P Aufmuth,C Aulbert,S Babak,R Balasubramanian,Bw Barr,S Berukoff,S Bose,G Cagnoli,Mm Casey,D Churches,Cn Colacino,Drm Crooks,C Cutler,K Danzmann,R Davies,Rj Dupuis,E Elliffe,C Fallnich,A Freise,S Gossler,A Grant,H Grote,G Heinzel,A Hepstonstall,M Heurs,M Hewitson,J Hough,O Jennrich,K Kawabe,K Kotter,V Leonhardt, H Luck,M Malec, Pw Mcnamara,K Mossavi,S Mohanty,S Mukherjee,S Nagano,Gp Newton,Bj Owen,Ma Papa,Mv Plissi,V Quetschke,Di Robertson,Na Robertson,S Rowan,A Rudiger,Bs Sathyaprakash, R Schilling,Bf Schutz, R Senior,Am Sintes,Kd Skeldon,P Sneddon, F Stief,Ka Strain,I Taylor,Ci Torrie, A Vecchio,H Ward,U Weiland,H Welling,P Williams,W Winkler,B Willke,I Zawischa

RADIO PULSARS, PROCEEDINGS（2003）

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摘要

The GEO 600 laser-interferometric gravitational wave detector near Hannover, Germany, is one of six such interferometers now close to operation worldwide. The UK/German GEO collaboration uses advanced technologies, including monolithic silica suspensions and signal recycling, to deliver a sensitivity comparable with much larger detectors in their initial configurations. Here we review the design and performance of GEO 600 and consider the prospects for a direct detection of continuous gravitational waves from spinning neutron stars.

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