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Charge measurement and mitigation for the main test masses of the GEO 600 gravitational wave observatory

M Hewitson et al 2007 Class. Quantum Grav. 24 6379-6391   doi: 10.1088/0264-9381/24/24/013  Help

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M Hewitson1, K Danzmann1, H Grote1, S Hild1, J Hough2, H Lück1, S Rowan2, J R Smith1, K A Strain1,2 and B Willke1
1 Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) und Universität Hannover, Außenstelle Hannover, Callinstr 38, 30167 Hannover, Germany
2 Department of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, UK
E-mail: martin.hewitson@aei.mpg.de

Abstract. Spurious charging of the test masses in gravitational wave interferometers is a well-known problem. Typically, concern arises due to the possibility of increased thermal noise due to a lowering of the quality factor of modes of the test-mass suspension, or due to the potential for increased displacement noise arising from charge migration on the surface of the test masses. Recent experience gained at the GEO 600 gravitational wave detector has highlighted an additional problem. GEO 600 uses electrostatic actuators to control the longitudinal position of the main test masses. The presence of charge on the test masses is shown to strongly affect the performance of the electrostatic actuators. This paper reports on a measurement scheme whereby the charge state of the GEO 600 test masses can be measured using the electrostatic actuators. The resulting measurements are expressed in terms of an effective bias voltage on the electrostatic actuators. We also describe attempts to remove the charge from the test masses and we show that the use of UV illumination was the most successful. Using UV illumination we were able to discharge and re-charge the test masses.

PACS numbers: 95.55.Ym, 04.80.Nn

Print publication: Issue 24 (21 December 2007)
Received 15 August 2007, in final form 5 November 2007
Published 29 November 2007

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