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Phys. Rev. D 81, 021101(R) (2010) [5 pages]

Charge management for gravitational-wave observatories using UV LEDs

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S. E. Pollack*, M. D. Turner, S. Schlamminger, C. A. Hagedorn, and J. H. Gundlach
Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA

Received 9 December 2009; published 21 January 2010

Accumulation of electrical charge on the end mirrors of gravitational-wave observatories can become a source of noise limiting the sensitivity of such detectors through electronic couplings to nearby surfaces. Torsion balances provide an ideal means for testing gravitational-wave technologies due to their high sensitivity to small forces. Our torsion pendulum apparatus consists of a movable plate brought near a plate pendulum suspended from a nonconducting quartz fiber. A UV LED located near the pendulum photoejects electrons from the surface, and a UV LED driven electron gun directs photoelectrons towards the pendulum surface. We have demonstrated both charging and discharging of the pendulum with equivalent charging rates of ∼105e/s, as well as spectral measurements of the pendulum charge resulting in a white noise level equivalent to 3×105e/√Hz.

© 2010 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.81.021101
DOI:
10.1103/PhysRevD.81.021101
PACS:
04.80.Nn, 07.10.Pz, 07.87.+v, 95.55.Ym

*Present address: Department of Physics and Astronomy and Rice Quantum Institute, Rice University, Houston, Texas 77251, USA.