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Charge management for gravitational-wave observatories using UV LEDs

S. E. Pollack, M. D. Turner, S. Schlamminger, C. A. Hagedorn, and J. H. Gundlach
Phys. Rev. D 81, 021101(R) – Published 21 January 2010

Abstract

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.

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  • Received 9 December 2009

DOI:https://doi.org/10.1103/PhysRevD.81.021101

©2010 American Physical Society

Authors & Affiliations

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

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

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Vol. 81, Iss. 2 — 15 January 2010

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