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Phys. Rev. Lett. 98, 150802 (2007) [4 pages]

An All-Optical Trap for a Gram-Scale Mirror

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Thomas Corbitt1, Yanbei Chen2, Edith Innerhofer1, Helge Müller-Ebhardt3, David Ottaway1, Henning Rehbein3, Daniel Sigg4, Stanley Whitcomb5, Christopher Wipf1, and Nergis Mavalvala1
1LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
2Max-Planck-Institut für Gravitationsphysik, Am Mühlenberg 1, 14476 Potsdam, Germany
3Max-Planck-Institut für Gravitationsphysik (Albert Einstein Institute), Callinstraße 38, 30167 Hannover, Germany
4LIGO Hanford Observatory, Route 10, Mile marker 2, Hanford, Washington 99352, USA
5LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA

Received 23 January 2007; published 13 April 2007

We report on a stable optical trap suitable for a macroscopic mirror, wherein the dynamics of the mirror are fully dominated by radiation pressure. The technique employs two frequency-offset laser fields to simultaneously create a stiff optical restoring force and a viscous optical damping force. We show how these forces may be used to optically trap a free mass without introducing thermal noise, and we demonstrate the technique experimentally with a 1 g mirror. The observed optical spring has an inferred Young’s modulus of 1.2 TPa, 20% stiffer than diamond. The trap is intrinsically cold and reaches an effective temperature of 0.8 K, limited by technical noise in our apparatus.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.98.150802
DOI:
10.1103/PhysRevLett.98.150802
PACS:
07.10.Cm, 04.80.Nn