An All-Optical Trap for a Gram-Scale Mirror
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- 13 April 2007
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 98 (15) , 150802
- https://doi.org/10.1103/physrevlett.98.150802
Abstract
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.Keywords
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This publication has 16 references indexed in Scilit:
- Radiation Pressure Cooling of a Micromechanical Oscillator Using Dynamical BackactionPhysical Review Letters, 2006
- Self-cooling of a micromirror by radiation pressureNature, 2006
- Radiation-pressure cooling and optomechanical instability of a micromirrorNature, 2006
- Sub-kelvin optical cooling of a micromechanical resonatorNature, 2006
- Cooling a nanomechanical resonator with quantum back-actionNature, 2006
- Measurement of optical response of a detuned resonant sideband extraction gravitational wave detectorPhysical Review D, 2006
- Squeezed-state source using radiation-pressure-induced rigidityPhysical Review A, 2006
- Cavity cooling of a microleverNature, 2004
- Low quantum noise tranquilizer for Fabry–Perot interferometerPhysics Letters A, 2002
- Signal recycled laser-interferometer gravitational-wave detectors as optical springsPhysical Review D, 2002