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Fabrication And Characterization Of Photonic Crystal Slow Light Waveguides And Cavities
Published on: November 30, 2012
Experimental demonstration of a suspended diffractively coupled optical cavity
M P Edgar1, B W Barr, J Nelson
11Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, UK. m.edgar@physics.gla.ac.uk
Optics Letters
|October 20, 2009
Summary
Future gravitational wave detectors may use all-reflective optics. This study demonstrates a suspended diffractive coupled cavity using gratings as input couplers, controlled with Pound-Drever-Hall techniques for stable operation.
Area of Science:
- Optical Physics
- Gravitational Wave Astronomy
- Interferometry
Background:
- Advanced gravitational wave detectors require novel optical configurations.
- All-reflective optical systems offer potential advantages for future detector designs.
- Diffraction gratings are being explored as input couplers for Fabry-Perot cavities in these systems.
Purpose of the Study:
- To experimentally demonstrate a fully suspended diffractive coupled cavity.
- To investigate the applicability of Pound-Drever-Hall techniques for controlling such cavities.
- To assess the feasibility of using diffraction gratings in gravitational wave detector topologies.
Main Methods:
- Construction and suspension of a diffractive coupled cavity.
- Implementation of Pound-Drever-Hall length sensing and control.
- Experimental validation of cavity stability and operating conditions.
Main Results:
- Successful experimental demonstration of a fully suspended diffractive coupled cavity.
- Validation of conventional Pound-Drever-Hall techniques for length sensing and control in this system.
- Confirmation of the potential for using diffractive optics in gravitational wave detectors.
Conclusions:
- Diffractively coupled cavities are experimentally feasible for gravitational wave detector applications.
- Pound-Drever-Hall techniques are effective for stabilizing these novel optical systems.
- This work supports the development of all-reflective optical systems for future gravitational wave observatories.

