Demonstration of a cavity coupler based on a resonant waveguide grating
- authored by
- Frank Brückner, Daniel Friedrich, Tina Clausnitzer, Oliver Burmeister, Michael Britzger, Ernst Bernhard Kley, Karsten Danzmann, Andreas Tünnermann, Roman Schnabel
- Abstract
Thermal noise in multilayer optical coatings may not only limit the sensitivity of future gravitational wave detectors in their most sensitive frequency band but is also a major impediment for experiments that aim to reach the standard quantum limit or to cool mechanical systems to their quantum ground state. Here, we present the experimental realization and characterization of a cavity coupler, which is based on a surface relief guided-mode resonant grating. Since the required thickness of the dielectric coating is dramatically decreased compared to conventional mirrors, it is expected to provide low mechanical loss and, thus, low thermal noise. The cavity coupler was incorporated into a Fabry-Perot resonator together with a conventional high quality mirror. The finesse of this cavity was measured to be F = 657, which corresponds to a coupler reflectivity of R = 99.08 %.
- Organisation(s)
-
Institute of Gravitation Physics
- External Organisation(s)
-
Friedrich Schiller University Jena
Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
- Type
- Article
- Journal
- Optics express
- Volume
- 17
- Pages
- 163-169
- No. of pages
- 7
- ISSN
- 1094-4087
- Publication date
- 05.01.2009
- Publication status
- Published
- Peer reviewed
- Yes
- ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics
- Electronic version(s)
-
https://doi.org/10.1364/OE.17.000163 (Access:
Open)