Squeezed light at sideband frequencies below 100 kHz from a single OPA
Abstract
Quantum noise of the electromagnetic field is one of the limiting noise sources in interferometric gravitational wave detectors. Shifting the spectrum of squeezed vacuum states downwards into the acoustic band of gravitational wave detectors is therefore of challenging demand to quantum optics experiments. We demonstrate a system that produces nonclassical continuous variable states of light that are squeezed at sideband frequencies below 100 kHz. A single optical parametric amplifier (OPA) is used in an optical noise cancellation scheme providing squeezed vacuum states with coherent bright phase modulation sidebands at higher frequencies. The system has been stably locked to a reference laser beam for half an hour limited by thermal stability of our laboratory.
- Publication:
-
Optics Communications
- Pub Date:
- October 2004
- DOI:
- arXiv:
- arXiv:quant-ph/0402064
- Bibcode:
- 2004OptCo.240..185S
- Keywords:
-
- Gravitational wave detectors;
- Squeezed states;
- 04.80.Nn;
- 42.50.Dv;
- 42.65.Yj;
- Gravitational wave detectors and experiments;
- Nonclassical states of the electromagnetic field including entangled photon states;
- quantum state engineering and measurements;
- Optical parametric oscillators and amplifiers;
- Quantum Physics
- E-Print:
- 3 pages, 3 figures