Systematic and quantitative analysis of residual amplitude modulation in Pound-Drever-Hall frequency stabilization
- 7 December 2015
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review A
- Vol. 92 (6), 063809
- https://doi.org/10.1103/physreva.92.063809
Abstract
We theoretically analyze the effects of two primary mechanisms of residual amplitude modulation, estimate the resulting frequency instabilities, and discuss relevant experimental countermeasures, providing useful information that are beneficial for the development of ultrastable optical oscillators as well as many precision experiments relying on stable lasers. A Pound-Drever-Hall signal comprising contributions from the birefringence of the electro-optic crystal is derived and used to examine the birefringence-related amplitude modulation and the resultant frequency offset in terms of various experimental parameters. The combined effect of the crystal birefringence and pararsitic étalons is further investigated by dividing the étalons into three representative categories according to their locations in the optical path. The analysis shows that introducing a resonant optical cavity only scales the birefringence-generated amplitude modulation by a constant, thereby lending strong support to the active control scheme using a separate detection path. When a parasitic étalon is added, the active control scheme can still suppress the resultant instability except for the parasitic étalon that is located closely in front of the optical cavity. In this case the étalon produces rather large frequency instability and therefore should be avoided. In addition, numerical calculations are performed to assess the impact of a special situation where the front and end surfaces of an ultrastable optical cavity are potential sources of the parasitic étalon that can strongly couple with the cavity.Keywords
Funding Information
- National Natural Science Foundation of China (11235004, 11327407)
This publication has 45 references indexed in Scilit:
- Towards a gravitational wave observatory designer: sensitivity limits of spaceborne detectorsClassical and Quantum Gravity, 2015
- Accelerated Gravitational Wave Parameter Estimation with Reduced Order ModelingPhysical Review Letters, 2015
- Advanced Virgo: a second-generation interferometric gravitational wave detectorClassical and Quantum Gravity, 2014
- Improved Upper Limits on the Stochastic Gravitational-Wave Background from 2009–2010 LIGO and Virgo DataPhysical Review Letters, 2014
- Gravitational radiation detection with laser interferometryReviews of Modern Physics, 2014
- Virgo: a laser interferometer to detect gravitational wavesJournal of Instrumentation, 2012
- A gravitational wave observatory operating beyond the quantum shot-noise limitNature Physics, 2011
- Laser interferometry for the detection of gravitational wavesJournal of Optics A: Pure and Applied Optics, 2005
- An introduction to signal extraction in interferometric gravitational wave detectorsAmerican Journal of Physics, 2003
- Laser phase and frequency stabilization using an optical resonatorApplied Physics B Laser and Optics, 1983