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Residual amplitude modulation in interferometric gravitational wave detectors

Kokeyama, Keiko and Izumi, Kiwamu and Korth, William Z. and Smith-Lefebvre, Nicolas and Arai, Koji and Adhikari, Rana X. (2014) Residual amplitude modulation in interferometric gravitational wave detectors. Journal of the Optical Society of America A, 31 (1). pp. 81-88. ISSN 1084-7529. http://resolver.caltech.edu/CaltechAUTHORS:20140129-105348434

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Abstract

The effects of residual amplitude modulation (RAM) in laser interferometers using heterodyne sensing can be substantial and difficult to mitigate. In this work, we analyze the effects of RAM on a complex laser interferometer used for gravitational wave detection. The RAM introduces unwanted offsets in the cavity length signals and thereby shifts the operating point of the optical cavities from the nominal point via feedback control. This shift causes variations in the sensing matrix, and leads to degradation in the performance of the precision noise subtraction scheme of the multiple-degree-of-freedom control system. In addition, such detuned optical cavities produce an optomechanical spring, which also perturbs the sensing matrix. We use our simulations to derive requirements on RAM for the Advanced LIGO (aLIGO) detectors, and show that the RAM expected in aLIGO will not limit its sensitivity.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1364/JOSAA.31.000081DOIArticle
http://www.opticsinfobase.org/josaa/abstract.cfm?uri=josaa-31-1-81PublisherArticle
http://arxiv.org/abs/1309.4522arXivDiscussion Paper
ORCID:
AuthorORCID
Korth, William Z.0000-0003-3527-1348
Adhikari, Rana X.0000-0002-5731-5076
Additional Information:© 2013 Optical Society of America. Received September 19, 2013; revised November 8, 2013; accepted November 10, 2013; posted November 11, 2013 (Doc. ID 197967); published December 10, 2013. We thank the reviewers for their detailed and perceptive commentary. We would like to thank Peter Fritschel and Gabriela Gonzalez for their comments on an early version of the manuscript and our colleagues at the LIGO Livingston Observatory for sharing with us their experiences with RAM over long periods of time. KK was supported by the National Science Foundation with awards 0905184 and 1205882. We also gratefully acknowledge the National Science Foundation for their support under grant PHY-0555406.
Group:LIGO
Funders:
Funding AgencyGrant Number
NSFPHY-0905184
NSFPHY-1205882
NSFPHY-0555406
Classification Code:(040.0040) Detectors; (120.0120) Instrumentation, measurement, and metrology; (120.5060) Phase modulation; (140.0140) Lasers and laser optics
Record Number:CaltechAUTHORS:20140129-105348434
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140129-105348434
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:43547
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:29 Jan 2014 21:42
Last Modified:21 Nov 2017 21:35

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