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Full modal simulation of opto-mechanical effects in optical systems

Vajente, Gabriele (2014) Full modal simulation of opto-mechanical effects in optical systems. Classical and Quantum Gravity, 31 (7). Art. No. 075005. ISSN 0264-9381. http://resolver.caltech.edu/CaltechAUTHORS:20140425-092252942

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Abstract

The interaction of light with optical elements via radiation pressure plays a predominant role in determining the dynamics of many optical configurations, in particular when the mirrors composing the system have small masses or the light power is large. Gravitational wave interferometric detectors fall in the second category: opto-mechanical effects have been measured in first generation instruments and will be very relevant in second and third generations. So far, radiation pressure effects were studied using analytical models or simulation tools which were limited to specific optical systems or low order Hermite–Gauss modes. In this paper we present the first tool, to our knowledge, capable of a complete Hermite–Gauss modal simulation of radiation pressure induced effects, based on the modal interferometer simulation toolbox (MIST), described in details in a previous paper. This tool opens the possibility of the simulation of radiation pressure effects in realistic interferometric systems that include beam and optical element aberrations. The application of this tool to gravitational wave detectors will allow to better understand the incidence of realistic optical defects on the instrument operation and sensitivity. We also expect that this tool will be useful outside the gravitational wave community, for application on interferometric systems where radiation pressure dynamics is dominant, such as opto-mechanically-induced transparency, light mirror cavities and membrane-in-a-cavity systems. In this paper we describe the formalism used to implement radiation pressure in the MIST simulation tool and we give some example applications, including the first results on parametric instabilities in Fabry–Perot cavities based on a complete modal optical simulation.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0264-9381/31/7/075005DOIArticle
http://iopscience.iop.org/0264-9381/31/7/075005/PublisherArticle
Additional Information:© 2014 IOP Publishing Ltd. Received 5 December 2013; revised 28 January 2014; Accepted for publication 7 February 2014; Published 5 March 2014 The author is grateful to R. Day (EGO), J. Marque (former EGO), A. Chiummo (EGO), B. Swinkels (EGO), E. Calloni (INFN Napoli) and M. Evans (MIT) for many useful discussion on the topic of radiation pressure effects. This research activity has been partially supported by Regione Toscana (Italy) through the program POR CreO FSE 2007–2013 of the European Community, within the project no. 18113 (ISAV). LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the United States National Science Foundation under grant PHY-0757058.
Funders:
Funding AgencyGrant Number
European Community Regione Toscana (Italy) POR CreO FSE 2007-201318113 (ISAV)
NSFPHY-0757058
Subject Keywords:optical simulation; radiation pressure; gravitational wave detectors
Classification Code:PACS: 42.60.Da, 04.80.Nn, 07.05.Tp, 07.60.Ly
Record Number:CaltechAUTHORS:20140425-092252942
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20140425-092252942
Official Citation:Full modal simulation of opto-mechanical effects in optical systems Gabriele Vajente 2014 Class. Quantum Grav. 31 075005
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:45219
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:25 Apr 2014 17:52
Last Modified:25 Apr 2014 17:52

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