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Coherent coupling completing an unambiguous optomechanical classification framework

Li, Xiang and Korobko, Mikhail and Ma, Yiqiu and Schnabel, Roman and Chen, Yanbei (2019) Coherent coupling completing an unambiguous optomechanical classification framework. Physical Review A, 100 (5). Art. No. 053855. ISSN 2469-9926. doi:10.1103/physreva.100.053855. https://resolver.caltech.edu/CaltechAUTHORS:20191125-143133452

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Abstract

In most optomechanical systems, a movable mirror is a part of an optical cavity, and its oscillation modulates either the resonance frequency of the cavity or its coupling to the environment. There exists the third option—which we call a “coherent coupling”—when the mechanical oscillation couples several nondegenerate optical modes supported by the cavity. Identifying the nature of the coupling can be an important step in designing the setup for a specific application. In order to unambiguously distinguish between different optomechanical couplings, we develop a general framework based on the Hamiltonian of the system. Using this framework, we give examples of different couplings and discuss in details one particular case of a purely coherent coupling in a ring cavity with a movable mirror inside. We demonstrate that in certain cases coherent coupling can be beneficial for cooling the motion of the mechanical oscillator. Our general framework allows us to approach the design of optomechanical experiments in a methodological way, for precise exploitation of the strengths of particular optomechanical couplings.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/physreva.100.053855DOIArticle
https://arxiv.org/abs/1908.03372arXivDiscussion Paper
ORCID:
AuthorORCID
Li, Xiang0000-0002-3780-7735
Korobko, Mikhail0000-0002-3839-3909
Ma, Yiqiu0000-0001-7192-4874
Schnabel, Roman0000-0003-2896-4218
Chen, Yanbei0000-0002-9730-9463
Additional Information:© 2019 American Physical Society. Received 28 August 2019; published 25 November 2019. We thank Farid Khalili for useful discussions. The work of X.L., Y.M., and Y.C. are supported by the National Science Foundation through Grants No. PHY-1612816, No. PHY-1708212, and No. PHY-1708213; the Brinson Foundation; and the Simons Foundation (Award No. 568762). The work of M.K. and R.S. was supported by the Deutsche Forschungsgemeinschaft (DFG) (No. SCHN 757/6-1).
Group:TAPIR, Astronomy Department
Funders:
Funding AgencyGrant Number
NSFPHY-1612816
NSFPHY-1708212
NSFPHY-1708213
Brinson FoundationUNSPECIFIED
Simons Foundation568762
Deutsche Forschungsgemeinschaft (DFG)SCHN 757/6-1
Issue or Number:5
DOI:10.1103/physreva.100.053855
Record Number:CaltechAUTHORS:20191125-143133452
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191125-143133452
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:100043
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:25 Nov 2019 23:13
Last Modified:16 Nov 2021 17:51

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