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Negative optical inertia for enhancing the sensitivity of future gravitational-wave detectors

Khalili, Farid and Danilishin, Stefan and Müeller-Ebhardt, Helge and Miao, Haixing and Chen, Yanbei and Zhao, Chunnong (2011) Negative optical inertia for enhancing the sensitivity of future gravitational-wave detectors. Physical Review D, 83 (6). Art. No. 062003. ISSN 0556-2821. http://resolver.caltech.edu/CaltechAUTHORS:20110404-100247235

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Abstract

We consider enhancing the sensitivity of future gravitational-wave detectors by using double optical spring. When the power, detuning and bandwidth of the two carriers are chosen appropriately, the effect of the double optical spring can be described as a “negative inertia,” which cancels the positive inertia of the test masses and thus increases their response to gravitational waves. This allows us to surpass the free-mass standard quantum limit (SQL) over a broad frequency band, through signal amplification, rather than noise cancellation, which has been the case for all broadband SQL-beating schemes so far considered for gravitational-wave detectors. The merit of such signal amplification schemes lies in the fact that they are less susceptible to optical losses than noise-cancellation schemes. We show that it is feasible to demonstrate such an effect with the Gingin High Optical Power Test Facility, and it can eventually be implemented in future advanced GW detectors.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1103/PhysRevD.83.062003DOIArticle
http://link.aps.org/doi/10.1103/PhysRevD.83.062003PublisherArticle
http://prd.aps.org/abstract/PRD/v83/i6/e062003PublisherArticle
Additional Information:© 2011 American Physical Society. Received 6 October 2010; published 16 March 2011. We thank all our colleagues in the LIGO Macroscopic-Quantum-Mechanics (MQM) group for fruitful discussions. F. K.'s and S. D.'s research have been supported by the Russian Foundation for Basic Research Grant No. 08-02-00580-a. S. D., H. M.-E., and Y. C. are supported by the Alexander von Humboldt Foundation’s Sofja Kovalevskaja Programme, NSF Grant Nos. PHY-0653653 and PHY-0601459, as well as the David and Barbara Groce startup fund at Caltech. H. M. and C. Z. have been supported by the Australian Research Council.
Group:TAPIR
Funders:
Funding AgencyGrant Number
Russian Foundation for Basic Research 08-02-00580-a
Alexander von Humboldt Foundation Sofja Kovalevskaja ProgrammeUNSPECIFIED
NSFPHY-0653653
NSFPHY-0601459
Caltech David and Barbara Groce Startup FundUNSPECIFIED
Australian Research CouncilUNSPECIFIED
Classification Code:PACS: 04.80.Nn, 03.65.Ta, 42.50.Dv, 42.50.Lc
Record Number:CaltechAUTHORS:20110404-100247235
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20110404-100247235
Official Citation:Negative optical inertia for enhancing the sensitivity of future gravitational-wave detectors Farid Khalili, Stefan Danilishin, Helge Müller-Ebhardt, Haixing Miao, Yanbei Chen, and Chunnong Zhao Published 16 March 2011 (7 pages) 062003
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:23222
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:10 Apr 2011 01:22
Last Modified:01 Nov 2017 23:35

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