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
- Published Version
See Usage Policy.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20110404-100247235
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.
|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.|
|Classification Code:||PACS: 04.80.Nn, 03.65.Ta, 42.50.Dv, 42.50.Lc|
|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.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||10 Apr 2011 01:22|
|Last Modified:||26 Dec 2012 13:08|
Repository Staff Only: item control page