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  White-light cavities, atomic phase coherence, and gravitational wave detectors

Wicht, A., Danzmann, K., Fleischhauer, M., Scully, M., Müller, G., & Rinkleff, R.-H. (1997). White-light cavities, atomic phase coherence, and gravitational wave detectors. Optics Communications, 134(1-6), 431-439. doi:10.1016/S0030-4018(96)00579-2.

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372445.pdf (Publisher version), 802KB
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Wicht, A.1, Author
Danzmann, Karsten2, Author           
Fleischhauer, M., Author
Scully, M., Author
Müller, G., Author
Rinkleff, Rolf-Hermann2, 3, Author
Affiliations:
1External Organizations, ou_persistent13              
2Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              
3AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24009              

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 Abstract: We propose a new concept to realize optical cavities with large buildup but broadband response (white-light cavities) using atomic phase coherence. We demonstrate that strongly driven double-Λ systems can show negative dispersion without absorption, which is needed in order to compensate for the variation of the wavelength with frequency. Internal buildup profiles and the cavity bandwidth of standard devices and white-light cavities will be briefly compared. These devices may be useful to improve the bandwidth and sensitivity of future generations of laser interferometric gravitational wave detectors.

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 Dates: 1997-01
 Publication Status: Issued
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 Identifiers: eDoc: 372445
DOI: 10.1016/S0030-4018(96)00579-2
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Title: Optics Communications
Source Genre: Journal
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Pages: - Volume / Issue: 134 (1-6) Sequence Number: - Start / End Page: 431 - 439 Identifier: ISSN: 0030-4018