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authorEugeniy Mikhailov <evgmik@gmail.com>2012-03-29 11:59:49 -0400
committerEugeniy Mikhailov <evgmik@gmail.com>2012-03-29 11:59:49 -0400
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@@ -4750,3 +4750,20 @@ eprint = {http://www.tandfonline.com/doi/pdf/10.1080/09500340903159495}
see additional noise from the light-atom interaction.}
}
+@article{schnabel2005pra_squeezing_control,
+ title = {Experimental characterization of frequency-dependent squeezed light},
+ author = {Chelkowski, Simon and Vahlbruch, Henning and Hage, Boris and Franzen, Alexander and Lastzka, Nico and Danzmann, Karsten and Schnabel, Roman},
+ journal = {Phys. Rev. A},
+ month = {Jan},
+ url = {http://link.aps.org/doi/10.1103/PhysRevA.71.013806},
+ doi = {10.1103/PhysRevA.71.013806},
+ volume = {71},
+ year = {2005},
+ issue = {1},
+ publisher = {American Physical Society},
+ numpages = {8},
+ pages = {013806},
+ abstract = {
+ We report on the demonstration of broadband squeezed laser beams that show a frequency-dependent orientation of the squeezing ellipse. Carrier frequency as well as quadrature angle were stably locked to a reference laser beam at 1064 nm. This frequency-dependent squeezing was characterized in terms of noise power spectra and contour plots of Wigner functions. The latter were measured by quantum state tomography. Our tomograph allowed a stable lock to a local oscillator beam for arbitrary quadrature angles with ±1° precision. Frequency-dependent orientations of the squeezing ellipse are necessary for squeezed states of light to provide a broadband sensitivity improvement in third-generation gravitational-wave interferometers. We consider the application of our system to long-baseline interferometers such as a future squeezed-light upgraded GEO 600 detector.
+ }
+}