2004
DOI: 10.1364/ol.29.002800
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Sub-shot-noise heterodyne polarimetry

Abstract: We report an experimental demonstration of a heterodyne polarization rotation measurement with a noise floor 4.8 dB below the optical shot noise by use of classically phase-locked quantum twin beams emitted above threshold by an ultrastable type II Na:KTP cw optical parametric oscillator. We believe that this is the largest noise reduction achieved to date in optical phase-difference measurements.

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Cited by 20 publications
(15 citation statements)
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“…In the context of single-parameter phase estimation, it is very well explored how quantum resources allow an improvement in the precision limit [19,20]. Such quantum metrology techniques are particularly important for measuring very light-sensitive biological samples [21] and delicate materials [22], where high power and long exposure time is not permitted.…”
Section: Introductionmentioning
confidence: 99%
“…In the context of single-parameter phase estimation, it is very well explored how quantum resources allow an improvement in the precision limit [19,20]. Such quantum metrology techniques are particularly important for measuring very light-sensitive biological samples [21] and delicate materials [22], where high power and long exposure time is not permitted.…”
Section: Introductionmentioning
confidence: 99%
“…It is also equivalent to the generation of a bright entangled state, albeit a nonmaximally entangled one. The experimental challenge lied in the stabilization of the OPO frequencies to the level of in- B. Sub-shot-noise heterodyne polarimetry [18] S. Feng and O. Pfister, Opt. Lett.…”
Section: Summary Of the Most Important Resultsmentioning
confidence: 99%
“…This was demonstrated experimentally [7,8] and is now the approach adopted for high-frequency signals (above the standard quantum limit) in gravitational-wave detectors [9,10]. Many other approaches have been investigated [11,12], such as twin beams [13][14][15][16][17][18], "noon" states [19][20][21][22][23], or two-mode squeezed states. These different schemes were recently compared in terms of their quantum Cramér-Rao bound [24].…”
Section: Introductionmentioning
confidence: 99%
“…Gravitational-wave observatory LIGO is described by case 2, and soon case 3 [10], whereas GEO-600 is now operating with squeezing [9]. Table I is the twin Fock state input first proposed by Holland and Burnett [13], and which is im-plementable, to a good approximation, with large photon numbers by using an optical parametric oscillator above threshold [17,18,[31][32][33]. The input density operator is then of the form, in the absence of losses,…”
Section: Introductionmentioning
confidence: 99%