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dc.creatorNovikova, I.
dc.creatorMatsko, A. B.
dc.creatorVelichansky, V. L.
dc.creatorScully, Marlan O.
dc.creatorWelch, George R.
dc.date.accessioned2011-09-08T21:35:53Z
dc.date.available2011-09-08T21:35:53Z
dc.date.issued2001
dc.identifier.citationI. Novikova, A. B. Matsko, V. L. Velichansky, Marlan O. Scully and George R. Welch. Phys.Rev.A 63 063802 2001. "Copyright (2001) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevA.63.063802
dc.identifier.urihttps://hdl.handle.net/1969.1/126547
dc.descriptionJournals published by the American Physical Society can be found at http://publish.aps.org/en
dc.description.abstractThe ac Stark shift of the resonance frequency of the nonlinear magneto-optic effect (NMOE) results in a fundamental broadening of this resonance which limits the precision of optical magnetometry based on NMOE. We have studied the dependence of the ac Stark shift versus frequency of the probing laser for the D-1 and D-2 lines of Rb-87 and have shown that there exists a frequency where the shifts from different hyperfine components of the upper level cancel each other. This holds promise for an in-principle increase in the sensitivity of optical magnetometers. The influence of buffer gas on Faraday rotation and ac Stark shifts is also considered.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.subjectNONLINEAR MAGNETOOPTICAL ROTATIONen
dc.subjectINTENSE LASER FIELDSen
dc.subjectSAMARIUM VAPORen
dc.subjectFARADAYen
dc.subjectOpticsen
dc.subjectPhysicsen
dc.titleCompensation of ac Stark shifts in optical magnetometry RID B-9041-2008 RID A-1272-2007en
dc.typeArticleen
local.departmentPhysics and Astronomyen


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