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dc.contributor.authorFranssens, G.R.
dc.date2015
dc.date.accessioned2016-03-24T12:08:13Z
dc.date.available2016-03-24T12:08:13Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/2775
dc.descriptionThe polarization of a partially coherent, transverse electric, electromagnetic plane wave is commonly represented by a Stokes vector. The similarity between Stokes vectors and four-momentum vectors in special relativity (SR) is studied in depth. The set of Stokes vectors naturally possesses a Euclidean and a Lorentzian geometry. The latter is used to express the polarization-altering properties of Jones–Mueller matrices in a simple and elegant way. In particular, it is shown that the action of a diattenuator on a Stokes vector can be understood in terms of the addition law for velocities from SR. An important simplification in the resulting mathematical expressions further arises if the degree of polarization of a Stokes vector is represented by a hyperbolic polarization angle. This then allows us to demonstrate that the output hyperbolic polarization angle is related to a diattenuator hyperbolic polarization angle and the input hyperbolic polarization angle by the hyperbolic law of cosines holding in a hyperbolic triangle.
dc.languageeng
dc.titleRelativistic kinematics formulation of the polarization effects of Jones–Mueller matrices
dc.typeArticle
dc.subject.frascatiMathematics
dc.audienceScientific
dc.source.titleJournal of the Optical Society of America A
dc.source.volume32
dc.source.issue2
dc.source.page164-172
Orfeo.peerreviewedYes
dc.identifier.doi10.1364/JOSAA.32.000164


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