Integral Equation for Scattering of Light by a Strong Magnetostatic Field in Vacuum

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dc.creatorLakhtakia, Akhlesh
dc.creatorMackay, Tom G.
dc.date2007-02-21
dc.date.accessioned2026-07-07T08:23:49Z
dc.date.available2026-07-07T08:23:49Z
dc.descriptionWhen a strong magnetostatic field is present, vacuum effectively appears as a linear, uniaxial, dielectric-magnetic medium for small-magnitude optical fields. The availability of the frequency-domain dyadic Green function when the magnetostatic field is spatially uniform facilitates the formulation of an integral equation for the scattering of an optical field by a spatially varying magnetostatic field in vacuum. This integral equation can be numerically treated by using the method of moments as well as the coupled dipole method. Furthermore, the principle underlying the strong-property-fluctuation theory allows the homogenization of a spatially varying magnetostatic field in the context of light scattering.
dc.identifierhttps://arxiv.org/abs/physics/0702175
dc.identifierhttp://arxiv.org/abs/physics/0702175
dc.identifierElectromagnetics, Vol. 27, pp. 341-354 (2007)
dc.identifierdoi:10.1080/02726340701492554
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/136137
dc.subjectOptics
dc.titleIntegral Equation for Scattering of Light by a Strong Magnetostatic Field in Vacuum
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