2002
DOI: 10.1002/1521-3889(200211)11:10/11<717::aid-andp717>3.0.co;2-6
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Linear pre-metric electrodynamics and deduction of the light cone

Abstract: We formulate a general framework for describing the electromagnetic properties of spacetime. These properties are encoded in the 'constitutive tensor of the vacuum', a quantity analogous to that used in the description of material media. We give a generally covariant derivation of the Fresnel equation describing the local properties of the propagation of electromagnetic waves for the case of the most general possible linear constitutive tensor. We also study the particular case in which a light cone structure … Show more

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Cited by 53 publications
(107 citation statements)
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“…For our simple example of a Klein-Gordon field on a metric geometry, the determinant in (2) is of weight zero, and for the choice ρ = 1 we obtain P i 1 i 2 = G i 1 i 2 , and one indeed recovers the familiar massless dispersion relation G a 1 a 2 k a 1 k a 2 = 0. An instructive non-metric example is provided by abelian gauge theory coupled to an inverse area metric tensor geometry [11,12], which is based on a fourth rank contravariant tensor field G featuring the algebraic symmetries G abcd = G cdab = −G bacd ; calculation of the principal polynomial (after removing gauge-invariance, observing resulting constraints on initial conditions and re-covariantizing the expression) one obtains [10,13,14] in dim M = d dimensions the totally symmetric tensor field…”
Section: A Primer On Tensorial Spacetime Geometriesmentioning
confidence: 99%
“…For our simple example of a Klein-Gordon field on a metric geometry, the determinant in (2) is of weight zero, and for the choice ρ = 1 we obtain P i 1 i 2 = G i 1 i 2 , and one indeed recovers the familiar massless dispersion relation G a 1 a 2 k a 1 k a 2 = 0. An instructive non-metric example is provided by abelian gauge theory coupled to an inverse area metric tensor geometry [11,12], which is based on a fourth rank contravariant tensor field G featuring the algebraic symmetries G abcd = G cdab = −G bacd ; calculation of the principal polynomial (after removing gauge-invariance, observing resulting constraints on initial conditions and re-covariantizing the expression) one obtains [10,13,14] in dim M = d dimensions the totally symmetric tensor field…”
Section: A Primer On Tensorial Spacetime Geometriesmentioning
confidence: 99%
“…The skewon contributions in (24) and (25) are responsible for the electric and magnetic Faraday effects, respectively, whereas skewon terms in (26) and (27) describe optical activity.…”
Section: General Local and Linear Constitutive Relationmentioning
confidence: 99%
“…Here we briefly summarize the results of previous work [6,22,26,27]. In the Hadamard approach, one studies the propagation of a discontinuity in the first derivative of the electromagnetic field.…”
Section: General Fresnel Equations: Wave and Ray Surfacesmentioning
confidence: 99%
“…We have shown in the past (see [13,14]) how one can determine light propagation in an arbitrary spacetime by means of a generalized Fresnel equation provided a linear spacetime relation H = κ(F ), or in components H αβ = 1 2 κ αβ γδ F γδ , is specified. Recently, we applied this method also to nonlinear electrodynamics, see [15].…”
Section: Birefringence For An Arbitrary Spherically Symmetric Tomentioning
confidence: 99%