2004
DOI: 10.1088/0264-9381/21/13/007
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Maxwell fields and shear-free null geodesic congruences

Abstract: We study and report on the class of vacuum Maxwell fields in Minkowski space that possess a non-degenerate, diverging, principle null vector field (null eigenvector field of the Maxwell tensor) that is tangent to a shear-free null geodesics congruence. These congruences can be either surface forming (the tangent vectors being proportional to gradients) or not, i.e., the twisting congruences. In the non-twisting case, the associated Maxwell fields are precisely the Lienard-Wiechert fields, i.e., those Maxwell f… Show more

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Cited by 36 publications
(65 citation statements)
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“…In section 2.3, we describe the requirements which must be satisfied by a gauge field single copy of a Kerr-Schild metric. Referring to previous work of Newman, in section 3 we relate these single copies to real slices of complex Liénard-Wiechert fields [13], and use this identification to systematically construct all four-dimensional black hole spacetimes on Minkowski backgrounds. In section 4, we present a test for Kerr-Schild structure in any number of dimensions.…”
Section: Contentsmentioning
confidence: 99%
See 1 more Smart Citation
“…In section 2.3, we describe the requirements which must be satisfied by a gauge field single copy of a Kerr-Schild metric. Referring to previous work of Newman, in section 3 we relate these single copies to real slices of complex Liénard-Wiechert fields [13], and use this identification to systematically construct all four-dimensional black hole spacetimes on Minkowski backgrounds. In section 4, we present a test for Kerr-Schild structure in any number of dimensions.…”
Section: Contentsmentioning
confidence: 99%
“…In fact, any field strength with this property is a Liénard-Wiechert field. The result of [13] is to generalize this construction to twisting congruences. If we take a complex extension of Minkowski space and consider a particle on a worldline z µ (τ ) = x µ (τ ) + iy µ (τ ), (3.3) gives a complex gauge field which can be used to construct a complex field strength.…”
Section: Liénard-wiechert Single Copy Fieldsmentioning
confidence: 99%
“…, by omitting cubic terms including L 2 φ 0 2 , then using the first two terms of the Taylor series 16) and the Clebsch-Gordon expansions of the products of the spherical harmonics (see Appendix A) we finally have (after simplification) for just the l = 1 harmonic terms…”
Section: The Quantities Qηmentioning
confidence: 99%
“…The simple answer is that an (analytic) asymptotically flat Maxwell field in Minkowski space with non-vanishing total charge generates, in the complex Minkowski space, a unique complex analytic world-line: the complex center of charge world-line, where the real part describes the standard center of charge while the ribbon thickness encodes magnetic dipole information [16,17]. For the case of asymptotically flat space-times there are two situations: the vacuum asymptotically flat and the Einstein-Maxwell asymptotically flat spacetimes.…”
Section: Introductionmentioning
confidence: 99%
“…Though we are dealing with real electromagnetic fields in real Minkowski space, this trivial observation can be formally generalized [8,9,17] to complex translations defining a complex center of charge world-line around which both the electric and magnetic dipoles vanish. Associated with this complex center of charge world-line is a null geodesic congruence in Minkowski space that is shear-free but twisting.…”
Section: Introductionmentioning
confidence: 99%