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Journal ArticleDOI

Killing vector fields and the Einstein-Maxwell field equations in general relativity

H. Michalski, +1 more
- 01 Jun 1975 - 
- Vol. 6, Iss: 3, pp 289-318
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Abstract
A number of theorems concerning non-null electrovac spacetimes, that is space-times whose metric satisfies the source-free Einstein-Maxwell equations for some non-null bivector Fij, are presented. Firstly, we suppose that the metric is invariant under a one-parameter group of isornetries with Killing vector field ξ. It is proved that the electromagnetic field tensor Fij is invariant under the group, in the sense that its Lie derivative with respect to ξ vanishes, if and only if the gradient αij of the complexion scalar is orthogonal to ξ. It is is also proved that if in addition ξ is hypersurface orthogonal, it is necessarily parallel to α,i. These results are used to generalize theorems of Perjes and Majumdar concerning static electrovac space-times. Secondly, we suppose that the metric is invariant under a two-parameter othogonally transitive Abelian group of isometries. It is proved that in this case Fij is necessarily invariant under the group. The above results can be used to simplify many derivations of exact solutions of the Einstein-Maxwell equations.

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Citations
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Super-energy tensors

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On the evolution equations for Killing fields

TL;DR: In this article, it was shown that the evolution equations obtained in all these cases are of nonstrictly hyperbolic type, and thus the Cauchy data must belong to a special class of functions.
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Symmetries and the Einstein-Maxwell field equations the null field case

TL;DR: In this article, it was shown that if the space-time admits a group of isometrics, then the fluid velocity, energy density, pressurep, and charge densitye are invariant under the group.
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Killing Vector Fields and the Einstein-Maxwell Field Equations with Perfect Fluid Source

TL;DR: In this paper, the authors considered the case of the electromagnetic field tensor tensor, the charge density, and the four-velocityui, energy densityμ, and pressurep of the fluid, and showed that the behavior of these quantities under the group is strongly restricted.
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Symmetry inheritance of scalar fields

TL;DR: In this article, the symmetry non-inheritance of scalar fields of real and complex objects is studied. But the symmetry inheritance is not necessarily shared with the spacetime they live in.
References
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Journal ArticleDOI

The classical theory of fields

TL;DR: The principle of relativity Relativistic mechanics Electromagnetic fields electromagnetic waves as discussed by the authors The propagation of light The field of moving charges Radiation of electromagnetic waves Particle in a gravitational field The gravitational field equation
Book

The Large Scale Structure of Space-Time

TL;DR: In this paper, the authors discuss the General Theory of Relativity in the large and discuss the significance of space-time curvature and the global properties of a number of exact solutions of Einstein's field equations.
Journal ArticleDOI

Global structure of the Kerr family of gravitational fields

TL;DR: In this article, it was shown that in all except the spherically symmetric cases there is a nontrivial causality violation, i.e., there are closed timelike lines which are not removable by taking a covering space; moreover, when the charge or angular momentum is so large that there are no Killing horizons, this causal violation is of the most flagrant possible kind in that it is possible to connect any event to any other by a future-directed time line.
Journal ArticleDOI

Metric of a Rotating, Charged Mass

TL;DR: In this article, a new solution of the Einstein-Maxwell equations is presented, which has certain characteristics that correspond to a rotating ring of mass and charge, similar to the one described in this paper.
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