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On the structure of the new electromagnetic conservation laws

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S Brian Edgar

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LETTER TO THE EDITOR

New electromagnetic conservation laws have recently been proposed: in the absence of electromagnetic currents, the trace of the Chevreton superenergy tensor, Hab is divergence free in four-dimensional (a) Einstein spacetimes for test fields, and (b) Einstein–Maxwell spacetimes. Subsequently it has been pointed out, in analogy with flat spaces, that for Ricci-flat spacetimes the trace of the Chevreton superenergy tensor Hab can be rearranged in the form of a generalized wave operator squL acting on the energy–momentum tensor Tab of the test fields, i.e., Hab = squLTab/2. In this letter we show, for Einstein–Maxwell spacetimes in the full nonlinear theory, that, although, the trace of the Chevreton superenergy tensor Hab can again be rearranged in the form of a generalized wave operator squG acting on the electromagnetic energy–momentum tensor, in this case the result is also crucially dependent on Einstein's equations; hence we argue that the divergence-free property of the tensor Hab = squGTab/2 has significant independent content beyond that of the divergence-free property of Tab.


PACS

03.50.De Classical electromagnetism, Maxwell equations

04.40.Nr Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields

MSC

83C22 Einstein-Maxwell equations

83C50 Electromagnetic fields

83C40 Gravitational energy and conservation laws; groups of motions

Subjects

Gravitation and cosmology

Particle physics and field theory

Dates

Issue 4 (21 February 2004)

Received 18 November 2003

Published 14 January 2004



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