S Brian Edgar 2004 Class. Quantum Grav. 21 L21 doi:10.1088/0264-9381/21/4/L04
S Brian Edgar
Show affiliationsNew 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
L acting on the energy–momentum tensor Tab of the test fields, i.e., Hab =
LTab/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
G 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 =
GTab/2 has significant independent content beyond that of the divergence-free property of Tab.
03.50.De Classical electromagnetism, Maxwell equations
04.40.Nr Einstein-Maxwell spacetimes, spacetimes with fluids, radiation or classical fields
83C22 Einstein-Maxwell equations
83C40 Gravitational energy and conservation laws; groups of motions
Issue 4 (21 February 2004)
Received 18 November 2003
Published 14 January 2004
S Brian Edgar 2004 Class. Quantum Grav. 21 L21
F Petrů et al 1992 Metrologia 29 301
John Terblanche et al 2004 Physiol. Meas. 25 1189
Ganesh K Ramachandran et al 2005 Nanotechnology 16 1294
Wai Lam Chan et al 2007 Rep. Prog. Phys. 70 1325
Junxiang Zhang et al 2001 Europhys. Lett. 56 478
Nita Dilawar et al 2003 Metrologia 40 74
Davinder Kaur and A K Gupta 2002 J. Phys. D: Appl. Phys. 35 729
J M Gibson 2009 Rep. Prog. Phys. 72 076001
C M Surko et al 2005 J. Phys. B: At. Mol. Opt. Phys. 38 R57