2000
DOI: 10.1134/1.1342880
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On the energy flux of stationary electromagnetic waves in anisotropic dissipative media with spatial dispersion

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Cited by 5 publications
(7 citation statements)
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“…In our previous papers, we have shown how for the time independent case the term G can be recast in order to obtain the wave power balance in the form ∇S + Q = 0, with modified wave power flux S and power loss Q [9,10]. What follows is a straightforward generalization of these results from threedimensional space dependence to four-dimensional spacetime dependence.…”
Section: The Power Balance Equationmentioning
confidence: 85%
See 1 more Smart Citation
“…In our previous papers, we have shown how for the time independent case the term G can be recast in order to obtain the wave power balance in the form ∇S + Q = 0, with modified wave power flux S and power loss Q [9,10]. What follows is a straightforward generalization of these results from threedimensional space dependence to four-dimensional spacetime dependence.…”
Section: The Power Balance Equationmentioning
confidence: 85%
“…In previous papers, we have derived a generalized wave energy flux for time independent wave beams [9,10]. The real part of the eigenvalue of the dispersion tensor corresponding to the wave mode under consideration has been identified as an appropriate ray-Hamiltonian in this case: it has been shown that the ray traces obtained by this approach coincide with the direction of the generalized energy flux.…”
Section: Introductionmentioning
confidence: 99%
“…, and λ t (ω t , k t ) are the eigennumbers of the operators D s pm and D t pm , which determine, in particular, the law of wave dispersion in the linear approximation: λ s (ω s , k s , r) = 0 and λ t (ω t , k t , r) = 0 (on using the eigennumber of the corresponding operator in the dispersion equation see [19,20]). In the absence of the right-hand sides, Eqs.…”
Section: Basic Equationsmentioning
confidence: 99%
“…(11) have the integrals div(p s |A s | 2 ) = 0 and div(p t |A t | 2 ) = 0. These integrals reflect the conservation of wave-energy fluxes (on presenting the energy flux in the form I = p |A| 2 see [19,20] for more detail). In the presence of nonlinear interaction and taking into account symmetry relationships (6), from Eq.…”
Section: Basic Equationsmentioning
confidence: 99%
“…One of the reasons, already described in the previous section, is that the dissipation in terms of geometric optics, Im H(x, q) > 0, does not guarantee the positive-definiteness of the corresponding operator termĤ A . More generally, this is a known issue of finding a proper approximation for physically correct wave absorption in media with a spatial dispersion [22][23][24][25][26][27] . In our case, errors in the approximation of the Hermitian part (e.g.…”
Section: Numerical Solutionmentioning
confidence: 99%