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Causality criteria
Authors:Eckhard Krotscheck  Wolfgang Kundt
Institution:(1) I. Institut für Theoretische Physik der Universität Hamburg, D-2000 Hamburg, Federal Republic of Germany;(2) Institut für Astrophysik und Extraterrestrische Physik der Universität Bonn, D-5300 Bonn, Federal Republic of Germany
Abstract:By ldquocausality of matterrdquo one means its property not to admitsuperluminal excitations, i.e. excitations that propagate faster than the vacuum speed of lightc. In discussing the propagation of small excitations, one has to distinguish betweenphase velocities ohgr j /k, (1lEjlEg=number of dispersion branches),group velocities dohgr j /dk, a front velocityv f : = 
$$\mathop {\max }\limits_j  \mathop {\lim }\limits_{k \to \infty } \left( {{{\omega _j } \mathord{\left/ {\vphantom {{\omega _j } k}} \right. \kern-\nulldelimiterspace} k}} \right)$$
and the propagation speedv q :=(dp/drhov)1/2 of isotropic quasistatic (small) perturbations. We discuss some of their properties. In particular, the (maximal) speedv s of small signals is not smaller thanv f , and equalsv f whenever the dispersion branches ohgr j (k) behave reasonably at infinity of the complexk-plane. In essence stronger conditions guaranteev q <v f (in which casev q gEc would imply superluminal behaviour).
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