Abstract: | The dependence of the momentum flux density on the particle flux and pressure tensor is calculated for a relativistic collisionless plasma. It is shown that the relativistic plasma is not representable by the ideal fluid model in the presence of longitudinal and transverse perturbations.Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 4, pp. 80–83, April, 1989. |