Abstract
The closed set of relativistic hydrodynamical equations describing strongly magnetized collisionless plasma with an anisotropic pressure tensor is offered. This model is the generalization of Chew–Goldberger–Low [Proc. R. Soc. London Ser. A 236, 112 (1956)] theory for the relativistic case. It is shown that at high temperatures the equation of state differs significantly from the ones used earlier.
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