On the flow of special relativistic fluids through channels

Details On the flow of special relativistic fluids through channels On the flow of special relativistic fluids through channels

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..54..407w&link_type=abstract

Astrophysics and Space Science, vol. 54, no. 2, Apr. 1978, p. 407-415.

Astronomy and Astrophysics

Astronomy

4

Astronomical Models, Channel Flow, Magnetohydrodynamic Flow, One Dimensional Flow, Radio Sources (Astronomy), Relativistic Plasmas, Relativistic Velocity, Energy Conservation, Flow Equations, Galactic Nuclei, Kelvin-Helmholtz Instability, Particle Beams, Steady State

Scientific paper

The equations for the flow of a relativistic fluid down a channel of constantly changing cross section are derived for the twin-exhaust model of double radio sources, in which a large quantity of relativistic plasma is quasi-continuously ejected from the active region of a galactic nucleus. The major assumptions are that the flow is predominantly one-dimensional and that the fluid is perfect. The expressions for the time change of the components of the stress-energy tensor are compact and amenable to numerical integration.

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