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A virial theorem for rotating charged perfect fluids in general relativity

A Georgiou

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We obtain an exact form of the virial theorem in general relativity, which is sufficiently general to be applied to charged, conducting, rotating perfect fluids in electromagnetic and gravitational fields. The case of infinite conductivity is of particular importance in astrophysics and we derive the relevant equations from the general results. We indicate how to calculate the post-Newtonian limits of various expressions and show that in the absence of both, the electric and magnetic fields, they lead to Chandrasekhar's post-Newtonian virial theorem in hydrodynamics. We also note that Chandrasekhar's (Newtonian) virial theorem in hydromagnetics may be derived from the Newtonian limit of the exact equations obtained. Some possible applications are pointed out. Finally, we use the exact form of the virial theorem to obtain, in co-moving coordinates, equilibrium conditions for bounded rotating charged dust.


PACS

04.25.Nx Post-Newtonian approximation; perturbation theory; related approximations

95.30.Sf Relativity and gravitation

41.20.Jb Electromagnetic wave propagation; radiowave propagation

95.30.Lz Hydrodynamics

95.30.Wi Dust processes (condensation, evaporation, sputtering, mantle growth, etc.)

MSC

83C50 Electromagnetic fields

83C55 Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.)

Subjects

Fluid dynamics

Accelerators, beams and electromagnetism

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 2 (21 January 2003)

Received 12 August 2002, in final form 5 November 2002

Published 3 January 2003



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