RELATIVISTIC MAGNETOFLUID DISK WITH NONZERO RADIAL-VELOCITY IN SCHWARZSCHILD GEOMETRY

In this paper we consider the equilibrium of a magnetofluid disc in Schwarzschild background with an external magnetic field, having the azimuthal and the radial components of the flow velocity nonzero. The electrical conductivity σ of the fluid is taken to be finite and thus the solution for the electromagnetic field is required to satisfy the Ohm's law too with the four-current having only J φ{symbol} and J t nonzero. The various physical parameters that have to correlate for possible equilibrium configurations are identified and their respective magnitudes estimated. It is found that for a given angular momentum distribution the inner edge of the disc can reach well within the usual 6m limit only when the surface magnetic field of the central object is not too high when the matter density at the outer edge of the disc and the accretion rate are taken with reasonable limits © 1990 Indian Academy of Sciences.