Steady flow around a rotating black hole

Statistics – Computation

Scientific paper

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Astrophysics, Black Holes (Astronomy), Rotating Fluids, Steady Flow, Angle Of Attack, Angular Momentum, Computational Fluid Dynamics, Energy Absorption, Equations Of State, Gas Density, Gravitational Fields, Ideal Gas, Incompressible Fluids, Newtonian Fluids, Potential Flow, Sinks

Scientific paper

An analysis is presented of the steady potential flow of an ideal relativistic gas in a given gravitational field. The equation of state is a generalization of the model of a Newtonian incompressible fluid. A solution is obtained in a finite form to the problem of the flow around a rotating Kerr black hole for an arbitrary angle of attack. This solution makes it possible to determine the magnitude of the sink from the condition of the finiteness of gas density at the horizon, and to calculate the energy absorption, momentum, and angular momentum of the medium surrounding a translationally moving and rotating black hole.

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