Wave Properties of Isothermal Magneto-Rotational Fluids

Abstract

In this paper, the isothermal plasma wave properties in the neighborhood of the pair production region for the Kerr black hole magnetosphere are discussed. We have considered the Fourier analyzed form of the perturbed general relativistic magnetohydrodynamical equations whose determinant leads to a dispersion relation. For the special scenario, the $x$-component of the complex wave vectors are numerically calculated. Respective components of the propagation vector, attenuation vector, phase and group velocities are shown in graphs. We have particularly investigated the existence of a Veselago medium and wave behavior (modes of waves dispersion

29 pages, 24 figures accepted for publication in Canadian J. Physics

References in corpus (5)

• Cold Plasma Dispersion Relations in the Vicinity of a Schwarzschild Black Hole Horizon
• Effects of Schwarzschild Black Hole Horizon on Isothermal Plasma Wave Dispersion
• Complex Wave Numbers in the Vicinity of the Schwarzschild Event Horizon
• Isothermal Plasma Waves in Gravitomagnetic Planar Analogue
• Wave Properties of Plasma Surrounding the Event Horizon of a Non-Rotating Black Hole

Cited by in corpus (6)

• Plasma Wave Properties of the Schwarzschild Magnetosphere in a Veselago Medium
• Hot Plasma Waves Surrounding the Schwarzschild Event Horizon in a Veselago Medium
• Isothermal Plasma Wave Properties of the Schwarzschild de-Sitter Black Hole in a Veselago Medium
• Dispersion Modes of Hot Plasma for Schwarzschild de-Sitter Horizon in a Veselago Medium
• Cold Plasma Wave Analysis in Magneto-Rotational Fluids
• Hot Plasma Modes Across Reissner-Nordstrom de Sitter Horizon in a Veselago Medium