Thin accretion disk around the distorted Schwarzschild black hole

Abstract

We construct the relativistic standard steady, optically thick, cold and geometrically thin accretion disk around a distorted Schwarzschild black hole. The distortion of this static and axially symmetric black hole solution, is connected to an external distribution of matter. If the effects due to the rotation are negligible, this distribution can describe the exterior of any axially symmetric astrophysical model. Also, the distortion could be related to the outer parts of the accretion disk. We study the effects due to a distortion up to the quadrupole, and compare the physical characteristics of this disk to the usual Schwarzschild case.

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Cited by in corpus (8)

• Thin Accretion Disk around a four-dimensional Einstein-Gauss-Bonnet Black Hole
• Thin Accretion Disk onto slowly rotating black holes in Einstein-Æther theory
• Image of Bonnor black dihole with a thin accretion disk and its polarization information
• Accretion of matter and spectra of Binary X-ray sources in Massive Gravity
• Nonassociative black ellipsoids distorted by R-fluxes and four dimensional thin locally anisotropic accretion disks
• Binary X-ray sources in massive Brans-Dicke gravity
• Effect of an external mass distribution on the magnetized accretion disk
• Thin accretion disks around a Schwarzschild acoustic black hole