Thin accretion disk around the distorted Schwarzschild black hole

verfasst von

Shokoufe Faraji, Eva Hackmann

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.

Externe Organisation(en)

Universität Bremen

Typ

Artikel

Journal

Physical Review D

Band

101

ISSN

2470-0010

Publikationsdatum

02.01.2020

Publikationsstatus

Veröffentlicht

Peer-reviewed

Ja

ASJC Scopus Sachgebiete

Physik und Astronomie (sonstige)

Elektronische Version(en)

https://doi.org/10.1103/PhysRevD.101.023002 (Zugang: Unbekannt)