Observable characteristics of the charged black hole surrounded by thin disk accretion in Rastall gravity

DOI10.1088/1361-6382/ac6fa8zbMath1497.83025arXiv2205.11241OpenAlexW4280577744MaRDI QIDQ5865234

Unnamed Author, Sen Guo, Guanru Li

Publication date: 13 June 2022

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2205.11241

zbMATH Keywords

ringblack hole shadowthin disk accretion

Mathematics Subject Classification ID

Black holes (83C57) Diffraction, scattering (78A45) Electromagnetic fields in general relativity and gravitational theory (83C50) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Motion of charged particles (78A35)

Related Items (1)

Observational signatures: shadow cast by the effective metric of photons for black holes with rational non-linear electrodynamics

Cites Work

• Shadows and strong gravitational lensing: a brief review
• Gravity effects on Hawking radiation from charged black strings in Rastall theory
• Black hole solutions surrounded by perfect fluid in Rastall theory
• Generalization of the Einstein Theory
• Gravitational analysis of neutral regular black hole in Rastall gravity
• Lensing and shadow of a black hole surrounded by a heavy accretion disk
• Dynamics of charged and rotating NUT black holes in Rastall gravity
• Shadow cast of noncommutative black holes in Rastall gravity
• The shadow and photon sphere of the charged black hole in Rastall gravity

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