Thin accretion disk images of the black hole in symmergent gravity

Abstract

In this paper, we study circular orbits, effective potential, and thin-accretion disk of a black hole in symmergent gravity within the Novikov-Thorne model in a way including the energy flux and temperature distribution. We determine bounds on symmergent gravity parameters and conclude that the accretion disk could be used as an astrophysical tool to probe symmergent gravity.

30 pages. Accepted for publication in Classical and Quantum Gravity, "Special Issue: Focus on Quantum Gravity Phenomenology in the Multi-Messenger Era: Challenges and Perspectives" (https://iopscience.iop.org/article/10.1088/1361-6382/aceb45). arXiv admin note: text overlap with arXiv:1901.05762, arXiv:2002.00589 by other authors

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Cited by in corpus (8)

• Black hole surrounded by the pseudo-isothermal dark matter halo
• Shadow and deflection angle of asymptotic, magnetically-charged, non-singular black hole
• Quasinormal modes and greybody factors of symmergent black hole
• Analyzing the Influence of Geometrical Deformation on Photon Sphere and Shadow Radius: A New Analytical Approach -- Spherically Symmetric Spacetimes
• Image of the Kerr-Newman black hole surrounded by a thin accretion disk
• Topological dyonic black holes of massive gravity with generalized quasitopological electromagnetism
• Quasinormal Modes and Greybody Factors of Charged Symmergent Black Hole
• Aberration effect on lower-order images of thin accretion disk in the astrometric approach