Thin accretion disk images of the black hole in symmergent gravity
General Relativity and Quantum Cosmology
2023-08-09 v1
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.
Keywords
Cite
@article{arxiv.2308.03947,
title = {Thin accretion disk images of the black hole in symmergent gravity},
author = {İlim İrfan Çimdiker and Ali Övgün and Durmuş Demir},
journal= {arXiv preprint arXiv:2308.03947},
year = {2023}
}
Comments
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