Thin accretion disk images of the black hole in symmergent gravity

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

Automated summary

In this study, we investigate circular orbits, effective potential, and thin-accretion disk of a black hole in symmergent gravity (SG), using the Novikov-Thorne model and considering the energy flux and temperature distribution. We establish limits on SG parameters and conclude that the accretion disk can serve as an astrophysical tool for probing SG.