Thin accretion disk images of the black hole in symmergent gravity
Ilim Çimdiker, Ali Övgün, D. Demir
Abstract
Abstract 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.
Topics & Concepts
PhysicsAccretion discThin diskAstrophysicsAccretion (finance)Black hole (networking)AstronomyStarsRouting protocolComputer networkComputer scienceLink-state routing protocolRouting (electronic design automation)Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsAstrophysical Phenomena and Observations