Thin accretion disk images of the black hole in symmergent gravity
İrfan ÇimdikerInstitute of Physics, University of Szczecin, Wielkopolska 15, Szczecin, Szczecin, Zachodniopomorskie, 70-453, POLANDAli ÖvgünDepartment of Physics, Eastern Mediterranean University Faculty of Arts and Sciences, Eastern Mediterranean University, Physics Department, Famagusta, 99628, CYPRUSD. DemirFaculty of Engineering and Natural Sciences, Sabanci University, Tuzla, Istanbul, 34956, TURKEY
2023en
ABI
Аннотация
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.
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