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.
Original language | English |
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Article number | 184001 |
Journal | Classical and Quantum Gravity |
Volume | 40 |
Issue number | 18 |
DOIs | |
State | Published - 10 Sep 2023 |
Externally published | Yes |
Keywords
- black hole
- modified gravity
- symmergent gravity
- thin accretion disk