Equilibrium configuration of perfect fluid orbiting around black holes in some classes of alternative gravity theories
Sumanta Chakraborty

TL;DR
This paper investigates the structure and stability of perfect fluid accretion disks around black holes in various alternative gravity theories, highlighting differences from general relativity that could serve as observational probes.
Contribution
It analyzes the hydrodynamic behavior and equipotential surface structures of perfect fluids in alternative gravity spacetimes, revealing unique accretion disk configurations.
Findings
Closed equipotential surfaces with cusps allow accretion disks.
Stable central rings form with increasing angular momentum density.
Charged $F(R)$ gravity and Einstein-Maxwell-Gauss-Bonnet solutions show inflow and outflow of matter.
Abstract
The hydrodynamic behaviour of perfect fluid orbiting around black holes in spherically symmetric spacetime for various alternative gravity theories has been investigated. For this purpose we have assumed an uniform distribution for the angular momentum density of the rotating perfect fluid. The contours of equipotential surfaces are illustrated in order to obtain the nature of inflow and outflow of matters. It has been noticed that, the marginally stable circular orbits originating from decreasing angular momentum density lead to closed equipotential surfaces along with cusp allowing existence of accretion disks. On the other hand, the growing part of angular momentum density exhibits central rings for which stable configurations are possible. However inflow of matter is prohibited. Among the solutions discussed in this work, the charged gravity and Einstein-Maxwell-Gauss-Bonnet…
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