Study of relativistic accretion flow in the $f(R)$ theory of gravity
Akhil Uniyal, Sayan Chakrabarti, Santabrata Das

TL;DR
This paper investigates relativistic accretion flows within an $f(R)$ gravity framework, analyzing how modifications to gravity influence flow properties, critical points, and luminosity, with implications for accretion disk observations.
Contribution
It provides a detailed analysis of accretion flow solutions in $f(R)$ gravity, including the effects of gravity parameters on critical points and luminosity, extending understanding beyond general relativity.
Findings
Flow can have single or multiple critical points depending on parameters.
The parameter space for accretion solutions shrinks with decreasing $A$ and vanishes at $A=-2.34$.
Inner critical point solutions are more luminous than outer critical point solutions.
Abstract
We present the properties of relativistic, inviscid, low angular momentum, advective accretion flow in a gravity theory that satisfactorily mimics the asymptotically flat vacuum solutions of the Einstein's equations. With this, we solve the governing equations describing the accretion flow and obtain the global transonic accretion solutions in terms of flow energy (), angular momentum () and gravity parameter () that determines the effect of gravity. We observe that depending on the model parameters, flow may contain either single or multiple critical points. We separate the effective domain of the parameter space in plane that admits accretion solutions possessing multiple critical points and observe that solution of this kind continues to form for wide range of the flow parameters. We examine the modification of the parameter…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Galaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories
