Quasinormal modes, thermodynamics and shadow of black holes in Hu-Sawicki f(R) gravity theory

TL;DR

This paper introduces new black hole solutions in Hu-Sawicki f(R) gravity, analyzing their quasinormal modes, thermodynamics, and shadows, and constrains model parameters using observational data.

Contribution

It provides novel black hole solutions in Hu-Sawicki f(R) gravity and studies their quasinormal modes, thermodynamics, and shadows, with observational parameter constraints.

Findings

Black hole solutions derived in Hu-Sawicki f(R) gravity.

Quasinormal modes depend on model parameters and are computed with errors.

Black hole shadow radius depends on model parameters and observational data constrains parameters.

Abstract

We derive novel black hole solutions in a modified gravity theory, namely the Hu-Sawicki model of $f(R)$ gravity. After obtaining the black hole solution, we study the horizon radius of the black hole from the metric and then analyse the dependence of the model parameters on the horizon. We then use the 6th-order WKB method to study the quasinormal modes of oscillations (QNMs) of the black hole perturbed by a scalar field. The dependence of the amplitude and damping part of the QNMs are analysed with respect to variations in model parameters and the errors associated with the QNMs are also computed. After that, we study some thermodynamic properties associated with the black hole such as its thermodynamic temperature as well as greybody factors. It is found that the black hole has the possibility of showcasing negative temperatures. We also analyse the geodesics and derive the photon sphere radius as well as the shadow radius of the black hole. The photon radius is independent of the model parameters while the shadow radius showed a fair amount of dependence on the model parameters. We tried to constrain the parameters with the help of Keck and VLTI observational data and obtained some bounds on $m$ and $c_{2}$ parameters.