Quasinormal modes, thermodynamics and shadow of black holes in Hu–Sawicki $$\varvec{f(R)}$$ gravity theory

• Published in: The European physical journal. C, Particles and fields Vol. 84; no. 9
• Main Authors: Karmakar, Ronit, Goswami, Umananda Dev
• Format: Journal Article
• Language: English
• Published: 27.09.2024
• ISSN: 1434-6052; 1434-6052
• DOI: 10.1140/epjc/s10052-024-13359-4

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 error 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 and is thermodynamically unstable for feasible values of model parameters. Then we 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 shadow radius showed 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 $$c_{2}$$ c 2 parameters.