Preprint Article Version 1 Preserved in Portico This version is not peer-reviewed

Trajectory of Massive Particles around a Static Black Hole in f(R) Gravity

Version 1 : Received: 21 July 2022 / Approved: 22 July 2022 / Online: 22 July 2022 (14:14:20 CEST)

A peer-reviewed article of this Preprint also exists.

Mandal, S. Trajectory of Massive Particles around a Static Black Hole in f(R) Gravity. Europhysics Letters 2022, 140, 69001, doi:10.1209/0295-5075/aca92f. Mandal, S. Trajectory of Massive Particles around a Static Black Hole in f(R) Gravity. Europhysics Letters 2022, 140, 69001, doi:10.1209/0295-5075/aca92f.

Abstract

In this paper, we investigated the trajectory of the massive particle in the vicinity of a general spherical symmetric black hole. Also, in the framework of general sphericalily symmetric black hole, Pseudo-Newtonian potential (PNP) and effective potentials has been investigated. As an example, static spherically symmetric black hole in f(R) gravity is considered and presented the brief discussion on the structure of spacetime and horizons. We calculated energy and angular momentum in the framework of general relativity as well as in Pseudo-Newtonian theory. A graphical comparison of angular momentum in this both framework has been studied.

Keywords

Massive particle; Static black hole; f(R) gravity; Pseudo-Newtonian Potential

Subject

Physical Sciences, Astronomy and Astrophysics

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