Neutral particle motion around a Schwarzschild-de Sitter Black Hole in f(R) gravity

This article investigates the presence of a static spherically symmetric solution in the metric f® gravity. Consequently, we have examined the presence of horizons for the extreme and hyperextreme Schwarzschild-de Sitter solution. Further, we have investigated the orbital motion of a time-like particle around the Schwarzschild-dS solution by forming the constraints for the existence of circular orbits and have subsequently developed an approximation to the innermost stable circular orbit (ISCO).