In this study of Kerr-type black hole within the Starobinsky–Bel–Robinson gravity, we unveil
intriguing dynamics. We observe that the black hole spin weakens the effective potential …

This study investigates the optical properties of a rotating black hole in Starobinsky-Bel-
Robinson gravity, characterized by the additional parameter β. The black hole is assumed to …

This work is devoted to the study of motion of spinning test particles in the spacetime of the
Kerr–Newman–NUT black hole with quintessence, in the Rastall gravity theory. We use the …

In this work we focus on the effects of Starobinsky–Bel–Robinson (SBR) gravity parameter
and external magnetic field on the motion of charged test particles and magnetic dipoles …

In this work, we investigate the electromagnetic energy released by astrophysical black
holes within the Kerr-Taub-NUT solution, which describes rotating black holes with a …

Investigation of the optical properties of a black hole described by the so-called “eye of the
storm” space–time has been the main aim of the work. Such a space–time is regular and …

Abstract In 2022, the Event Horizon Telescope (EHT) collaboration has reported the first
observations of Sagittarius A*(SgrA*). Applying the EHT observational results, we find out …

In this research, we explore the electromagnetic energy emitted by astrophysical black holes
within the Kerr+ PFDM (Kerr+ perfect fluid dark matter) spacetime, a model comprising …

Here we investigate the energetics of the charged-rotating-NUT-Kiselev black hole (CRNK-
BH) in the Rastall modified theory of gravity. First, we study the dependence of the …

In this paper, we investigated the motion of massive particles in the presence of scalar and
gravitational fields, particularly focusing on the Janis-Newman-Winicour (JNW) naked …