Abstract Using the Keeton and Petters approach, we determine the deflection angle. We
also investigate the motion of photons around a parameterized black hole in the presence of …

The Rastall theory of gravity is the generalized form of the Einstein theory which describes
the conservation law of energy and momentum tensor. In our work, we compute the charged …

In this paper, we explore the thermodynamic aspects of the hairy black hole solution
developed by gravitational decoupling in the spherical symmetry, considering its energy …

In this paper, we study two different phenomena (the Newman–Janis algorithm and the
semiclassical Hamilton–Jacobi method) to analyze the Hawking temperature (TH) for …

We consider an equation of motion for Glashow–Weinberg–Salam model and apply the
semiclassical Hamilton–Jacobi process and WKB approximation in order to compute the …

This work analyzes the Einstein–Gauss–Bonnet gravity of charged black hole solutions
through Newman–Janis approach. The Hawking temperature for corresponding black hole …

In this paper, we study the Tours-like black hole solution in the regularized self-energy of the
electrostatic field in the context of thermodynamics, energy emission, and Gibbs free energy …

The observable characteristics of the charged black hole (BH) surrounded by a thin disk
accretion are investigated in the Rastall gravity. We found that the radii of the direct …

We examine the thermodynamic properties of the symmergent black hole in this work. For
boson masses, we set the symmergent parameter to α= 0. 9, and for fermion masses, using …

In this study, we investigate the thermodynamic characteristics of the Simpson–Visser
Minkowski core black hole solution within Verlinde's emergent gravity framework. Our …