activity
20242026
collaborators

17 papers

gr-qc2026

Thermodynamics of Genuine Kerr-Bertotti-Robinson Black Holes

David Kubiznak, Hryhorii Ovcharenko, Jiri Podolsky

We propose a thermodynamic description of the genuine Kerr-Bertotti-Robinson (Kerr-BR) black hole spacetimes. Contrary to previous studies, such solutions no longer have electric c…

gr-qc2026

Kerr-Newman and genuine Kerr black holes in the Bertotti-Robinson magnetic field

Hryhorii Ovcharenko, Jiri Podolsky

We present a spacetime that describes a rotating and charged black hole immersed in an external magnetic field. This exact solution to the Einstein-Maxwell equations has a surprisi…

gr-qc2026

Circular orbits in spherically symmetric spacetimes and BSW effect with nonzero force

Hryhorii Ovcharenko, O. B. Zaslavskii

We consider circular particle motion under the action of an unspecified force in a static spherically symmetric spacetime. We derive the machinery that allows one to find the force…

gr-qc2026

Comment on the "New Rotating Black Hole in Electromagnetic Fields: Cosmological Horizon without Cosmological Constant''

Hryhorii Ovcharenko

In this comment we discuss some properties of the novel spacetime, recently found in [L. Ma, H. Lü, arXiv:2606.23782]. In particular, we draw attention to the background of this s…

gr-qc2026

Uniqueness of stationary axisymmetric type D black holes with non-aligned electromagnetic field

Hryhorii Ovcharenko, Jiri Podolsky

We demonstrate the uniqueness of the spacetimes recently found by us in [H. Ovcharenko and J. Podolsky, Phys. Rev. D 112 (2025) 064076]. First, we prove that the conformal-to-Carte…

gr-qc2026

Exact Kerr-Newman-(A)dS and other spacetimes in bumblebee gravity: employing a simple generating technique

Hryhorii Ovcharenko

In this work, we show that if the bumblebee field in the Einstein-bumblebee theory is given by its vacuum expectation value () and it is not dynamical ($\partial_μB_ν-…