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20222026
most citedKerr black hole in a uniform Bertotti-Robinson magnetic field: An exact solution

26 citations · 74 across the 19 of their papers we have counts for

collaborators

19 papers

gr-qc2026

Global structure of Kerr-Newman-BR spacetime

Hryhorii Ovcharenko

We conduct an investigation of the global structure of Kerr-Newman-BR spacetime and its various subcases such as Schwarzschild-BR spacetime. In this work, we extend the result of o…

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

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 so…

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

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

Static black holes in an external uniform electromagnetic field: Reissner-Nordstrom accelerating in Bertotti-Robinson

Hryhorii Ovcharenko, Jiri Podolsky

We provide a detailed analysis of the non-twisting subcase of the large class of type D black holes with a non-aligned electromagnetic field, presented recently in [H. Ovcharenko a…

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-\par…

gr-qc2025

Hidden symmetries and separability structures of Ovcharenko-Podolský and conformal-to-Carter spacetimes

Finnian Gray, David Kubiznak, Hryhorii Ovcharenko +1

Recently, a remarkable new class of spacetimes describing black holes immersed in a non-aligned electromagnetic field has been found. While still of type D, this class goes beyond…

gr-qc2025

A novel class of rotating black holes with non-aligned electromagnetic field

Hryhorii Ovcharenko, Jiri Podolsky

We present a new class of expanding and twisting solutions to the Einstein-Maxwell equations of algebraic type D, where the null eigendirections of the Faraday tensor are not align…

gr-qc2025★ 17 cited

New class of rotating charged black holes with nonaligned electromagnetic field

Hryhorii Ovcharenko, Jiří Podolský

We present a large family of twisting and expanding solutions to the Einstein-Maxwell equations of algebraic type D, for which the two double principal null directions (PNDs) of th…

gr-qc2025★ 26 cited

Kerr black hole in a uniform Bertotti-Robinson magnetic field: An exact solution

Jiri Podolsky, Hryhorii Ovcharenko

A new class of exact spacetimes in Einstein's gravity, which are Kerr black holes immersed in an external magnetic (or electric) field that is asymptotically uniform and oriented a…

gr-qc2025

Near-horizon behavior of nonequatorial accelerated particle motion and high energy particle collisions

H. V. Ovcharenko, O. B. Zaslavskii

We consider motion of a particle in the background of a stationary axially symmetric generic black hole. A particle experiences the action of a force of unspecified nature. We requ…

gr-qc2025★ 2 cited

Naked and truly naked rotating black holes

H. V. Ovcharenko, O. B. Zaslavskii

Previously, it was noticed that in some space-times with Killing horizons some curvature components, responsible for tidal forces, small or even zero in the static frame, become en…

gr-qc2025★ 14 cited

Revisiting black holes of algebraic type D with a cosmological constant

Hryhorii Ovcharenko, Jiri Podolsky, Marco Astorino

As an extension of our previous work [1] (arXiv:2409.02308), we study a complete family of type D black holes with Kerr-like rotation, NUT twist, acceleration, electric and magneti…

gr-qc2024★ 12 cited

Black holes of type D revisited: relating their various metric forms

Hryhorii Ovcharenko, Jiri Podolsky, Marco Astorino

We investigate a complete family of spacetimes which represent black holes with rotation, NUT twist, acceleration, electric and magnetic charges. These are exact solutions of the E…

gr-qc2024★ 3 cited

High energy head-on particle collisions near event horizons: classifcation of scenarios

H. V. Ovcharenko, O. B. Zaslavskii

We consider head-on collisions of two particles near the event horizon. Particle 1 is outgoing, particle 2 is ingoing. We elucidate, in which case the energy in the cent…

gr-qc2023

Dynamics of redshift/blueshift during free fall under the Schwarzschild horizon

H. V. Ovcharenko, O. B. Zaslavskii

We consider a free-falling observer who crosses the event horizon in the Schwarzschild background. In the course of this fall, he/she can receive signals from an object (like a sta…

gr-qc2022

Axially symmetric rotating black hole with regular horizons

H. V. Ovcharenko, O. B. Zaslavskii

We consider the metric of an axially symmetric rotating black hole. We do not specify the concrete form of a metric and rely on its behavior near the horizon only. Typically, it is…