New class of rotating charged black holes with nonaligned electromagnetic field

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F25%3A10506808" target="_blank" >RIV/00216208:11320/25:10506808 - isvavai.cz</a>

Výsledek na webu

<a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=B5vwXl6Obd" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=B5vwXl6Obd</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1103/8wkz-th6v" target="_blank" >10.1103/8wkz-th6v</a>

Jazyk výsledku

angličtina

Název v původním jazyce

New class of rotating charged black holes with nonaligned electromagnetic field

Popis výsledku v původním jazyce

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 the Weyl tensor are not aligned with the null eigendirections of the Faraday tensor. In addition to systematically deriving this new class, we present its various metric forms and convenient parametrizations. We show that in BoyerLindquist-type coordinates these solutions depend on seven parameters, namely the Kerr and NUT (Newman-Unti-Tamburino) twist parameters a and l, mass parameter m, acceleration alpha, strength of the Maxwell field c , and angular parameters beta, gamma that represent two duality rotations of the Faraday tensor, which include the rotation between the electric and magnetic charges generating the aligned part of the Maxwell field. This coordinate parametrization, analogous to the Griffiths-Podolsk &amp; yacute; form of the Pleba &amp; nacute;skiDemia &amp; nacute;ski solutions, allows us to perform various limits, explicitly identify the subcases, and determine the physical interpretation of the new class. Interestingly, by considering the limit with no acceleration (alpha -* 0), one obtains either the famous Kerr-Newman-NUT black holes (if the parameter c remains constant) or the novel Kerr-Bertotti-Robinson black holes, announced recently in our work [Kerr black hole in a uniform Bertotti-Robinson magnetic field: An exact solution, Phys. Rev. Lett. (to be published), 10.1103/rfgvybz5.] (if c -* infinity while alpha c = const:). We may thus conclude that this new class of spacetimes represents twisting charged accelerating black holes, immersed in an external magnetic (or electric) field. In the nontwisting subcase, we obtain the previously known solution of Van den Bergh-Carminati.

Název v anglickém jazyce

New class of rotating charged black holes with nonaligned electromagnetic field

Popis výsledku anglicky

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 the Weyl tensor are not aligned with the null eigendirections of the Faraday tensor. In addition to systematically deriving this new class, we present its various metric forms and convenient parametrizations. We show that in BoyerLindquist-type coordinates these solutions depend on seven parameters, namely the Kerr and NUT (Newman-Unti-Tamburino) twist parameters a and l, mass parameter m, acceleration alpha, strength of the Maxwell field c , and angular parameters beta, gamma that represent two duality rotations of the Faraday tensor, which include the rotation between the electric and magnetic charges generating the aligned part of the Maxwell field. This coordinate parametrization, analogous to the Griffiths-Podolsk &amp; yacute; form of the Pleba &amp; nacute;skiDemia &amp; nacute;ski solutions, allows us to perform various limits, explicitly identify the subcases, and determine the physical interpretation of the new class. Interestingly, by considering the limit with no acceleration (alpha -* 0), one obtains either the famous Kerr-Newman-NUT black holes (if the parameter c remains constant) or the novel Kerr-Bertotti-Robinson black holes, announced recently in our work [Kerr black hole in a uniform Bertotti-Robinson magnetic field: An exact solution, Phys. Rev. Lett. (to be published), 10.1103/rfgvybz5.] (if c -* infinity while alpha c = const:). We may thus conclude that this new class of spacetimes represents twisting charged accelerating black holes, immersed in an external magnetic (or electric) field. In the nontwisting subcase, we obtain the previously known solution of Van den Bergh-Carminati.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10300 - Physical sciences

Projekt

<a href="/cs/project/GA23-05914S" target="_blank" >GA23-05914S: Pokročilé techniky aplikované na přesné prostoročasy s černými dírami a gravitačními vlnami</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2025

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Physical Review D

ISSN

2470-0010

e-ISSN

2470-0029

Svazek periodika

112

Číslo periodika v rámci svazku

6

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

27

Strana od-do

064076

Kód UT WoS článku

001583141300007

EID výsledku v databázi Scopus

2-s2.0-105020637838