New class of rotating charged black holes with nonaligned electromagnetic field
The result's identifiers
Result code in 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>
Result on the web
<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>
Alternative languages
Result language
angličtina
Original language name
New class of rotating charged black holes with nonaligned electromagnetic field
Original language description
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 & yacute; form of the Pleba & nacute;skiDemia & 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.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10300 - Physical sciences
Result continuities
Project
<a href="/en/project/GA23-05914S" target="_blank" >GA23-05914S: Advanced Techniques Applied to Black-Hole and Gravitational-Wave Exact Spacetimes</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2025
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Physical Review D
ISSN
2470-0010
e-ISSN
2470-0029
Volume of the periodical
112
Issue of the periodical within the volume
6
Country of publishing house
US - UNITED STATES
Number of pages
27
Pages from-to
064076
UT code for WoS article
001583141300007
EID of the result in the Scopus database
2-s2.0-105020637838