Kerr Black Hole in a Uniform Bertotti-Robinson Magnetic Field: An Exact Solution
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F25%3A10509506" target="_blank" >RIV/00216208:11320/25:10509506 - isvavai.cz</a>
Result on the web
<a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=MYFan0vG8W" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=MYFan0vG8W</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1103/rfgv-ybz5" target="_blank" >10.1103/rfgv-ybz5</a>
Alternative languages
Result language
angličtina
Original language name
Kerr Black Hole in a Uniform Bertotti-Robinson Magnetic Field: An Exact Solution
Original language description
A new class of exact spacetimes in Einstein's gravity, which are Kerr black holes immersed in an external uniform magnetic (or electric) field that is oriented along the rotational axis, is presented. These are axisymmetric stationary solutions to the Einstein-Maxwell equations such that (unlike in the Pleba & nacute;ski-Demia & nacute;ski spacetime) the null directions of the Faraday tensor are not aligned with either of the two principal null directions of the Weyl tensor of algebraic type D (unlike the Kerr-Melvin spacetime). Three physical parameters are the black hole mass m, its rotation a, and the external field value B. For vanishing B the metric directly reduces to standard Boyer-Lindquist form of the Kerr black hole, while for zero m we recover a conformally flat Bertotti-Robinson universe with a uniform Maxwell field. For zero a, the spacetime is contained in the Van den Bergh-Carminati solutions which can be understood as the Schwarzschild black hole in a magnetic field. Our family of black holes with nonaligned Maxwell hair- that can be called the Kerr-Bertotti-Robinson black holes-may find application in various studies ranging from mathematical relativity to relativistic astrophysics.
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
—
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 Letters
ISSN
0031-9007
e-ISSN
1079-7114
Volume of the periodical
135
Issue of the periodical within the volume
18
Country of publishing house
US - UNITED STATES
Number of pages
7
Pages from-to
181401
UT code for WoS article
001610975300001
EID of the result in the Scopus database
2-s2.0-105022231726