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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&apos;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 &amp; nacute;ski-Demia &amp; 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

  • Czech description

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