All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Rotating Carroll black holes: A no go theorem

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F25%3A10511998" target="_blank" >RIV/00216208:11320/25:10511998 - isvavai.cz</a>

  • Result on the web

    <a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=hnlA9hxvie" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=hnlA9hxvie</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/twv1-kphf" target="_blank" >10.1103/twv1-kphf</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Rotating Carroll black holes: A no go theorem

  • Original language description

    Recently, there has been a lot of interest in Carroll black holes and in particular whether or not one could find a Carrollian analog of a rotating black hole spacetime. Here we show that every stationary and axisymmetric solution (and thence also a black hole) of Carrollian general relativity in any number of d &gt; 3 dimensions is necessarily also static (up to a &quot;topological rotation&quot;). The case of d = 3 dimensions is special. There, the topological rotation is important and one can have a rotating Carroll Ba &amp; nacute;ados-Teitelboim-Zanelli black hole, obtained from a static one by the Carroll boost accompanied by the reidentification of the angular coordinate, similar to what happens in the Lorentzian case. We also find a Carrollian analog of an accelerating black hole, showing that Schwarzschild is not the only possible stationary and axisymmetric Carroll black hole in four dimensions. A generalization of the no go theorem to include Maxwell, dilatonic, and axionic matter fields is also discussed.

  • 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/GA23-07457S" target="_blank" >GA23-07457S: Hidden Symmetries and Black Hole Chemistry</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

    12

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    8

  • Pages from-to

    L121504

  • UT code for WoS article

    001651706000004

  • EID of the result in the Scopus database

    2-s2.0-105025700874