pith. sign in

arxiv: hep-th/9909205 · v2 · submitted 1999-09-29 · ✦ hep-th · astro-ph· hep-ph

Brane-World Black Holes

A. Chamblin , S.W. Hawking , H.S. Reall This is my paper
classification ✦ hep-th astro-phhep-ph
keywords blackbranedomainfiveholeholeswallanti-de
0
0 comments X
read the original abstract

Gravitational collapse of matter trapped on a brane will produce a black hole on the brane. We discuss such black holes in the models of Randall and Sundrum where our universe is viewed as a domain wall in five dimensional anti-de Sitter space. We present evidence that a non-rotating uncharged black hole on the domain wall is described by a ``black cigar'' solution in five dimensions.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Localized five-dimensional rotating brane-world black hole Analytically Connected to an to an AdS$_5$ boundary

    gr-qc 2025-09 unverdicted novelty 7.0

    Analytic construction of a 5D rotating braneworld black hole using Janis-Newman algorithm in Hopf coordinates that induces Kerr on the brane and connects to AdS5 boundary through bulk anisotropic fluid.

  2. Kerr-Schild Double Copy of the Randall-Sundrum Black String

    hep-th 2026-04 unverdicted novelty 6.0

    Kerr-Schild double copy of the RS II black string produces a sourceless Maxwell single copy and a warp-induced massive scalar zeroth copy, with an alternative splitting giving inequivalent gauge and scalar fields.

  3. On regular black strings spacetimes in nonlinear electrodynamics

    gr-qc 2026-03 unverdicted novelty 6.0

    No regular purely electric black strings exist in NED recovering the Maxwell limit, but regular cylindrical Bardeen and Hayward analogues are constructed with finite curvature.

  4. Investigating the interplay of the braneworld gravity and the plasma environment on the black hole shadow

    gr-qc 2025-12 unverdicted novelty 4.0

    Negative tidal charge enlarges the shadow of rotating braneworld black holes while inhomogeneous plasma shrinks it and homogeneous plasma enlarges it; EHT data limits q to roughly -1.15 to 0.45 for M87* in the low-den...

  5. Holographic entanglement entropy and complexity for the cosmological braneworld model

    hep-th 2025-05 unverdicted novelty 3.0

    Time-dependent holographic entanglement entropy and complexity are computed perturbatively for braneworld FLRW universes with radiation, matter, and exotic matter by using time-dependent brane positions in black brane...