When black holes meet Kaluza-Klein bubbles

Henriette Elvang and Gary T. Horowitz
Phys. Rev. D 67, 044015 – Published 27 February 2003
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Abstract

We explore the physical consequences of a recently discovered class of exact solutions to the five dimensional Kaluza-Klein theory. We find a number of surprising features including the following: (1) In the presence of a Kaluza-Klein bubble, there are arbitrarily large black holes with topology S3. (2) In the presence of a black hole or a black string, there are expanding bubbles (with de Sitter geometry) which never reach null infinity. (3) A bubble can hold two black holes of arbitrary size in static equilibrium. In particular, two large black holes can be close together without merging to form a single black hole.

  • Received 14 November 2002

DOI:https://doi.org/10.1103/PhysRevD.67.044015

©2003 American Physical Society

Authors & Affiliations

Henriette Elvang* and Gary T. Horowitz

  • Department of Physics, UCSB, Santa Barbara, California 93106

  • *Email address: elvang@physics.ucsb.edu
  • Email address: gary@physics.ucsb.edu

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Issue

Vol. 67, Iss. 4 — 15 February 2003

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