English

When Black Holes Meet Kaluza-Klein Bubbles

High Energy Physics - Theory 2009-11-07 v2 General Relativity and Quantum Cosmology

Abstract

We explore the physical consequences of a recently discovered class of exact solutions to five dimensional Kaluza-Klein theory. We find a number of surprising features including: (1) In the presence of a Kaluza-Klein bubble, there are arbitrarily large black holes with topology S^3. (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.

Keywords

Cite

@article{arxiv.hep-th/0210303,
  title  = {When Black Holes Meet Kaluza-Klein Bubbles},
  author = {Henriette Elvang and Gary T. Horowitz},
  journal= {arXiv preprint arXiv:hep-th/0210303},
  year   = {2009}
}

Comments

23 pages, 5 figures, v2: few comments on stability modified