corner
corner

Phys. Rev. D 67, 044015 (2003) [10 pages]

When black holes meet Kaluza-Klein bubbles

Download: PDF (109 kB) Buy this article Export: BibTeX or EndNote (RIS)

Henriette Elvang* and Gary T. Horowitz
Department of Physics, UCSB, Santa Barbara, California 93106

Received 14 November 2002; published 27 February 2003

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.

© 2003 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.67.044015
DOI:
10.1103/PhysRevD.67.044015
PACS:
04.70.Bw

*Email address: elvang@physics.ucsb.edu

Email address: gary@physics.ucsb.edu