When black holes meet Kaluza-Klein bubbles
- 27 February 2003
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 67 (4) , 044015
- https://doi.org/10.1103/physrevd.67.044015
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 (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.
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This publication has 11 references indexed in Scilit:
- Colliding Kaluza Klein bubblesClassical and Quantum Gravity, 2002
- Clean Time-Dependent String Backgrounds from Bubble BathsJournal of High Energy Physics, 2002
- Generalized Weyl solutionsPhysical Review D, 2002
- Collapse of Kaluza-Klein bubblesPhysical Review D, 1994
- Horizon structure of initial-data sets for axisymmetric two-black-hole collisionsPhysical Review D, 1992
- Negative energy in string theoryPhysics Letters B, 1991
- Higher-dimensional black holes in compactified space-timesPhysical Review D, 1987
- Instability of the Kaluza-Klein vacuumNuclear Physics B, 1982
- Collinear particles and bondi dipoles in general relativityIl Nuovo Cimento (1869-1876), 1964
- Zur GravitationstheorieAnnalen der Physik, 1917