Rotating Kaluza-Klein Black Holes

1999/09/30 by Finn Larsen · 30 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #hep-th

paper · pdf · doi:10.1016/s0550-3213(00)00064-x

published as Nucl.Phys. B575 (2000) 211-230 · 27 pages; v2: refs added, improved discussion of the extremal limit; v3: note added, to appear in Nucl. Phys. B

arxiv created 2000/02/04 · openalex publication_date 2000/05/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30

Abstract

All regular four-dimensional black holes are constructed in the theory obtained by Kaluza-Klein reduction of five-dimensional Einstein gravity. They are interpreted in string theory as rotating bound states of D0- and D6-branes. Conservation of angular momentum is important for the stability of the bound states. The thermodynamics, the duality symmetries, and the near-horizon limit are explored.

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