Global Charges of Stationary Non-Abelian Black Holes

Burkhard Kleihaus, Jutta Kunz, and Francisco Navarro-Lérida
Phys. Rev. Lett. 90, 171101 – Published 2 May 2003

Abstract

We consider stationary axially symmetric black holes in SU(2) Einstein-Yang-Mills-dilaton theory. We present a mass formula for these stationary non-Abelian black holes, which also holds for Abelian black holes. The presence of the dilaton field allows for rotating black holes, which possess nontrivial electric and magnetic gauge fields, but do not carry a non-Abelian charge. We further present a new uniqueness conjecture.

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  • Received 21 October 2002

DOI:https://doi.org/10.1103/PhysRevLett.90.171101

©2003 American Physical Society

Authors & Affiliations

Burkhard Kleihaus

  • Department of Mathematical Physics, University College, Dublin, Belfield, Dublin 4, Ireland

Jutta Kunz

  • Fachbereich Physik, Universität Oldenburg, D-26111 Oldenburg, Germany

Francisco Navarro-Lérida

  • Departamento de Física Teórica II, Ciencias Físicas, Universidad Complutense de Madrid, E-28040 Madrid, Spain

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Issue

Vol. 90, Iss. 17 — 2 May 2003

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