2000/08/03 by Burkhard Kleihaus, B. Kleihaus, Jutta Kunz +1 · 3 citations
Engineering · Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Fluid Dynamics and Turbulent Flows #gr-qc #hep-th
paper · pdf · doi:10.1016/s0370-2693(00)01162-x
published as Phys.Lett. B494 (2000) 130-134 · 10 pages, including 3 eps figures, LaTex format
arxiv created 2000/08/03 · openalex publication_date 2000/11/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We construct static axially symmetric black holes in SU(2) Einstein-Yang-Mills-Higgs theory. Located in between a monopole-antimonopole pair, these black holes possess magnetic dipole hair. The difference of their mass and their horizon mass equals the mass of the regular monopole-antimonopole solution, as expected from the isolated horizon framework.