1995/04/10 by Burkhard Kleihaus, Jutta Kunz, Abha Sood · 2 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Black hole (networking) #Boundary (topology) #Cosmology and Gravitation Theories #Einstein #Embedding #Gauge theory #Mathematical analysis #Mathematical physics #Mathematics #Particle physics theoretical and experimental studies #Physics #Yang–Mills existence and mass gap #gr-qc #hep-th
paper · pdf · doi:10.1016/0370-2693(95)00664-7
published as Phys.Lett. B354 (1995) 240-246 · LATEX, 16 pages, 5 figures
arxiv created 1995/04/10 · openalex publication_date 1995/07/01 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In the SU(3) Einstein-Yang-Mills system sequences of static spherically symmetric regular solutions and black hole solutions exist for both the SU(2) and the SO(3) embedding. We construct the lowest regular solutions of the SO(3) embedding, missed previously, and the corresponding black holes. The SO(3) solutions are classified according to their boundary conditions and the number of nodes of the matter functions. Both, the regular and the black hole solutions are unstable.