Slowly Rotating Non-Abelian Black Holes
Mikhail S. Volkov, Norbert Straumann
Abstract
It is shown that the well-known non-Abelian static SU(2) black hole solutions have rotating generalizations, provided that the hypothesis of linearization stability is accepted. Surprisingly, this rotating branch has an asymptotically Abelian gauge field with an electric charge that cannot vanish, although the non-rotating limit is uncharged. We argue that this may be related to our second finding, namely that there are no globally regular slowly rotating excitations of the particle-like Bartnik-McKinnon solutions.
Create a lesson
Related papers
Heavy-Heavy-Light-Light correlators from holography on the worldsheet
Matías Colaneri, Diego H. Correa, Víctor I. Giraldo-Rivera et al.
Post-Newtonian theory in de Sitter and anti-de Sitter spacetimes
R. Loganayagam, Avi Wadhwa
Thermal AdS two-point functions and loop induced effective one-point vertices
Astha Kakkar
Giant Wilson loops from Fredholm determinants
Ludvig Chen, Victor Mishnyakov, Konstantin Zarembo
Degeneracy graph determinants and higher-dimensional Young diagrams
Sanjaye Ramgoolam, Michał Studziński
Black hole cohomologies in N=4 SYM
Seunggyu Kim, Jehyun Lee, Siyul Lee et al.