Einstein-Yang-Mills non-Abelian black holes

Details Einstein-Yang-Mills non-Abelian black holes Einstein-Yang-Mills non-Abelian black holes

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pzetf..50..312v&link_type=abstract

Pis'ma v Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0370-274X), vol. 50, Oct. 10, 1989, p. 312-315. In Russian.

Statistics

Computation

16

Black Holes (Astronomy), Cosmology, Einstein Equations, Gauge Theory, Yang-Mills Theory, Asymptotic Properties, Computational Astrophysics, Electromagnetic Interactions, Phase Transformations, Runge-Kutta Method

Scientific paper

Solutions to the self-consistent system of Einstein-Yang-Mills equations with an SU(2) group are obtained which describe black holes with a non-Abelian structure of gauge fields in the outer regions. Black holes corresponding to solutions of the self-consistent system of Einstein-Yang-Mills equations thus form a larger family than in the previously studied vacuum and electrovacuum cases. This should be considered in discussing the hypothesis of primary black holes formed at an early stage of cosmological expansion, prior to the moment of the phase transition separating electromagnetic interactions.

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