Properties of black hole solutions in the SU(3) Einstein-Yang-Mills-dilaton system

Details Properties of black hole solutions in the SU(3) Einstein-Yang-Mills-dilaton system Properties of black hole solutions in the SU(3) Einstein-Yang-Mills-dilaton system

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrvd..63h7504t&link_type=abstract

Physical Review D, vol. 63, Issue 8, id. 087504

Physics

2

Physics Of Black Holes, Self-Gravitating Systems, Continuous Media And Classical Fields In Curved Spacetime, Thermodynamic Processes, Conduction, Convection, Equations Of State, Black Holes

Scientific paper

We consider black hole solutions in the SU(3) Einstein-Yang-Mills-dilaton system under the static and spherically symmetric ansatz. We reveal some properties which were not investigated before. In particular, we find that there appears a shell-like structure in the energy density distribution outside the horizon which can be interpreted as a symptom of the instability of black holes.

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