Abstract
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.
| Original language | English |
|---|---|
| Article number | 087504 |
| Journal | Physical Review D |
| Volume | 63 |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - 2001 Dec 1 |
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ASJC Scopus subject areas
- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)
Cite this
Kei-Ichi, M., & Inada, M. (2001). Properties of black hole solutions in the SU(3) Einstein-Yang-Mills-dilaton system. Physical Review D, 63(8), [087504]. https://doi.org/10.1103/PhysRevD.63.087504