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Stable black hole solutions with non-Abelian fields
Phys. Rev. D 85, 084022 – Published 19 April, 2012
DOI: https://doi.org/10.1103/PhysRevD.85.084022
Abstract
We construct finite mass, asymptotically flat black hole solutions in Einstein—Yang-Mills theory augmented with higher order curvature terms of the gauge field. They possess non-Abelian hair in addition to Coulomb electric charge, and, below some nonzero critical temperature, they are thermodynamically preferred over the Reissner-Nordström solution. Our results indicate the existence of hairy non-Abelian black holes which are stable under linear, spherically symmetric perturbations.
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References (13)
- G. T. Horowitz, arXiv:1002.1722.
- S. S. Gubser, Phys. Rev. Lett. 101, 191601 (2008).
- D. V. Galtsov and M. S. Volkov, Phys. Lett. B 274, 173 (1992).
- M. S. Volkov and D. V. Gal’tsov, Phys. Rep. 319, 1 (1999).
- E. E. Donets and D. V. Gal’tsov, Phys. Lett. B 352, 261 (1995); P. Kanti and E. Winstanley, Phys. Rev. D 61, 084032 (2000).
- B. Zwiebach, Phys. Lett. B 156, 315 (1985).
- T. H. R. Skyrme, Nucl. Phys. 31, 556 (1962).
- D. H. Tchrakian, Phys. Lett. B 150, 360 (1985).
- D. V. Galtsov and A. A. Ershov,Phys. Lett. A 138, 160 (1989); P. Bizon, O. T. Popp, Classical Quantum Gravity 9, 193 (1992).
- M. S. Volkov and D. V. Galtsov, JETP Lett. 50, 346 (1989); H. P. Kuenzle and A. K. Masood-ul-Alam, J. Math. Phys. (N.Y.) 31, 928 (1990); P. Bizon, Phys. Rev. Lett. 64, 2844 (1990).
- A. Messiah, Quantum Mechanics (North-Holland, Amsterdam, 1962).
- A. A. Tseytlin, Nucl. Phys. B501, 41 (1997).
- J. Polchinski, String Theory. Vol. 2: Superstring Theory and Beyond (Cambridge University Press, Cambridge, 1998).