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arXiv · hep-th/0507268

Non-BPS Black holes in N=4 Supersymmetric Yang-Mills Theory Coupled to Gravity

Theodora Ioannidou·Burkhard Kleihaus
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Abstract

We construct non-BPS regular and black hole solutions of N=4 SU(N) supersymmetric Yang-Mills theory coupled to Einstein gravity. Our numerical studies reveal a number of interesting phenomena when the gravitational constant $α=M_{YM}/gM_{Planck}$ (where $M_{Planck}$ is the Planck mass and $M_{YM}$ is the monopole mass) is either weak (flat limit) or comparable to the Yang-Mills interaction. In fact, black hole solutions exist in a certain bounded domain in the $(α, r_H)$ plane where $r_H$ denotes the radius of the black

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Theodora Ioannidou, Burkhard Kleihaus. 2005-11-21. Non-BPS Black holes in N=4 Supersymmetric Yang-Mills Theory Coupled to Gravity. https://doi.org/10.1088/1126-6708%2F2006%2F01%2F032

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