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

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

2005-07-27

arxiv.org/abs/hep-th/0507268v2

JHEP 0601:032,2006

Physics

High Energy Physics

High Energy Physics - Theory

18 pages, 7 figures, expaned the discussion

Scientific paper

10.1088/1126-6708/2006/01/032

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 $\alpha=M_{YM}/gM_{Planck}$ (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 $(\alpha, r_H)$ plane where $r_H$ denotes the radius of the black

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