Supersymmetric Rotating Black Holes and Attractors
نویسندگان
چکیده
Five-dimensional stringy rotating black holes are embedded into N=2 supergravity interacting with one vector multiplet. The existence of an unbroken supersymmetry of the rotating solution is proved directly by solving the Killing spinor equations. The asymptotic enhancement of supersymmetry near the horizon in the presence of rotation is established via the calculation of the super-curvature. The area of the horizon of the rotating supersymmetric black holes is found to be √ Z3 fix − J2, where Zfix is the extremal value of the central charge in moduli space. ∗ E-mail: [email protected], [email protected], [email protected] SLAC-PUB-9841 Work supported in part by Department of Energy Contract DE-AC03-76SF00515
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تاریخ انتشار 2003