Constituent Model of Extremal non-BPS Black Holes
arXiv:0903.0719 · doi:10.1088/1126-6708/2009/07/052
Abstract
We interpret extremal non-BPS black holes in four dimensions as threshold bound states of four 1/2-BPS constituents. We verify the no-force condition for each of the primitive constituents in the probe approximation. Our computations are for a seed solution with charges and equal -fields, but symmetries extend the result to any U-dual frame. We make the constituent model for the system explicit, and also discuss a duality frame where the constituents are branes at angles. We demonstrate stability of the constituent model in the weak coupling description of the constituent D-branes. We discuss the relation between the BPS and non-BPS branches of configuration space.
29 pages; v2. references added
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