期刊
NUCLEAR PHYSICS B
卷 824, 期 1-2, 页码 239-253出版社
ELSEVIER
DOI: 10.1016/j.nuclphysb.2009.09.003
关键词
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资金
- MIUR-PRIN [20075ATT78]
- Fondazione Cariparo Excellence
- D.O.E. [DE-FG03-91ER40662]
- CERN-PH-TH
We derive explicitly the superpotential W for the non-BPS branch of N = 2 extremal black holes in terms of duality invariants of special geometry. Although this is done for a one-modulus case (the t(3) model), the example gives Z not equal 0 black holes and captures the basic distinction from previous attempts on the quadratic series (vanishing C tensor) and front the other Z = 0 cases. The superpotential W turns out to be a non-polynomial expression (containing radicals) of the basic duality invariant quantities. These are the same which enter in the quartic invariant I-4 for N = 2 theories based oil symmetric spaces. Using the flow equations generated by W, we also provide the analytic general solution for the warp factor and for the scalar field Supporting the non-BPS black holes. (c) 2009 Elsevier B.V. All rights reserved.
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