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stu Black Holes Unveiled
AbstractThe general solutions of the radial attractor flow equations for extremal black holes, both for non-BPS with non-vanishing central charge Z and for Z = 0, are obtained for the so-called stu model, the minimal rank-3 N = 2 symmetric supergravity in d = 4 space-time dimensions. Comparisons with previous results, as well as the fake supergravity (first order) formalism and an analysis of the BPS bound all along the non-BPS attractor flows and of the marginal stability of corresponding D-brane configurations, are given.
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Bellucci, S.; Ferrara, S.; Marrani, A.; Yeranyan, A. stu Black Holes Unveiled. Entropy 2008, 10, 507-555.View more citation formats
Bellucci S, Ferrara S, Marrani A, Yeranyan A. stu Black Holes Unveiled. Entropy. 2008; 10(4):507-555.Chicago/Turabian Style
Bellucci, Stefano; Ferrara, Sergio; Marrani, Alessio; Yeranyan, Armen. 2008. "stu Black Holes Unveiled." Entropy 10, no. 4: 507-555.
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