Abstract
We develop a method of constructing generic black hole attractor solutions, both BPS and non-BPS, single-centered as well as multi-centered, in a large class of 4D \(\mathcal{N}\,=\,2\) supergravities coupled to vector-multiplets with cubic prepotentials. The method is applicable to models for which the 3D moduli spaces obtained via c ∗-map are symmetric coset spaces. All attractor solutions in such a 3D moduli space can be constructed algebraically in a unified way. Then the 3D attractor solutions are mapped back into four dimensions to give 4D extremal black holes.
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Acknowledgements
The author would like to thank D. Gaiotto and M. Padi for the collaboration on the project this talk was based on. We are grateful to A. Neitzke and J. Seo for helpful discussions. It is also a pleasure to thank the warm hospitality of the School of Attractor Mechanism (2007). The work is supported by DOE grant DE-FG02-91ER40654.
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Li, W. (2010). Non-supersymmetric Attractors in Symmetric Coset Spaces. In: Bellucci, S. (eds) The Attractor Mechanism. Springer Proceedings in Physics, vol 134. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-10736-8_6
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DOI: https://doi.org/10.1007/978-3-642-10736-8_6
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