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First Order Description of Black Holes in Moduli Space

We show that the second order field equations characterizing extremal solutions for spherically symmetric, stationary black holes are in fact implied by a system of first order equations given in terms of a prepotential W. This confirms and generalizes the results in hep-th/0702088. When the black h...

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Detalles Bibliográficos
Autores principales: Andrianopoli, Laura, D'Auria, Riccardo, Orazi, Emanuele, Trigiante, Mario
Lenguaje:eng
Publicado: 2007
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1126-6708/2007/11/032
http://cds.cern.ch/record/1040351