Subtracted Geometry from Harrison Transformations: II
arXiv:1305.2800 · doi:10.1007/JHEP07(2013)089
Abstract
We extend our previous study (arXiv:1203.5088) to the case of five-dimensional multi-charge black holes, thus showing that these configurations and their subtracted geometries also lie in a 3d duality orbit. In order to explore the 3d duality orbit, we do a timelike reduction from 5d to 4d and a spacelike reduction from 4d to 3d. We present our analysis in the notation of Euclidean N=2 supergravity and its c-map. We also relate our analysis to that of Cvetič, Guica, and Saleem.
18 pages, no figures; v2: a typo in equation (3.18) fixed, no other changes
References in corpus (7)
- Universal BPS structure of stationary supergravity solutions
- Special Geometry of Euclidean Supersymmetry III: the local r-map, instantons and black holes
- Subtracted Geometry From Harrison Transformations
- Separability of Black Holes in String Theory
- Conformal Symmetry for Black Holes in Four Dimensions and Irrelevant Deformations
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Cited by in corpus (7)
- Entropy-Product Rules for Charged Rotating Black Holes
- An Inverse Scattering Construction of the JMaRT Fuzzball
- Quasi-Normal Modes for Subtracted Rotating and Magnetised Geometries
- Time-like reductions of five-dimensional supergravity
- Smooth non-extremal D1-D5-P solutions as charged gravitational instantons
- Geroch Group Description of Bubbling Geometries
- The Spectrum of Static Subtracted Geometries