Subtracted Geometry From Harrison Transformations
arXiv:1203.5088 · doi:10.1007/JHEP07(2012)086
Abstract
We consider the rotating non-extremal black hole of N=2 D=4 STU supergravity carrying three magnetic charges and one electric charge. We show that its subtracted geometry is obtained by applying a specific SO(4,4) Harrison transformation on the black hole. As previously noted, the resulting subtracted geometry is a solution of the N=2 S=T=U supergravity.
11 pages main text; total 24 pages; Latex file; v2 typos corrected + ref added; v3 results significantly strengthened, changes in section 3.1 and appendix C, version to appear in JHEP
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Cited by in corpus (9)
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- An Inverse Scattering Construction of the JMaRT Fuzzball
- Black Holes with Intrinsic Spin
- Vacuum Polarization of STU Black Holes and their Subtracted Geometry Limit
- Thermodynamics of Asymptotically Conical Geometries
- Attraction, with Boundaries
- Entanglement entropy of subtracted geometry black holes