1997
DOI: 10.1016/s0370-2693(97)00144-5
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Electrically charged black-holes for the heterotic string compactified on a (10 - D)-torus

Abstract: We show that the most general stationary electrically charged black-hole solutions of the heterotic string compactified on a (10−D)-torus (where D > 3) can be obtained by using the solution generating transformations of Sen acting on the Myers and Perry metric. The conserved charges labeling these black-hole solutions are the mass, the angular momentum in all allowed commuting planes, and 36 − 2D electric charges. General properties of these black-holes are also studied.

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Cited by 15 publications
(20 citation statements)
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“…In particular, they include the elusive electric rotating black holes of the Einstein-Maxwell theory (a = 0), which for the first time are described in these regimes. They also include the previously known charged rotating black holes in Kaluza-Klein theory [9,10], whose properties we show are accurately reproduced in the appropriate regime. We shall argue that in the blackfold regime all these black holes are unstable even when they are close to extremality and slowly rotating.…”
Section: D−3mentioning
confidence: 59%
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“…In particular, they include the elusive electric rotating black holes of the Einstein-Maxwell theory (a = 0), which for the first time are described in these regimes. They also include the previously known charged rotating black holes in Kaluza-Klein theory [9,10], whose properties we show are accurately reproduced in the appropriate regime. We shall argue that in the blackfold regime all these black holes are unstable even when they are close to extremality and slowly rotating.…”
Section: D−3mentioning
confidence: 59%
“…We can unify the description of fluids with either of these currents if we introduce the projector onto the space parallel to the particle/string worldline/sheet, 9) and onto directions in W p+1 orthogonal to it,…”
Section: Jhep04(2011)013mentioning
confidence: 99%
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“…We discuss rotating black holes in heterotic string on T 10−D (4 ≤ D ≤ 9) with general U (1) 36−2D electric charge configurations [184,449]. The generating solution is parameterized by the ADM mass M BH (or alternatively the non-extremality parameter m), […”
Section: Rotating Black Holes In Higher Dimensionsmentioning
confidence: 99%
“…For such configurations, the equations depend only on the radial variable r and the extra-dimension variable z and are solved to first order in the angular momentum parameter. To simplify the general picture, we shall restrict here to the case of EM theory, 18 Except for special values of the dilaton coupling constant where the solutions can be generated from the Myers-Perry black holes following the techniques in [48], [49].…”
Section: Slowly Rotating Charged Nubsmentioning
confidence: 99%