2009
DOI: 10.1103/physrevd.80.045020
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More onN=8attractors

Abstract: We examine a few simple extremal black hole configurations of N ¼ 8, d ¼ 4 supergravity. We first elucidate the relation between the BPS Reissner-Nördstrom black hole and the non-BPS Kaluza-Klein dyonic black hole. Their classical entropy, given by the Bekenstein-Hawking formula, can be reproduced via the attractor mechanism by suitable choices of symplectic frame. Then, we display the embedding of the axion-dilaton black hole into N ¼ 8 supergravity.

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Cited by 21 publications
(52 citation statements)
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“…This paper aims to study d-geometries in a framework broader than N = 2, considering the r-map for N ≥ 2 extended supergravities along the lines of previous work on this 4D/5D relation in the context of black hole supergravity solutions and their attractors [7,8,9]. Due to the structure of 5D spinors, these generalized d-geometries encompass all extended supergravities with a number of supercharges multiple of 8, and thus an even number of supersymmetries N = 2, 4, 6, 8.…”
Section: Introductionmentioning
confidence: 99%
“…This paper aims to study d-geometries in a framework broader than N = 2, considering the r-map for N ≥ 2 extended supergravities along the lines of previous work on this 4D/5D relation in the context of black hole supergravity solutions and their attractors [7,8,9]. Due to the structure of 5D spinors, these generalized d-geometries encompass all extended supergravities with a number of supercharges multiple of 8, and thus an even number of supersymmetries N = 2, 4, 6, 8.…”
Section: Introductionmentioning
confidence: 99%
“…It is worth recalling that the case n = 0 of the truncation (6.6) has been considered in section 5 of [68] (see also the considerations in subsection 8.3.1).…”
Section: Jhep06(2012)074mentioning
confidence: 99%
“…, 4) (see e.g. [39,[66][67][68]). In group-theoretical terms, the "degeneration" truncating procedure under consideration goes as follows:…”
Section: Jhep06(2012)074mentioning
confidence: 99%
“…The attractor mechanism [43] (see also the more recent reference [44]) has been one of the main tools for the study of supersymmetric black-hole solutions. Our results establish a clear distinction between the scalars which are driven by the electric and magnetic charges of the vector fields (which would belong to the would-be vector multiplets of the associated N = 2 truncation) and, therefore, subject to the attractor mechanism, and those that are not (which would belong to the would-be hypermultiplets of the associated N = 2 truncation).…”
Section: Discussionmentioning
confidence: 99%