2013
DOI: 10.1007/jhep11(2013)056
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Dualities near the horizon

Abstract: In 4-dimensional supergravity theories, covariant under symplectic electricmagnetic duality rotations, a significant role is played by the symplectic matrix M(ϕ), related to the coupling of scalars ϕ to vector field-strengths. In particular, this matrix enters the twisted self-duality condition for 2-form field strengths in the symplectic formulation of generalized Maxwell equations in the presence of scalar fields.In this investigation, we compute several properties of this matrix in relation to the attractor… Show more

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Cited by 16 publications
(19 citation statements)
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References 60 publications
(164 reference statements)
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“…As observed in [84], at least for all automorphism groups of reduced FTS's over simple or semisimple rank-3 Jordan algebras it holds that (see e.g. [87])…”
Section: Let Us Consider a Particularly Simple Anti-symplectic Case mentioning
confidence: 75%
“…As observed in [84], at least for all automorphism groups of reduced FTS's over simple or semisimple rank-3 Jordan algebras it holds that (see e.g. [87])…”
Section: Let Us Consider a Particularly Simple Anti-symplectic Case mentioning
confidence: 75%
“…In this section we shall briefly review the Freudenthal duality in ungauged supergravity [27,29,31], and subsequently generalize it to the gauged case.…”
Section: Freudenthal Dualitymentioning
confidence: 99%
“…It can be defined as an anti-involutive, nonlinear map acting on symplectic spaces, in particular on the representation space in which the electromagnetic charges of the black holes sit. After its introduction in [27] in the context of the so-called U -duality Lie groups of type E 7 [28] in extended supergravity theories, interesting relations between Freudenthal duality, the Hessian matrix of the black hole entropy and the rigid special (pseudo-)Kähler metric of the prehomogeneous vector spaces associated to the Uorbits, were discovered and studied in [29,30]. In [31] Freudenthal duality was proved to be a symmetry not only of the classical Bekenstein-Hawking entropy, but also of the critical points of the black hole potential.…”
Section: Introductionmentioning
confidence: 99%
“…the standard form of this invariant can be expressed in the following manifestly Sp(6, R)-invariant form (see for instance [76])…”
Section: The Quartic Invariant In the 14 ′mentioning
confidence: 99%