2002
DOI: 10.1088/1367-2630/4/1/371
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N= 4 gauged supergravity and a IIB orientifold with fluxes

Abstract: We analyze the properties of a spontaneously broken D = 4, N = 4 supergravity without cosmological constant, obtained by gauging translational isometries of its classical scalar manifold. This theory offers a suitable low energy description of the super-Higgs phases of certain Type-IIB orientifold compactifications with 3-form fluxes turned on. We study its N = 3, 2, 1, 0 phases and their classical moduli spaces and we show that this theory is an example of no-scale extended supergravity.

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Cited by 76 publications
(145 citation statements)
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“…The scalar potential of the reduced theory will be obtained in this case by a particular truncation of the original potential [24].…”
Section: Discussionmentioning
confidence: 99%
“…The scalar potential of the reduced theory will be obtained in this case by a particular truncation of the original potential [24].…”
Section: Discussionmentioning
confidence: 99%
“…This gives a term in the potential of the form 14) whereg ind is the induced world-volume metric. In addition there will be corrections due to the shift in warping, found by solving equation (5.6), and due to curvature.…”
Section: Simple Examplesmentioning
confidence: 99%
“…Given the possibly profound implications arising from the study of flux vacua and warped compactifications (a partial list references includes [10][11][12][13][14][15]; useful reviews include [16,17]), it is particularly important to understand the space of such compactifications and their dynamics. While there have been many advances, the inherently greater complexity of these compactifications has left the subject in a significantly more primitive state than that of the traditional Kaluza-Klein compactifications of string/M theory.…”
Section: Introductionmentioning
confidence: 99%
“…The T 0 × T 6 model in the presence of D3-branes, with and without fluxes was constructed in [32,30,31]. The structure of the T 6 ×T 0 model, on the other hand, is somewhat trivial, since there is no room for fluxes to be turned on.…”
Section: 3mentioning
confidence: 99%
“…In these cases, turning on NS-NS and R-R three-form fluxes allows to obtain new string vacua with vanishing vacuum energy, reduced supersymmetry and moduli stabilisation [7,8,9,21,24]. These features can all be understood in terms of an effective gauged supergravity, where certain axion symmetries are gauged [31,30,32]. These are generalised no-scale models [33,34].…”
Section: Introductionmentioning
confidence: 99%