Abstract:Fourteen new stationary points in the scalar potential of SO (8) (8) is extended by fourteen new entries, whose properties have been obtained numerically using the sensitivity backpropagation technique. Eight of the new solutions break the gauge group completely, while three have a residual symmetry of U (1). Three further ones break the gauge group to U (1) × U (1). While the approximate numerical data are somewhat inconclusive, there is evidence that one of these may have a residual N = 1 supersymmetry, henc… Show more
“…Indeed, the solutions 3 (s 1 ,s 2 ) are nonsupersymmetric and still stable with a higher vacuum energy, as can be read from (4.10). This again differs from the situation in the prototypical N = 8 supergravity with SO (8) gauging, where the vacuum that preserves all supersymmetry has the highest potential energy of all known critical points [47].…”
Section: Full Vacua Analysis Of the N = 4 Theorymentioning
We analyse the vacuum structure of isotropic Z 2 × Z 2 flux compactifications, allowing for a single set of sources. Combining algebraic geometry with supergravity techniques, we are able to classify all vacua for both type IIA and IIB backgrounds with arbitrary gauge and geometric fluxes. Surprisingly, geometric IIA compactifications lead to a unique theory with four different vacua. In this case we also perform the general analysis allowing for sources compatible with minimal supersymmetry. Moreover, some relevant examples of type IIB non-geometric compactifications are studied. The computation of the full N = 4 mass spectrum reveals the presence of a number of non-supersymmetric and nevertheless stable AdS 4 vacua. In addition we find a novel dS 4 solution based on a non-semisimple gauging.
“…Indeed, the solutions 3 (s 1 ,s 2 ) are nonsupersymmetric and still stable with a higher vacuum energy, as can be read from (4.10). This again differs from the situation in the prototypical N = 8 supergravity with SO (8) gauging, where the vacuum that preserves all supersymmetry has the highest potential energy of all known critical points [47].…”
Section: Full Vacua Analysis Of the N = 4 Theorymentioning
We analyse the vacuum structure of isotropic Z 2 × Z 2 flux compactifications, allowing for a single set of sources. Combining algebraic geometry with supergravity techniques, we are able to classify all vacua for both type IIA and IIB backgrounds with arbitrary gauge and geometric fluxes. Surprisingly, geometric IIA compactifications lead to a unique theory with four different vacua. In this case we also perform the general analysis allowing for sources compatible with minimal supersymmetry. Moreover, some relevant examples of type IIB non-geometric compactifications are studied. The computation of the full N = 4 mass spectrum reveals the presence of a number of non-supersymmetric and nevertheless stable AdS 4 vacua. In addition we find a novel dS 4 solution based on a non-semisimple gauging.
“…Between 2008 and 2010, there has been also a considerable progress in developing numerical techniques to search for the critical points in the full 70-parameter space. Those methods were used by one of us to explore the vacuum structure of maximal gauged supergravity theories in three dimensions [16,17] and then ported to four dimensions in [18][19][20]. In particular, a new N = 1 supersymmetric critical point S1200000 2 was discovered in [18] and, using the numerical data as a guide, subsequently confirmed analytically in [14].…”
The recent comprehensive numerical study of critical points of the scalar potential of fourdimensional N = 8, SO(8) gauged supergravity using Machine Learning software in [1] has led to a discovery of a new N = 1 vacuum with a triality-invariant SO(3) symmetry. Guided by the numerical data for that point, we obtain a consistent SO(3) × Z 2 -invariant truncation of the N = 8 theory to an N = 1 supergravity with three chiral multiplets. Critical points of the truncated scalar potential include both the N = 1 point as well as two new non-supersymmetric and perturbatively unstable points not found by previous searches. Studying the structure of the submanifold of SO(3) × Z 2 -invariant supergravity scalars, we find that it has a simple interpretation as a submanifold of the 14-dimensional Z 3 2 -invariant scalar manifold (SU(1, 1)/U(1)) 7 , for which we find a rather remarkable superpotential whose structure matches the single bit error correcting (7, 4) Hamming code. This 14-dimensional scalar manifold contains approximately one quarter of the known critical points. We also show that there exists a smooth supersymmetric domain wall which interpolates between the new N = 1 AdS 4 solution and the maximally supersymmetric AdS 4 vacuum. Using holography, this result indicates the existence of an N = 1 RG flow from the ABJM SCFT to a new strongly interacting conformal fixed point in the IR.
Contents2 Following [20], we label the critical points by the first 7 digits of the critical value of the potential. 3 See, however, the construction of a new SO(4)-invariant point in [25].
“…However, one might also be interested in the interplay between gaugings, fluxes and moduli stabilisation: in short, fluxes were introduced in order to achieve moduli stabilisation. Sketchily, the picture in this respect seems to be the following Semisimple gaugings are likely to produce critical points and moduli stabilisation [49][50][51][52], but we will show that their embedding as type II flux compactifications involves highly non-geometric backgrounds. On the other hand, nilpotent gaugings can be obtained from type II compactifications including gauge fluxes [60], but they seem not to be enough to get moduli stabilisation.…”
Section: String Theory Embedding Vs Moduli Stabilisationmentioning
confidence: 99%
“…Note that this critical point relies on the Breitenlohner-Freedman bound to be perturbatively stable. More recently, this classification has been extended with a number of critical points with smaller or trivial invariance groups, which have been obtained with a numerical procedure [49,50].…”
We consider type II (non-)geometric flux backgrounds in the absence of brane sources, and construct their explicit embedding into maximal gauged D = 4 supergravity. This enables one to investigate the critical points, mass spectra and gauge groups of such backgrounds. We focus on a class of type IIA geometric vacua and find a novel, nonsupersymmetric and stable AdS vacuum in maximal supergravity with a non-semisimple gauge group. Our construction relies on a non-trivial mapping between SL(2) × SO(6, 6) fluxes, SU(8) mass spectra and gaugings of E 7(7) subgroups.
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