Abstract
In the first half of the paper, we study in details NS-branes, including the NS5-brane, the Kaluza-Klein monopole and the exotic $5_2^2$- or Q-brane, together with Bianchi identities for NSNS (non)-geometric fluxes. Four-dimensional Bianchi identities are generalized to ten dimensions with non-constant fluxes, and get corrected by a source term in presence of an NS-brane. The latter allows them to reduce to the expected Poisson equation. Without sources, our Bianchi identities are also recovered by squaring a nilpotent $Spin(D,D) \times \mathbb{R}^+$ Dirac operator. Generalized Geometry allows us in addition to express the equations of motion explicitly in terms of fluxes. In the second half, we perform a general analysis of ten-dimensional geometric backgrounds with non-geometric fluxes, in the context of $\beta$-supergravity. We determine a well-defined class of such vacua, that are non-geometric in standard supergravity: they involve $\beta$-transforms, a manifest symmetry of $\beta$-supergravity with isometries. We show as well that these vacua belong to a geometric T-duality orbit.
Highlights
Introduction and main resultsIn the last few years, there has been a renewed interest in the topic of non-geometry and non-geometric fluxes
In the first half of the paper, we study in details N S-branes, including the N S5brane, the Kaluza-Klein monopole and the exotic 522- or Q-brane, together with Bianchi identities for NSNS-geometric fluxes
We focus on Bianchi identities (BI) for the NSNS fluxes, and how they are corrected on specific backgrounds corresponding to NS-branes
Summary
In the last few years, there has been a renewed interest in the topic of non-geometry and non-geometric fluxes (for reviews see [2,3,4]). We take in this paper the last two points of view, and study the Bianchi identities for NSNS fluxes, the related NS-branes, and properties of further ten-dimensional backgrounds with non-geometric fluxes. We verify in appendix D.1 that it satisfies the β-supergravity equations of motion Two examples (or at least their NSNS sector) are helpful: the Q-brane mentioned previously, and the toroidal example studied in details in [1, 3, 37] Their standard supergravity description is non-geometric, and T-dual to a geometric one. We turn to the rewriting of its equations of motion in flat indices
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