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

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Summary

Introduction and main results

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

Technical review of β-supergravity
Equations of motion in flat indices and Generalized Geometry formalism
NSNS Bianchi identities without sources
Sourceless NSNS Bianchi identities through the literature
Rabc 3!
Rabc 3 ιa
T-dual NS-branes sourcing the Bianchi identities
NS-branes solutions
Smearing warp factors and Poisson equations
Geometric vacua of β-supergravity
Symmetries of the NSNS sector
General case
A new symmetry of β-supergravity
Elements of the T-duality symmetry
To be or not to be geometric
A proof of non-geometry
Geometric backgrounds of β-supergravity and T-duality orbits
Always on a geometric orbit?
On compact purely NSNS vacua
Outlook
A Conventions
B Derivation of the equations of motion in flat indices
Direct approach
Using the generalized geometry formalism
Relation to the subcase with simplifying assumption
Relations to other Bianchi identities in the literature
Findings
D The Q-brane background and the related Bianchi identity

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