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Circle compactifications of Minkowski$_D$ solutions, flux vacua and solitonic branes

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arxiv 2412.15102 v1 pith:CB3ZIAWS submitted 2024-12-19 hep-th

classification hep-th
keywords minksolutionsbranescirclecompactificationsconditionsconstructflux
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

G-structure techniques are used to construct broad classes of circle compactifications of Mink$_{D+1}$ solutions to Mink$_{D}$ embedded into type II supergravity for $D=1,...5$. Under a certain assumptions we show that the conditions that imply supersymmetry for Mink$_{D+1}$ imply those of the Mink$_{D}$ solution, but that Bianchi identities of the fluxes must be modified. This realises an off shell solution generating technique for supersymmetric solutions or a "supersymmetry generating" technique. Along the way it is necessary for us to derive G structure conditions for general ${\cal N}=(1,0)$ supersymmetric Mink$_2$ solutions and a restricted class of Mink$_1$ solutions. We apply our results to construct some simple Minkowski flux vacua before turning our attention to "solitonic branes" which are generalisations of the AdS soliton. We are able to generalise known examples in two ways: 1) to embed them in terms of generic Sasaki Einstein manifolds. 2) To modify the harmonic factor to include D$p$ brane sources at one end of the space.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Universal Observables, SUSY RG-Flows and Holography

    hep-th 2025-06 conditional novelty 6.0 of 10

    New Type IIB, 11d, and Type IIA supergravity flows dual to twisted-compactified 4d SCFTs yield a universal factorization of Wilson loops, flow central charges, and complexity.

  2. Supersymmetric Moduli Space and Vacua with Vector Fields in $D=4$ Gauged $\mathcal{N}=8$ Supergravity

    hep-th 2026-07 accept novelty 5.0 of 10

    Four-charge supersymmetric AdS solitons in the dilatonic STU model have a compact moduli space fixed by |ψ₁|+|ψ₂|+|ψ₃|+|ψ₄|=√2 L, with scalar VEVs determined by the Wilson lines.

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