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Holography for Confined and Deformed Theories: TsT-Generated Solutions in type IIB Supergravity

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arxiv 2410.00094 v2 pith:ABE55XGA submitted 2024-09-30 hep-th

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

In this paper, we present a series of solutions of type IIB Supergravity, obtained through the TsT deformation of a seed background that is holographically dual to ${\cal N}=4$ Super Yang-Mills theory compactified on a circle (with a twist). We explore various holographic observables, focusing on disentangling the contributions of confinement, marginal deformations, and their interplay. Additionally, we provide a detailed analysis of how certain observables are influenced by the dynamics of the Kaluza-Klein (KK) modes arising from the circle compactification. Our results offer an improved understanding of the connections between the type IIB deformed backgrounds and the dual QFTs.

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Cited by 3 Pith papers

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

  1. Krylov Complexity, Confinement and Universality

    hep-th 2026-02 conditional novelty 6.0 of 10

    Holographic calculations show the proper-momentum proxy for Krylov complexity oscillates in every confining geometry with a smooth infrared cap, with frequency set by the confinement scale.

  2. 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.

  3. 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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