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Constructing Non-Relativistic AdS$_5$/CFT$_4$ Holography

2 Pith papers cite this work. Polarity classification is still indexing.

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abstract

We construct a new type of holographic correspondence between non-relativistic string theory in String Newton-Cartan AdS$_5\times$S$^5$ and Galilean Yang-Mills supplemented with 5 adjoint interacting scalar fields living on the 3+1 dimensional Penrose conformal boundary. In our derivation, we start with Maldacena's setting of a stack of $N$ coincident D3-branes and we show that the near-horizon/decoupling limit commutes with the non-relativistic limit, giving a unique answer both from the gravity and gauge theory perspectives. As a first evidence, we systematically compute the Killing vectors on the string theory side, and find that they match the symmetries of the dual gauge theory.

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hep-th 2

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2026 2

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UNVERDICTED 2

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representative citing papers

Non-relativistic limits of $\mathcal N=4$ supersymmetric Yang-Mills theory and S-duality

hep-th · 2026-06-19 · unverdicted · novelty 7.0

Constructs a family of non-relativistic limits of 4d MSYM via brane setups that organize into a 3D moduli space with nontrivial topology where PSL(2,Z) dualities act more complexly than in the relativistic theory, establishing Abelian duality by path integral and supporting non-Abelian case via spec

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Showing 2 of 2 citing papers after filters.

  • Non-relativistic limits of $\mathcal N=4$ supersymmetric Yang-Mills theory and S-duality hep-th · 2026-06-19 · unverdicted · none · ref 18 · internal anchor

    Constructs a family of non-relativistic limits of 4d MSYM via brane setups that organize into a 3D moduli space with nontrivial topology where PSL(2,Z) dualities act more complexly than in the relativistic theory, establishing Abelian duality by path integral and supporting non-Abelian case via spec

  • Phase-Space Contractions of Carrollian Black-Hole Thermodynamics hep-th · 2026-04-30 · unverdicted · none · ref 37 · 3 links · internal anchor

    Double-scaling contractions of extended AdS black-hole thermodynamics produce finite Carrollian phase-space first laws with pressure-volume contributions under the condition α + γ = 1.