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All AdS_7 solutions of type II supergravity

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

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abstract

In M-theory, the only AdS_7 supersymmetric solutions are AdS_7 x S^4 and its orbifolds. In this paper, we find and classify new supersymmetric solutions of the type AdS_7 x M_3 in type II supergravity. While in IIB none exist, in IIA with Romans mass (which does not lift to M-theory) there are many new ones. We use a pure spinor approach reminiscent of generalized complex geometry. Without the need for any Ansatz, the system determines uniquely the form of the metric and fluxes, up to solving a system of ODEs. Namely, the metric on M_3 is that of an S^2 fibered over an interval; this is consistent with the Sp(1) R-symmetry of the holographically dual (1,0) theory. By including D8 brane sources, one can numerically obtain regular solutions, where topologically M_3 = S^3.

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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

Sharpened Dynamical Cobordism

hep-th · 2026-05-07 · unverdicted · novelty 7.0

Sharpened Dynamical Cobordism ties the allowed range of critical exponent δ to theory structure ξ, flagging obstructions from non-trivial cobordism charges that require new degrees of freedom.

Complexity and Operator Growth in Holographic 6d SCFTs

hep-th · 2026-03-10 · unverdicted · novelty 6.0

In holographic 6d N=(1,0) SCFTs, generalized proper momentum of infalling particles grows linearly at late times, with early dynamics modified by SU(2)_R charge and quiver spreading.

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Showing 2 of 2 citing papers.

  • Sharpened Dynamical Cobordism hep-th · 2026-05-07 · unverdicted · none · ref 79

    Sharpened Dynamical Cobordism ties the allowed range of critical exponent δ to theory structure ξ, flagging obstructions from non-trivial cobordism charges that require new degrees of freedom.

  • Complexity and Operator Growth in Holographic 6d SCFTs hep-th · 2026-03-10 · unverdicted · none · ref 16 · internal anchor

    In holographic 6d N=(1,0) SCFTs, generalized proper momentum of infalling particles grows linearly at late times, with early dynamics modified by SU(2)_R charge and quiver spreading.