Holographic Duals of D=3 N=4 Superconformal Field Theories
Benjamin Assel, Costas Bachas, John Estes, Jaume Gomis
TL;DR
The work constructs explicit warpings of Type-IIB supergravity, yielding AdS4×K backgrounds that holographically dualize a large family of 3D ${\mathcal N}=4$ SCFTs labeled by partitions $(\rho,\hat{\rho})$ of $N$, identified as IR fixed points of mirror-symmetric quivers $T^{\rho}_{\hat{\rho}}(SU(N))$ and their S-duals. The authors derive a gravitational version of the field-theory fixed-point constraint, show that the global symmetry $H_{\rho}\times H_{\hat{\rho}}$ is realized by bulk degrees of freedom on five-brane stacks, and map the gravitational data to the quiver data via the brane linking numbers, including a detailed treatment of brane charges, Page charges, and flux quantization. A key feature is the analysis of degeneration limits where AdS5×S^5 regions decouple or warp into wormhole-like connections between multiple AdS4 regions, corresponding to factorization of the quiver into subquivers connected by weak links. The results provide a concrete string-theory realization of a rich class of 3D fixed-point theories, enabling quantitative tests (e.g., partition functions on S^3) and offering insights into brane dynamics, holographic duality, and possible gravity-localization phenomena.
Abstract
We find the warped AdS_4 x K type-IIB supergravity solutions holographically dual to a large family of three dimensional \cN=4 superconformal field theories labeled by a pair (ρ,\hatρ) of partitions of N. These superconformal theories arise as renormalization group fixed points of three dimensional mirror symmetric quiver gauge theories, denoted by T^ρ_{\hat ρ}(SU(N)) and T_ρ^{\hat ρ}(SU(N)) respectively. We give a supergravity derivation of the conjectured field theory constraints that must be satisfied in order for these gauge theories to flow to a non-trivial supersymmetric fixed point in the infrared. The exotic global symmetries of these superconformal field theories are precisely realized in our explicit supergravity description.
