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From large to small \( \mathcal{N} \) = (4, 4) superconformal surface defects in holographic 6d SCFTs

  • Pietro Capuozzo,
  • John Estes,
  • Brandon Robinson,
  • Benjamin Suzzoni

摘要

Two-dimensional (2d) N \( \mathcal{N} \) = (4, 4) Lie superalgebras can be either “small” or “large”, meaning their R-symmetry is either so \( \mathfrak{so} \) (4) or so \( \mathfrak{so} \) (4) ⊕ so \( \mathfrak{so} \) (4), respectively. Both cases admit a superconformal extension and fit into the one-parameter family d \( \mathfrak{d} \) (2, 1; γ) ⊕ d \( \mathfrak{d} \) (2, 1; γ), with parameter γ ∈ (−∞, ∞). The large algebra corresponds to generic values of γ, while the small case corresponds to a degeneration limit with γ → −∞. In 11d supergravity, we study known solutions with superisometry algebra d \( \mathfrak{d} \) (2, 1; γ) ⊕ d \( \mathfrak{d} \) (2, 1; γ) that are asymptotically locally AdS7×𝕊4. These solutions are holographically dual to the 6d maximally superconformal field theory with 2d superconformal defects invariant under d \( \mathfrak{d} \) (2, 1; γ) ⊕ d \( \mathfrak{d} \) (2, 1; γ). We show that a limit of these solutions, in which γ → −∞, reproduces another known class of solutions, holographically dual to small N \( \mathcal{N} \) = (4, 4) superconformal defects. We then use this limit to generate new small N \( \mathcal{N} \) = (4, 4) solutions with finite Ricci scalar, in contrast to the known small N \( \mathcal{N} \) = (4, 4) solutions. We then use holography to compute the entanglement entropy of a spherical region centered on these small N \( \mathcal{N} \) = (4, 4) defects, which provides a linear combination of defect Weyl anomaly coefficients that characterizes the number of defect-localized degrees of freedom. We also comment on the generalization of our results to include N \( \mathcal{N} \) = (0, 4) surface defects through orbifolding.