Journal of High Energy Physics (Aug 2024)

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

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

DOI
https://doi.org/10.1007/JHEP08(2024)094
Journal volume & issue
Vol. 2024, no. 8
pp. 1 – 36

Abstract

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Abstract 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.

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