Superconformal indices and black hole saddles

Abstract

The AdS/CFT correspondence implies that the superconformal index $\mathcal{I}$ in $\mathcal{N}=4$ SU(N) supersymmetric Yang-Mills theory can be computed using the dual bulk theory. In particular, in the limit of large $N$, the index should be given by a sum over appropriate saddles. However, $\mathcal{I}$ depends on potentials $\sigma ,\tau ,\vec{\Delta }$ and, at large $\mathrm{Im}\tau =\mathrm{Im}\sigma$, the CFT index $\mathcal{I}$ rapidly approaches $1$ at all values of $N$. As a result, black hole saddles associated with exponentially large contributions in $N$ cannot contribute in this limit. This in particular excludes saddles that were previously suggested to be relevant in such regimes. We thus consider an approach to the bulk path integral motivated by taking it to be defined as an integral over real Lorentz-signature spacetimes with codimension-2 singularities. This approach leads only to saddles that satisfy the above bound, and to the enforcement of this bound via Stokes phenomena. We also find similar results for bulk AdS${}_4$ calculations of the ABJM superconformal index.

arXiv comment65 pages, 16 figures