Gravity duals of supersymmetric gauge theories on three-manifolds
Daniel Farquet, Jakob Lorenzen, Dario Martelli, James Sparks
TL;DR
The authors construct a broad class of gravity duals for ${ m N}=2$ gauge theories on curved 3-manifolds by using Euclidean self-dual solutions of four-dimensional minimal gauged supergravity with ball topology, establishing a universal holographic free-energy formula that depends only on the supersymmetric Killing vector data. They show that, for toric self-dual fillings on the four-ball, the renormalized on-shell action matches the large-$N$ localization predictions, providing an exact gauge/gravity check for theories defined on general backgrounds. The approach connects local geometric data (Toda/Kähler structures and Killing spinors) to global holographic quantities, and the paper provides explicit examples (AdS$_4$, Taub-NUT-AdS$_4$, and Plebanski-Demianski) illustrating the general construction, as well as an infinite-parameter extension via $m$-pole toric metrics. The results also relate holographic invariants to boundary conformal data and bulk topological invariants through index theorems, offering a versatile framework for computing holographic observables beyond round-sphere backgrounds. Overall, the work strengthens the gauge/gravity correspondence in curved-background settings and opens directions for extending to broader observables and higher dimensions.
Abstract
We study gravity duals to a broad class of N=2 supersymmetric gauge theories defined on a general class of three-manifold geometries. The gravity backgrounds are based on Euclidean self-dual solutions to four-dimensional gauged supergravity. As well as constructing new examples, we prove in general that for solutions defined on the four-ball the gravitational free energy depends only on the supersymmetric Killing vector, finding a simple closed formula when the solution has U(1) x U(1) symmetry. Our result agrees with the large N limit of the free energy of the dual gauge theory, computed using localization. This constitutes an exact check of the gauge/gravity correspondence for a very broad class of gauge theories with a large N limit, defined on a general class of background three-manifold geometries.
