Superfluid black branes in AdS_4\times S^7
Aristomenis Donos, Jerome P. Gauntlett
TL;DR
This work studies finite-temperature phases of the $d=3$ $N=8$ SCFT holographically via $AdS_4\times S^7$, constructing back-react black branes in $D=11$ supergravity that capture the highest-temperature superfluid instability for a diagonal $U(1)_R$. It demonstrates that the existence and thermodynamic relevance of these holographic superconductors depend crucially on which $SO(8)$ truncation is used, revealing a spectrum of back-reacted solutions including Gubser–Mitra branches and domain-wall flows to IR $AdS_4$ vacua in an alternative quantisation. In particular, the $SU(3)\times U(1)$ infrared fixed point can be reached by zero-temperature domain walls, yielding an emergent superconformal symmetry in the IR and providing top-down realizations of holographic superconductivity with nontrivial zero-temperature ground states. The results underscore the need to consider full or broader truncations (and possibly full $SO(8)$ or $D=11$ embeddings) to map the complete phase diagram and ground states of the dual CFT.
Abstract
We consider the d=3 N=8 SCFT dual to AdS_4\times S^7 when held at finite temperature and chemical potential with respect to a diagonal U(1)_R\subset SO(8) global symmetry and construct black brane solutions of D=11 supergravity that are associated with the superfluid instability with the highest known critical temperature. We construct a rich array of solutions using different sub-truncations of SO(8) gauged supergravity finding results that strongly depend on the truncation used. Our constructions include black brane solutions associated with the Gubser-Mitra instability which preserve the U(1)_R symmetry, and these, in turn, can have further superfluid instabilities. In addition, we also construct superfluid black branes that at zero temperature are domain walls that interpolate between the SO(8) AdS_4 vacuum in the UV, in an alternative quantisation, and the supersymmetric SU(3)\times U(1) AdS_4 vacuum in the IR.
