Holographic RG flows in N=4 SCFTs from half-maximal gauged supergravity

TL;DR

This paper explores the landscape of N=4 supersymmetric conformal field theories in three dimensions via holographic RG flows derived from four-dimensional N=4 gauged supergravity with various gauge groups, revealing multiple fixed points and their interconnections.

Contribution

It provides explicit constructions of holographic RG flows between multiple N=4 SCFT fixed points with different symmetries using supergravity models.

Findings

Identified four N=4 AdS4 vacua with distinct symmetry groups.

Computed full scalar mass spectra at all vacua.

Constructed holographic RG flows connecting these fixed points.

Abstract

We study four-dimensional $N=4$ gauged supergravity coupled to six vector multiplets with semisimple gauge groups $SO(4)\times SO(4)$, $SO(3,1)\times SO(3,1)$ and $SO(4)\times SO(3,1)$. All of these gauge groups are dyonically embedded in the global symmetry group $SO(6,6)$ via its maximal subgroup $SO(3,3)\times SO(3,3)$. For $SO(4)\times SO(4)$ gauge group, there are four $N=4$ supersymmetric $AdS_4$ vacua with $SO(4)\times SO(4)$, $SO(4)\times SO(3)$, $SO(3)\times SO(4)$ and $SO(3)\times SO(3)$ symmetries, respectively. These $AdS_4$ vacua correspond to $N=4$ SCFTs in three dimensions with $SO(4)$ R-symmetry and different flavor symmetries. We explicitly compute the full scalar mass spectra at all these vacua. Holographic RG flows interpolating between these conformal fixed points are also given. The solutions describe supersymmetric deformations of $N=4$ SCFTs by relevant operators of dimensions $\Delta=1,2$. A number of these solutions can be found analytically although some of them can only be obtained numerically. These results provide a rich and novel class of $N=4$ fixed points in three-dimensional Chern-Simons-Matter theories and possible RG flows between them in the framework of $N=4$ gauged supergravity in four dimensions. Similar studies are carried out for non-compact gauge groups, but the $SO(4)\times SO(4)$ gauge group exhibits a much richer structure.