On three-dimensional N=4 supersymmetry: maximally supersymmetric backgrounds and massive deformations

Abstract

Using the SO ( N) superspace formulation for N-extended conformal supergravity in three dimensions, we derive all maximally supersymmetric backgrounds in the N =4 case. The specific feature of this choice is that the so-called super Cotton tensor XIJKL = X[IJKL], which exists for N ≥ 4, is equivalent to the scalar X defined by XIJKL = IJKL X. This scalar may be used as a deformation parameter. In the family of (p,q) anti-de Sitter (AdS) superspaces with p+q=4, it is known that X≠ 0 exists only if p=4 and q=0. In general, the (4,0) AdS superspaces are characterised by the structure group SL(2, R) × SO (4) and their geometry is determined by two constant parameters, S and X, of which the former determines the AdS curvature, while the R-symmetry curvature is determined by the parameters (X+2S) and (X-2S) in the left and right sectors of SU(2) L × SU(2) R, respectively. Setting S=0 leads to the so-called deformed N=4 Minkowski superspace M3|8X introduced thirteen years ago. We construct general interacting supersymmetric field theories in M3|8X and demonstrate that they originate as massive deformations of the following two families of N =4 theories in standard Minkowski superspace M3|8: (i) N=4 superconformal field theories; and (ii) N=4 supersymmetric gauge theories in M3|8 which are not superconformal but possess the R-symmetry group SU(2) L × SU(2) R. Extensions of the theories in (ii) to M3|8X necessarily contain Chern-Simons terms at the component level. We also demonstrate the generation of topologically massive N=4 supersymmetric gauge theories from radiative corrections in the hypermultiplet sector.

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