<p>Using the <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq2.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="55" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi>SO</mi> <mfenced close=")" open="("> <mi mathvariant="script">N</mi> </mfenced> </math></EquationSource> <EquationSource Format="TEX">\( \textrm{SO}\left(\mathcal{N}\right) \)</EquationSource> </InlineEquation> superspace formulation for <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation>-extended conformal supergravity in three dimensions, we derive all maximally supersymmetric backgrounds in the <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 4 case. The specific feature of this choice is that the so-called super Cotton tensor <i>X</i><sup><i>IJKL</i></sup> = <i>X</i><sup>[<i>IJKL</i>]</sup>, which exists for <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> ≥ 4, is equivalent to the scalar <i>X</i> defined by <i>X</i><sup><i>IJKL</i></sup> = <i>ε</i><sup><i>IJKL</i></sup><i>X</i>. This scalar may be used as a deformation parameter. In the family of (<i>p</i>, <i>q</i>) anti-de Sitter (AdS) superspaces with <i>p</i> + <i>q</i> = 4, <i>p</i> ≥ <i>q</i>, it is known that <i>X</i> ≠ 0 exists only if <i>p</i> = 4 and <i>q</i> = 0. In general, the (4, 0) AdS superspaces are characterised by the structure group SL(2, <i>ℝ</i>) × SO(4) and their geometry is determined by two constant parameters, <i>S</i> and <i>X</i>, of which the former determines the AdS curvature, while the <i>R</i>-symmetry curvature is determined by the parameters (<i>X</i> + 2<i>S</i>) and (<i>X</i> – 2<i>S</i>) in the left and right sectors of SU(2)<sub>L</sub> × SU(2)<sub>R</sub>, respectively. Setting <i>S</i> = 0 leads to the so-called deformed <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 4 Minkowski superspace <InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq7.gif" Format="GIF" Height="25" Rendition="HTML" Resolution="72" Type="Linedraw" Width="34" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <msubsup> <mi mathvariant="double-struck">M</mi> <mi>X</mi> <mrow> <mfenced close="|"> <mn>3</mn> </mfenced> <mn>8</mn> </mrow> </msubsup> </math></EquationSource> <EquationSource Format="TEX">\( {\mathbbm{M}}_X^{\left.3\right|8} \)</EquationSource> </InlineEquation> introduced thirteen years ago. We use projective-superspace techniques to construct general interacting supersymmetric field theories in <InlineEquation ID="IEq8"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq7.gif" Format="GIF" Height="25" Rendition="HTML" Resolution="72" Type="Linedraw" Width="34" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <msubsup> <mi mathvariant="double-struck">M</mi> <mi>X</mi> <mrow> <mfenced close="|"> <mn>3</mn> </mfenced> <mn>8</mn> </mrow> </msubsup> </math></EquationSource> <EquationSource Format="TEX">\( {\mathbbm{M}}_X^{\left.3\right|8} \)</EquationSource> </InlineEquation> and demonstrate that they originate as massive deformations of the following two families of <InlineEquation ID="IEq9"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 4 theories in standard Minkowski superspace <InlineEquation ID="IEq10"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq10.gif" Format="GIF" Height="18" Rendition="HTML" Resolution="72" Type="Linedraw" Width="34" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <msup> <mi mathvariant="double-struck">M</mi> <mrow> <mfenced close="|"> <mn>3</mn> </mfenced> <mn>8</mn> </mrow> </msup> </math></EquationSource> <EquationSource Format="TEX">\( {\mathbbm{M}}^{\left.3\right|8} \)</EquationSource> </InlineEquation>: (i) <InlineEquation ID="IEq11"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 4 superconformal field theories; and (ii) <InlineEquation ID="IEq12"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 4 supersymmetric gauge theories in <InlineEquation ID="IEq13"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq10.gif" Format="GIF" Height="18" Rendition="HTML" Resolution="72" Type="Linedraw" Width="34" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <msup> <mi mathvariant="double-struck">M</mi> <mrow> <mfenced close="|"> <mn>3</mn> </mfenced> <mn>8</mn> </mrow> </msup> </math></EquationSource> <EquationSource Format="TEX">\( {\mathbbm{M}}^{\left.3\right|8} \)</EquationSource> </InlineEquation> which are not superconformal but possess the <i>R</i>-symmetry group SU(2)<sub>L</sub> × SU(2)<sub>R</sub>. Extensions of the theories in (ii) to <InlineEquation ID="IEq14"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq7.gif" Format="GIF" Height="25" Rendition="HTML" Resolution="72" Type="Linedraw" Width="34" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <msubsup> <mi mathvariant="double-struck">M</mi> <mi>X</mi> <mrow> <mfenced close="|"> <mn>3</mn> </mfenced> <mn>8</mn> </mrow> </msubsup> </math></EquationSource> <EquationSource Format="TEX">\( {\mathbbm{M}}_X^{\left.3\right|8} \)</EquationSource> </InlineEquation> necessarily contain Chern-Simons terms at the component level. We also demonstrate the generation of topologically massive <InlineEquation ID="IEq15"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_27467_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 4 supersymmetric gauge theories from radiative corrections in the hypermultiplet sector.</p>

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On three-dimensional \( \mathcal{N} \) = 4 supersymmetry: maximally supersymmetric backgrounds and massive deformations

  • Sergei M. Kuzenko,
  • Emmanouil S. N. Raptakis,
  • Igor B. Samsonov,
  • Gabriele Tartaglino-Mazzucchelli

摘要

Using the SO N \( \textrm{SO}\left(\mathcal{N}\right) \) superspace formulation for N \( \mathcal{N} \) -extended conformal supergravity in three dimensions, we derive all maximally supersymmetric backgrounds in the N \( \mathcal{N} \) = 4 case. The specific feature of this choice is that the so-called super Cotton tensor XIJKL = X[IJKL], which exists for N \( \mathcal{N} \) ≥ 4, is equivalent to the scalar X defined by XIJKL = εIJKLX. This scalar may be used as a deformation parameter. In the family of (p, q) anti-de Sitter (AdS) superspaces with p + q = 4, pq, 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, ) × 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 \( \mathcal{N} \) = 4 Minkowski superspace M X 3 8 \( {\mathbbm{M}}_X^{\left.3\right|8} \) introduced thirteen years ago. We use projective-superspace techniques to construct general interacting supersymmetric field theories in M X 3 8 \( {\mathbbm{M}}_X^{\left.3\right|8} \) and demonstrate that they originate as massive deformations of the following two families of N \( \mathcal{N} \) = 4 theories in standard Minkowski superspace M 3 8 \( {\mathbbm{M}}^{\left.3\right|8} \) : (i) N \( \mathcal{N} \) = 4 superconformal field theories; and (ii) N \( \mathcal{N} \) = 4 supersymmetric gauge theories in M 3 8 \( {\mathbbm{M}}^{\left.3\right|8} \) which are not superconformal but possess the R-symmetry group SU(2)L × SU(2)R. Extensions of the theories in (ii) to M X 3 8 \( {\mathbbm{M}}_X^{\left.3\right|8} \) necessarily contain Chern-Simons terms at the component level. We also demonstrate the generation of topologically massive N \( \mathcal{N} \) = 4 supersymmetric gauge theories from radiative corrections in the hypermultiplet sector.