<p>We propose an <InlineEquation ID="IEq2"> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 3 nonlinear multiplet coupled to conformal supergravity and use it to formulate the equations of motion for <InlineEquation ID="IEq3"> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 3 Poincaré supergravity. These equations, which are naturally described in a new curved supergeometry with structure group SL(2<i>,</i> ℂ), imply that the <InlineEquation ID="IEq4"> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 3 super-Bach tensor vanishes, and thus every solution of Poincaré supergravity is a solution of conformal supergravity. The aforementioned superspace formulation, which we refer to as <InlineEquation ID="IEq5"> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="script">N</mi> </math></EquationSource> <EquationSource Format="TEX">\( \mathcal{N} \)</EquationSource> </InlineEquation> = 3 Einstein superspace, is described in terms of two dimension-1<i>/</i>2 superfields: (i) the super-Weyl spinor <i>W</i><sub><i>α</i></sub>; and (ii) a spinor isospinor <InlineEquation ID="IEq6"> <EquationSource Format="MATHML"><math display="inline"> <msubsup> <mi>χ</mi> <mi>α</mi> <mi>i</mi> </msubsup> </math></EquationSource> <EquationSource Format="TEX">\( {\chi}_{\alpha}^i \)</EquationSource> </InlineEquation>.</p>

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\( \mathcal{N} \) = 3 nonlinear multiplet and supergravity

  • Sergei M. Kuzenko,
  • Emmanouil S. N. Raptakis

摘要

We propose an N \( \mathcal{N} \) = 3 nonlinear multiplet coupled to conformal supergravity and use it to formulate the equations of motion for N \( \mathcal{N} \) = 3 Poincaré supergravity. These equations, which are naturally described in a new curved supergeometry with structure group SL(2, ℂ), imply that the N \( \mathcal{N} \) = 3 super-Bach tensor vanishes, and thus every solution of Poincaré supergravity is a solution of conformal supergravity. The aforementioned superspace formulation, which we refer to as N \( \mathcal{N} \) = 3 Einstein superspace, is described in terms of two dimension-1/2 superfields: (i) the super-Weyl spinor Wα; and (ii) a spinor isospinor χ α i \( {\chi}_{\alpha}^i \) .