<p>In this paper, we study gravitational symmetry algebras that live on 2-dimensional cuts <i>S</i> of asymptotic infinity. We define a notion of wedge algebra <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11005_2025_1921_Article_IEq1.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="44" /> </InlineMediaObject> <EquationSource Format="TEX">\(\mathcal {W}(S)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi mathvariant="script">W</mi> <mo stretchy="false">(</mo> <mi>S</mi> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> that depends on the topology of <i>S</i>. For the cylinder <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11005_2025_1921_Article_IEq2.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="53" /> </InlineMediaObject> <EquationSource Format="TEX">\(S={\mathbb {C}}^*\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>S</mi> <mo>=</mo> <msup> <mrow> <mi mathvariant="double-struck">C</mi> </mrow> <mo>∗</mo> </msup> </mrow> </math></EquationSource> </InlineEquation>, we recover the celebrated <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11005_2025_1921_Article_IEq3.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="53" /> </InlineMediaObject> <EquationSource Format="TEX">\(Lw_{1+\infty }\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>L</mi> <msub> <mi>w</mi> <mrow> <mn>1</mn> <mo>+</mo> <mi>∞</mi> </mrow> </msub> </mrow> </math></EquationSource> </InlineEquation> algebra. For the 2-sphere <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11005_2025_1921_Article_IEq4.gif" Format="GIF" Height="16" Rendition="HTML" Resolution="72" Type="Linedraw" Width="19" /> </InlineMediaObject> <EquationSource Format="TEX">\(S^2\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mi>S</mi> <mn>2</mn> </msup> </math></EquationSource> </InlineEquation>, the wedge algebra reduces to a central extension of the anti-self-dual projection of the Poincaré algebra. We then extend <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11005_2025_1921_Article_IEq5.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="44" /> </InlineMediaObject> <EquationSource Format="TEX">\(\mathcal {W}(S)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi mathvariant="script">W</mi> <mo stretchy="false">(</mo> <mi>S</mi> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> outside of the wedge space and build a new Lie algebra <InlineEquation ID="IEq6"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11005_2025_1921_Article_IEq6.gif" Format="GIF" Height="19" Rendition="HTML" Resolution="72" Type="Linedraw" Width="50" /> </InlineMediaObject> <EquationSource Format="TEX">\(\mathcal {W}_\sigma (S)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi mathvariant="script">W</mi> <mi>σ</mi> </msub> <mrow> <mo stretchy="false">(</mo> <mi>S</mi> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation>, which can be viewed as a deformation of the wedge algebra by a spin two field <InlineEquation ID="IEq7"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11005_2025_1921_Article_IEq7.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="TEX">\(\sigma \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>σ</mi> </math></EquationSource> </InlineEquation> playing the role of the shear at a cut of <InlineEquation ID="IEq8"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="MediaObjects/11005_2025_1921_IEq8_HTML.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="120" Type="Linedraw" Width="13" /> </InlineMediaObject> </InlineEquation>. This algebra represents the gravitational symmetry algebra in the presence of a non-trivial shear and is characterized by a covariantized version of the wedge condition. Finally, we construct a dressing map that provides a Lie algebra isomorphism between the covariant and regular wedge algebras.</p>

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Asymptotic higher spin symmetries I: covariant wedge algebra in gravity

  • Nicolas Cresto,
  • Laurent Freidel

摘要

In this paper, we study gravitational symmetry algebras that live on 2-dimensional cuts S of asymptotic infinity. We define a notion of wedge algebra \(\mathcal {W}(S)\) W ( S ) that depends on the topology of S. For the cylinder \(S={\mathbb {C}}^*\) S = C , we recover the celebrated \(Lw_{1+\infty }\) L w 1 + algebra. For the 2-sphere \(S^2\) S 2 , the wedge algebra reduces to a central extension of the anti-self-dual projection of the Poincaré algebra. We then extend \(\mathcal {W}(S)\) W ( S ) outside of the wedge space and build a new Lie algebra \(\mathcal {W}_\sigma (S)\) W σ ( S ) , which can be viewed as a deformation of the wedge algebra by a spin two field \(\sigma \) σ playing the role of the shear at a cut of . This algebra represents the gravitational symmetry algebra in the presence of a non-trivial shear and is characterized by a covariantized version of the wedge condition. Finally, we construct a dressing map that provides a Lie algebra isomorphism between the covariant and regular wedge algebras.