<p>We clarify and extend our earlier work [<CitationRef CitationID="CR1">1</CitationRef>, <CitationRef CitationID="CR2">2</CitationRef>] where it was shown how to amend a scheme originally proposed by M. Gell-Mann to identify the three families of quarks and leptons of the Standard Model with the 48 spin-<InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_26913_Article_IEq1.gif" Format="GIF" Height="22" Rendition="HTML" Resolution="72" Type="Linedraw" Width="8" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mfrac> <mn>1</mn> <mn>2</mn> </mfrac> </math></EquationSource> <EquationSource Format="TEX">\( \frac{1}{2} \)</EquationSource> </InlineEquation> fermions of <i>N</i> = 8 supergravity that remain after absorption of eight Goldstinos, a scheme that in its original form is dynamically realized at the SU(3) × U(1) stationary point of gauged <i>N</i> = 8 supergravity. We explain how to deform and enlarge this symmetry at the kinematical level to the full Standard Model symmetry group SU(3)<sub><i>c</i></sub><i>×</i>SU(2)<sub><i>w</i></sub><i>×</i>U(1)<sub><i>Y</i></sub>, with the correct charge and chiral assignments for all fermions. The framework also leaves room for an extra U(1)<sub><i>B−L</i></sub> symmetry. This symmetry enhancement is achieved by embedding the Standard Model symmetries into (a quotient group of) K(E<sub>10</sub>), the ‘maximal compact subgroup’ of the maximal rank hyperbolic Kac-Moody symmetry E<sub>10</sub>, and an infinite prolongation of the SU(8) <i>R</i>-symmetry of <i>N</i> = 8 supergravity. This scheme, which is also supposed to encompass quantum gravity, cannot be realized within the framework of space-time based (quantum) field theory, but requires space-time and related geometrical concepts to be ‘emergent’. We critically review the main hypotheses underlying this construction.</p>

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Standard model symmetries and K(E10)

  • Krzysztof A. Meissner,
  • Hermann Nicolai

摘要

We clarify and extend our earlier work [1, 2] where it was shown how to amend a scheme originally proposed by M. Gell-Mann to identify the three families of quarks and leptons of the Standard Model with the 48 spin- 1 2 \( \frac{1}{2} \) fermions of N = 8 supergravity that remain after absorption of eight Goldstinos, a scheme that in its original form is dynamically realized at the SU(3) × U(1) stationary point of gauged N = 8 supergravity. We explain how to deform and enlarge this symmetry at the kinematical level to the full Standard Model symmetry group SU(3)c×SU(2)w×U(1)Y, with the correct charge and chiral assignments for all fermions. The framework also leaves room for an extra U(1)B−L symmetry. This symmetry enhancement is achieved by embedding the Standard Model symmetries into (a quotient group of) K(E10), the ‘maximal compact subgroup’ of the maximal rank hyperbolic Kac-Moody symmetry E10, and an infinite prolongation of the SU(8) R-symmetry of N = 8 supergravity. This scheme, which is also supposed to encompass quantum gravity, cannot be realized within the framework of space-time based (quantum) field theory, but requires space-time and related geometrical concepts to be ‘emergent’. We critically review the main hypotheses underlying this construction.