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March 19, 2026Journal of High Energy Physics0 citationsOpen Access

Asymptotic higher spin symmetries II: Noether realization in gravity

NCNicolas CrestoLFLaurent Freidel

Key Points

  • The aim is to construct a non-perturbative action of higher spin symmetries on the gravitational phase space.
  • Introduce a symmetry algebroid T to include radiation in an algebraic framework.
  • Define a non-linear realization of the algebroid on the asymptotic phase space.
  • Establish conservation of the Noether charge in the absence of radiation.
  • Restrict the algebroid to the wedge symmetry algebra at non-radiative cuts.
  • The Noether charge is conserved without radiation presence.
  • The symmetry parameters evolve according to equations of motion related to asymptotic Einstein's equations.
  • The underlying symmetry algebra is canonically represented.

Abstract

A bstract In this paper we construct a non-perturbative action of the higher spin symmetry algebra on the gravitational phase space. We introduce a symmetry algebroid T T which allows us to include radiation in an algebraic framework. We show that T T admits a non-linear realization on the asymptotic phase space generated by a Noether charge defined non-perturbatively for all spins. Besides, this Noether charge is conserved in the absence of radiation. Moreover, at non radiative cuts, the algebroid can be restricted to the wedge symmetry algebra studied in 1. The key ingredient for our construction is to consider field and time dependent symmetry parameters constrained to evolve according to equations of motion dual to (a truncation of) the asymptotic Einstein’s equations. This result then guarantees that the underlying symmetry algebra is also represented canonically.

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Cite This Study

Cresto et al. (2026) studied this question.

synapsesocial.com/papers/69bb92be496e729e62980431https://doi.org/10.1007/jhep03(2026)147
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