Asymptotic O $$ \mathcal{O} $$ (r) gauge symmetries and gauge-invariant Poincaré generators in higher spacetime dimensions

Abstract The asymptotic symmetries of electromagnetism in all higher spacetime dimensions d > 4 are extended, by incorporating consistently angle-dependent u(1) gauge transformations with a linear growth in the radial coordinate at spatial infinity. Finiteness of the symplectic structure and pres...

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Main Author: Oscar Fuentealba
Format: Article
Language:English
Published: SpringerOpen 2023-04-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP04(2023)047
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author Oscar Fuentealba
author_facet Oscar Fuentealba
author_sort Oscar Fuentealba
collection DOAJ
description Abstract The asymptotic symmetries of electromagnetism in all higher spacetime dimensions d > 4 are extended, by incorporating consistently angle-dependent u(1) gauge transformations with a linear growth in the radial coordinate at spatial infinity. Finiteness of the symplectic structure and preservation of the asymptotic conditions require to impose a set of strict parity conditions, under the antipodal map of the (d − 2)-sphere, on the leading order fields at infinity. Canonical generators of the asymptotic symmetries are obtained through standard Hamiltonian methods. Remarkably, the theory endowed with this set of asymptotic conditions turns out to be invariant under a six-fold set of angle-dependent u(1) transformations, whose generators form a centrally extended abelian algebra. The new charges generated by the O $$ \mathcal{O} $$ (r) gauge parameter are found to be conjugate to those associated to the now improper subleading O(r −d+3) transformations, while the standard O $$ \mathcal{O} $$ (1) gauge transformations are canonically conjugate to the subleading O $$ \mathcal{O} $$ (r −d+4) transformations. This algebraic structure, characterized by the presence of central charges, allows us to perform a nonlinear redefinition of the Poincaré generators, that results in the decoupling of all of the u(1) charges from the Poincaré algebra. Thus, the mechanism previously used in d = 4 to find gauge-invariant Poincaré generators is shown to be a robust property of electromagnetism in all spacetime dimensions d ≥ 4.
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spelling doaj.art-595e6968562e4048a96efe900043c12b2023-07-30T11:04:43ZengSpringerOpenJournal of High Energy Physics1029-84792023-04-012023412510.1007/JHEP04(2023)047Asymptotic O $$ \mathcal{O} $$ (r) gauge symmetries and gauge-invariant Poincaré generators in higher spacetime dimensionsOscar Fuentealba0Université Libre de Bruxelles and International Solvay InstitutesAbstract The asymptotic symmetries of electromagnetism in all higher spacetime dimensions d > 4 are extended, by incorporating consistently angle-dependent u(1) gauge transformations with a linear growth in the radial coordinate at spatial infinity. Finiteness of the symplectic structure and preservation of the asymptotic conditions require to impose a set of strict parity conditions, under the antipodal map of the (d − 2)-sphere, on the leading order fields at infinity. Canonical generators of the asymptotic symmetries are obtained through standard Hamiltonian methods. Remarkably, the theory endowed with this set of asymptotic conditions turns out to be invariant under a six-fold set of angle-dependent u(1) transformations, whose generators form a centrally extended abelian algebra. The new charges generated by the O $$ \mathcal{O} $$ (r) gauge parameter are found to be conjugate to those associated to the now improper subleading O(r −d+3) transformations, while the standard O $$ \mathcal{O} $$ (1) gauge transformations are canonically conjugate to the subleading O $$ \mathcal{O} $$ (r −d+4) transformations. This algebraic structure, characterized by the presence of central charges, allows us to perform a nonlinear redefinition of the Poincaré generators, that results in the decoupling of all of the u(1) charges from the Poincaré algebra. Thus, the mechanism previously used in d = 4 to find gauge-invariant Poincaré generators is shown to be a robust property of electromagnetism in all spacetime dimensions d ≥ 4.https://doi.org/10.1007/JHEP04(2023)047Gauge SymmetryGlobal SymmetriesSpace-Time Symmetries
spellingShingle Oscar Fuentealba
Asymptotic O $$ \mathcal{O} $$ (r) gauge symmetries and gauge-invariant Poincaré generators in higher spacetime dimensions
Journal of High Energy Physics
Gauge Symmetry
Global Symmetries
Space-Time Symmetries
title Asymptotic O $$ \mathcal{O} $$ (r) gauge symmetries and gauge-invariant Poincaré generators in higher spacetime dimensions
title_full Asymptotic O $$ \mathcal{O} $$ (r) gauge symmetries and gauge-invariant Poincaré generators in higher spacetime dimensions
title_fullStr Asymptotic O $$ \mathcal{O} $$ (r) gauge symmetries and gauge-invariant Poincaré generators in higher spacetime dimensions
title_full_unstemmed Asymptotic O $$ \mathcal{O} $$ (r) gauge symmetries and gauge-invariant Poincaré generators in higher spacetime dimensions
title_short Asymptotic O $$ \mathcal{O} $$ (r) gauge symmetries and gauge-invariant Poincaré generators in higher spacetime dimensions
title_sort asymptotic o mathcal o r gauge symmetries and gauge invariant poincare generators in higher spacetime dimensions
topic Gauge Symmetry
Global Symmetries
Space-Time Symmetries
url https://doi.org/10.1007/JHEP04(2023)047
work_keys_str_mv AT oscarfuentealba asymptoticomathcalorgaugesymmetriesandgaugeinvariantpoincaregeneratorsinhigherspacetimedimensions