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Asymptotic structure of a massless scalar field and its dual two-form field at spatial infinity

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it
abstract

Relativistic field theories with a power law decay in $r^{-k}$ at spatial infinity generically possess an infinite number of conserved quantities because of Lorentz invariance. Most of these are not related in any obvious way to symmetry transformations of which they would be the Noether charges. We discuss the issue in the case of a massless scalar field. By going to the dual formulation in terms of a $2$-form (as was done recently in a null infinity analysis), we relate some of the scalar charges to symmetry transformations acting on the $2$-form and on surface degrees of freedom that must be added at spatial infinity. These new degrees of freedom are necessary to get a consistent relativistic description in the dual picture, since boosts would otherwise fail to be canonical transformations. We provide explicit boundary conditions on the $2$-form and its conjugate momentum, which involves parity conditions with a twist, as in the case of electromagnetism and gravity. The symmetry group at spatial infinity is composed of `improper gauge transformations'. It is abelian and infinite-dimensional. We also briefly discuss the realization of the asymptotic symmetries, characterized by a non trivial central extension and point out vacuum degeneracy.

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hep-th 2 gr-qc 1

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UNVERDICTED 3

representative citing papers

Revisiting boundary electromagnetic duality and edge modes

hep-th · 2026-05-27 · unverdicted · novelty 6.0

In 4D Maxwell theory, standard Neumann/Dirichlet boundary conditions render large gauge transformations and edge mode shifts as gauge redundancies, while modified conditions make them physical symmetries generated by topological surface operators, with new electromagnetic dual boundary conditions co

Ti and Spi, Carrollian extended boundaries at timelike and spatial infinity

gr-qc · 2024-12-20 · unverdicted · novelty 6.0

Defines Ti and Spi extended boundaries from asymptotic metric data in Ashtekar-Romano asymptotically flat spacetimes, equipping them with Carrollian geometries that canonically match asymptotic symmetries and realize Strominger conditions via discrete symmetry restriction.

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Showing 3 of 3 citing papers.

  • Revisiting boundary electromagnetic duality and edge modes hep-th · 2026-05-27 · unverdicted · none · ref 54 · internal anchor

    In 4D Maxwell theory, standard Neumann/Dirichlet boundary conditions render large gauge transformations and edge mode shifts as gauge redundancies, while modified conditions make them physical symmetries generated by topological surface operators, with new electromagnetic dual boundary conditions co

  • Scalar, vector and tensor fields on $dS_3$ with arbitrary sources: harmonic analysis and antipodal maps hep-th · 2025-12-17 · unverdicted · none · ref 44 · internal anchor

    Scalar, vector, and tensor spherical harmonics on dS3 are constructed with explicit antipodal relationships between past and future asymptotic data, even with sources, plus decomposition theorems for tensors obeying inhomogeneous wave equations.

  • Ti and Spi, Carrollian extended boundaries at timelike and spatial infinity gr-qc · 2024-12-20 · unverdicted · none · ref 18 · internal anchor

    Defines Ti and Spi extended boundaries from asymptotic metric data in Ashtekar-Romano asymptotically flat spacetimes, equipping them with Carrollian geometries that canonically match asymptotic symmetries and realize Strominger conditions via discrete symmetry restriction.