Higher spin Lagrangians from higher derivative diffeomorphisms

Fuente: arXiv
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Autori principali: Barker, Will, Francia, Dario, Marzo, Carlo, Santoni, Alessandro
Natura: Preprint
Pubblicazione: 2025
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author Barker, Will
Francia, Dario
Marzo, Carlo
Santoni, Alessandro
author_facet Barker, Will
Francia, Dario
Marzo, Carlo
Santoni, Alessandro
contents The covariant description of massless particles of arbitrary spin typically employs symmetric tensors of rank $s$ and rests on a local symmetry carried by symmetric tensor parameters of rank $s-1$, suitably generalizing the $U(1)$ transformations of Maxwell's theory and the diffeomorphisms underlying general relativity. Here we show that Fronsdal's action is actually uniquely identified by the weaker requirement of invariance under higher-derivative gauge transformations driven by a vector parameter. This observation may hint to a tighter, if unexpected, connection between higher-spin symmetry and diffeomorphisms.
format Preprint
id arxiv_https___arxiv_org_abs_2510_20895
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Higher spin Lagrangians from higher derivative diffeomorphisms
Barker, Will
Francia, Dario
Marzo, Carlo
Santoni, Alessandro
High Energy Physics - Theory
General Relativity and Quantum Cosmology
The covariant description of massless particles of arbitrary spin typically employs symmetric tensors of rank $s$ and rests on a local symmetry carried by symmetric tensor parameters of rank $s-1$, suitably generalizing the $U(1)$ transformations of Maxwell's theory and the diffeomorphisms underlying general relativity. Here we show that Fronsdal's action is actually uniquely identified by the weaker requirement of invariance under higher-derivative gauge transformations driven by a vector parameter. This observation may hint to a tighter, if unexpected, connection between higher-spin symmetry and diffeomorphisms.
title Higher spin Lagrangians from higher derivative diffeomorphisms
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2510.20895