Completeness from Gravitational Scattering

Fuente: arXiv
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Main Authors: Calisto, Francesco, Cheung, Clifford, Remmen, Grant N., Sciotti, Francesco, Tarquini, Michele
Format: Preprint
Published: 2025
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author Calisto, Francesco
Cheung, Clifford
Remmen, Grant N.
Sciotti, Francesco
Tarquini, Michele
author_facet Calisto, Francesco
Cheung, Clifford
Remmen, Grant N.
Sciotti, Francesco
Tarquini, Michele
contents We prove that symmetry in the presence of gravity implies a version of the completeness hypothesis. For a broad class of theories, we demonstrate that the existence of finitely many charged particles logically necessitates the existence of infinitely many charged particles populating the entire charge lattice. Our conclusions follow from the consistency of perturbative gravitational scattering and require the following ingredients: 1) a weakly coupled ultraviolet completion of gravity, 2) a nonabelian symmetry $G$, gauged or global, whose Cartan subgroup generates the abelian charge lattice, and 3) a spectrum containing some finite set of charged representations, in the simplest cases taken to be a single particle in the fundamental. Under these conditions, the abelian charge lattice is completely filled by single-particle states for $G=SO(N)$ with $N\geq 5$ and $G=SU(N)$ with $N\geq 3$, which in turn implies completeness for other symmetry groups such as $Spin(N)$, $Sp(N)$, and $E_8$. Curiously, a corollary of our results is that the $SU(5)$ and $SO(10)$ grand unified theories have precisely the minimal field content needed to derive completeness using our methodology.
format Preprint
id arxiv_https___arxiv_org_abs_2512_11955
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Completeness from Gravitational Scattering
Calisto, Francesco
Cheung, Clifford
Remmen, Grant N.
Sciotti, Francesco
Tarquini, Michele
High Energy Physics - Theory
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
We prove that symmetry in the presence of gravity implies a version of the completeness hypothesis. For a broad class of theories, we demonstrate that the existence of finitely many charged particles logically necessitates the existence of infinitely many charged particles populating the entire charge lattice. Our conclusions follow from the consistency of perturbative gravitational scattering and require the following ingredients: 1) a weakly coupled ultraviolet completion of gravity, 2) a nonabelian symmetry $G$, gauged or global, whose Cartan subgroup generates the abelian charge lattice, and 3) a spectrum containing some finite set of charged representations, in the simplest cases taken to be a single particle in the fundamental. Under these conditions, the abelian charge lattice is completely filled by single-particle states for $G=SO(N)$ with $N\geq 5$ and $G=SU(N)$ with $N\geq 3$, which in turn implies completeness for other symmetry groups such as $Spin(N)$, $Sp(N)$, and $E_8$. Curiously, a corollary of our results is that the $SU(5)$ and $SO(10)$ grand unified theories have precisely the minimal field content needed to derive completeness using our methodology.
title Completeness from Gravitational Scattering
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2512.11955