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Inconsistency of interacting, multi-graviton theories

Nicolas Boulanger, Thibault Damour, Leonardo Gualtieri, Marc Henneaux

TL;DR

The work addresses whether multiple massless spin-2 fields can be consistently coupled in a ghost-free, local theory with at most two derivatives. Using BRST deformation theory and characteristic cohomology, the authors show that any consistent deformation must yield a direct sum of diffeomorphism algebras and, at two derivatives, a sum of independent Einstein–Hilbert actions; cross-interactions between different gravitons are therefore forbidden. Matter couplings do not remedy this prohibition, and even in the infinite-field limit the result generalizes to a parallel-set of graviton sectors. Only in cases with a non-positive internal metric or higher-derivative terms could cross-interactions appear, but these typically introduce ghosts or pathological features. The findings reinforce the special status of the Einstein theory as the unique ghost-free, multi-graviton structure under the stated assumptions, and illuminate the precise cohomological obstructions to more elaborate couplings.

Abstract

We investigate, in any spacetime dimension >=3, the problem of consistent couplings for a finite collection of massless, spin-2 fields described, in the free limit, by a sum of Pauli-Fierz actions. We show that there is no consistent (ghost-free) coupling, with at most two derivatives of the fields, that can mix the various "gravitons". In other words, there are no Yang-Mills-like spin-2 theories. The only possible deformations are given by a sum of individual Einstein-Hilbert actions. The impossibility of cross-couplings subsists in the presence of scalar matter. Our approach is based on the BRST-based deformation point of view and uses results on the so-called "characteristic cohomology" for massless spin-2 fields which are explained in detail.

Inconsistency of interacting, multi-graviton theories

TL;DR

The work addresses whether multiple massless spin-2 fields can be consistently coupled in a ghost-free, local theory with at most two derivatives. Using BRST deformation theory and characteristic cohomology, the authors show that any consistent deformation must yield a direct sum of diffeomorphism algebras and, at two derivatives, a sum of independent Einstein–Hilbert actions; cross-interactions between different gravitons are therefore forbidden. Matter couplings do not remedy this prohibition, and even in the infinite-field limit the result generalizes to a parallel-set of graviton sectors. Only in cases with a non-positive internal metric or higher-derivative terms could cross-interactions appear, but these typically introduce ghosts or pathological features. The findings reinforce the special status of the Einstein theory as the unique ghost-free, multi-graviton structure under the stated assumptions, and illuminate the precise cohomological obstructions to more elaborate couplings.

Abstract

We investigate, in any spacetime dimension >=3, the problem of consistent couplings for a finite collection of massless, spin-2 fields described, in the free limit, by a sum of Pauli-Fierz actions. We show that there is no consistent (ghost-free) coupling, with at most two derivatives of the fields, that can mix the various "gravitons". In other words, there are no Yang-Mills-like spin-2 theories. The only possible deformations are given by a sum of individual Einstein-Hilbert actions. The impossibility of cross-couplings subsists in the presence of scalar matter. Our approach is based on the BRST-based deformation point of view and uses results on the so-called "characteristic cohomology" for massless spin-2 fields which are explained in detail.

Paper Structure

This paper contains 30 sections, 9 theorems, 175 equations.

Key Result

Theorem 1.1

Under the assumptions of: locality, Poincaré invariance, Eq.(startingpoint) as free field limit and at most two derivatives in the Lagrangian, the only consistent deformation of Eq.(startingpoint) involving a collection of spin-2 fields is (modulo field redefinitions) a sum of independent Einstein-H where $R^a$ is the scalar curvature of $g^a_{\mu \nu}$, $g^a$ its determinant, $\kappa^a \geq 0$ a

Theorems & Definitions (9)

  • Theorem 1.1
  • Theorem 1.2
  • Theorem 3.1
  • Theorem 4.1
  • Theorem 4.2
  • Theorem 4.1
  • Theorem A.1
  • Lemma A.1
  • Lemma A.2