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Updated: Apr 24, 2026

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
No-go theorems for unitary and interacting partially massless spin-two fields.
Euihun Joung1, Wenliang Li1, Massimo Taronna2
1AstroParticule et Cosmologie, Unité Mixte de Recherche 7164 du CNRS, 10 rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France.
A partially massless spin-two field interacting with gravity cannot form a unitary theory. Theories with positive kinetic terms lead to imaginary coupling constants, while negative terms recover conformal gravity.
Area of Science:
- Theoretical Physics
- Quantum Field Theory
Background:
- Investigating theories of partially massless (PM) spin-two fields interacting with gravity is crucial for understanding fundamental forces.
- The behavior of such fields in four-dimensional spacetime requires detailed theoretical analysis.
Purpose of the Study:
- To examine the generic theory of a partially massless spin-two field interacting with gravity.
- To determine the conditions for the existence of a unitary theory and analyze its properties.
Main Methods:
- Analysis of the most general form of the Lagrangian for a PM spin-two field coupled to gravity.
- Investigation of de Sitter backgrounds and their associated global symmetries (so(1,5) or so(2,4)).
- Examination of the PM cubic self-interaction and its coupling constant.
Main Results:
- A de Sitter background requires so(1,5) or so(2,4) symmetry based on the sign of kinetic terms.
- A positive sign necessitates a purely imaginary coupling constant for PM cubic self-interaction.
- A negative sign leads to the recovery of conformal gravity.
Conclusions:
- A unitary theory of a PM spin-two field coupled to Einstein gravity with a perturbatively local Lagrangian cannot exist.
- The PM limit of massive gravity also lacks PM gauge symmetry.
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