An analogue of the Coleman-Mandula theorem for quantum field theory in curved spacetimes
Christopher J. Fewster

TL;DR
This paper proves an analogue of the Coleman-Mandula theorem for quantum field theories in curved spacetimes, showing that extended symmetries are trivial under certain conditions, thus constraining possible symmetry structures.
Contribution
It extends the Coleman-Mandula theorem to curved spacetimes, establishing conditions under which symmetries must be a direct product, applicable to both free and interacting theories.
Findings
Extended symmetry groups are trivial and decompose into gauge and Lorentz parts.
Fields form multiplets of the Lorentz group with no mixing between different spins.
Noninteger spin occurrences are governed by the gauge group's center.
Abstract
The Coleman-Mandula (CM) theorem states that the Poincar\'e and internal symmetries of a Minkowski spacetime quantum field theory cannot combine nontrivially in an extended symmetry group. We establish an analogous result for quantum field theory in curved spacetimes, assuming local covariance, the timeslice property, a local dynamical form of Lorentz invariance, and additivity. Unlike the CM theorem, our result is valid in dimensions and for free or interacting theories. It is formulated for theories defined on a category of all globally hyperbolic spacetimes equipped with a global coframe, on which the restricted Lorentz group acts, and makes use of a general analysis of symmetries induced by the action of a group on the category of spacetimes. Such symmetries are shown to be canonically associated with a cohomology class in the second degree nonabelian cohomology of …
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