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Unitarity of interacting fields in curved spacetime

Journal Article · · Physical Review, D (Particles Fields); (United States)
; ;  [1]
  1. Department of Physics, University of Wisconsin, Milwaukee, Wisconsin 53201 (United States)
On globally hyperbolic spacetimes, each foliation by spacelike hypersurfaces corresponds to a Hamiltonian description of field theory, and unitarity follows formally from the Hermiticity of the Hamiltonian. For a renormalizable theory, unitarity at each order in perturbation theory follows from the corresponding Hermiticity of each term in the time-ordered product of interaction Hamiltonians. For more general spacetimes, one can still use the path integral to obtain a generalized Lehmann-Symanzik-Zimmermann reduction formula for {ital S}-matrix elements and the corresponding perturbative expansion. Unitarity imposes an infinite set of identities on the scattering amplitudes, which are the generalizations of the flat-spacetime Cutkosky rules. We find these explicitly to {ital O}({lambda}{sup 3}) in a {lambda}{ital cphi}{sup 4} theory, and show how to find the relations to any order. For globally hyperbolic spacetimes the unitarity identities are satisfied (at least to {ital O}({lambda}{sup 3})) because of a single property of the configuration-space propagator that reflects the causal structure of the spacetime.
OSTI ID:
7030691
Journal Information:
Physical Review, D (Particles Fields); (United States), Journal Name: Physical Review, D (Particles Fields); (United States) Vol. 46:10; ISSN PRVDA; ISSN 0556-2821
Country of Publication:
United States
Language:
English

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