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QFT in curved spacetime from quantum gravity: Proper WKB decomposition of the gravitational component

Giulia Maniccia1,2,*, Giovanni Montani3,1,†, and Stefano Antonini4,‡

  • 1Physics Department, “La Sapienza” University of Rome, P.le A. Moro 5, 00185 Roma, Italy
  • 2INFN Section of Rome, “La Sapienza” University of Rome, P.le A. Moro 5, 00185 Roma, Italy
  • 3ENEA, FNS Department, C.R. Frascati, Via E. Fermi 45, 00044 Frascati (Roma), Italy
  • 4Maryland Center for Fundamental Physics, University of Maryland, College Park, Maryland 20742, USA

  • *giulia.maniccia@uniroma1.it
  • †giovanni.montani@enea.it
  • ‡santonin@umd.edu

Phys. Rev. D 107, L061901 – Published 13 March, 2023

DOI: https://doi.org/10.1103/PhysRevD.107.L061901

Abstract

Starting from a reanalysis of previous work, we construct the proper low-energy quantum field theory (QFT) limit of a full quantum gravity theory in the Born-Oppenheimer approach. We separate the gravitational sector into a classical background, given by a vacuum diagonal Bianchi I cosmology, and its quantum perturbations represented by the two graviton degrees of freedom; we further include quantum matter in the form of a test scalar field. We then implement a Born-Oppenheimer separation, where the gravitons and matter play the roles of “slow” and “fast” quantum components, respectively, and perform a WKB expansion in a Planckian parameter. The functional Schrödinger evolution for matter is recovered after averaging over quantum-gravitational effects, provided that a condition is imposed on the gravitons’ wave functional. Such a condition fixes the graviton dynamics and is equivalent to the purely gravitational Wheeler-DeWitt constraint imposed in previous approaches. The main accomplishment of the present work is to clarify that QFT in curved spacetime can be recovered in the low-energy limit of quantum gravity only after averaging over the graviton degrees of freedom, in the spirit of effective field theory. Furthermore, it justifies a posteriori the implementation of the gravitational Wheeler-DeWitt equation on the “slow” gravitons’ wave functional rather than assuming its validity a priori.

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