QFT in curved spacetime from quantum gravity: Proper WKB decomposition of the gravitational component
Feb 21, 2023
8 pages
Published in:
- Phys.Rev.D 107 (2023) 6, L061901
- Published: Mar 13, 2023
e-Print:
- 2302.10832 [gr-qc]
DOI:
- 10.1103/PhysRevD.107.L061901 (publication)
View in:
Citations per year
Abstract: (APS)
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.Note:
- 8 pages. Title updated and discussion expanded; matches published version
- energy: low
- background: classical
- field theory: scalar
- quantum gravity: effect
- gravitation
- graviton
- space-time
- Bianchi: Type I
- curvature
- WKB approximation
References(60)
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