Uniqueness of the Fock quantization of scalar fields in spatially flat cosmological spacetimes
Laura Castell\'o Gomar, Jer\'onimo Cortez, Daniel Mart\'in-de Blas,, Guillermo A. Mena Marug\'an, Jos\'e M. Velhinho

TL;DR
This paper demonstrates that in flat cosmological spacetimes, the Fock quantization of scalar fields is unique when requiring vacuum invariance under symmetries and unitary dynamics, ensuring robust quantum predictions.
Contribution
It proves the uniqueness of Fock quantization for scalar fields in flat cosmological backgrounds under symmetry and unitarity conditions.
Findings
Uniqueness of Fock quantization established.
Ambiguities in vacuum choice and field variables are resolved.
Results support consistent quantum cosmological predictions.
Abstract
We study the Fock quantization of scalar fields in (generically) time dependent scenarios, focusing on the case in which the field propagation occurs in --either a background or effective-- spacetime with spatial sections of flat compact topology. The discussion finds important applications in cosmology, like e.g. in the description of test Klein-Gordon fields and scalar perturbations in Friedmann-Robertson-Walker spacetime in the observationally favored flat case. Two types of ambiguities in the quantization are analyzed. First, the infinite ambiguity existing in the choice of a Fock representation for the canonical commutation relations, understandable as the freedom in the choice of inequivalent vacua for a given field. Besides, in cosmological situations, it is customary to scale the fields by time dependent functions, which absorb part of the evolution arising from the spacetime,…
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