Quantum Cosmological Backreactions I: Cosmological Space Adiabatic Perturbation Theory
S. Schander, T. Thiemann

TL;DR
This paper introduces a novel application of space adiabatic perturbation theory to quantum cosmology, aiming to improve the understanding of quantum backreactions near the big bang by systematically separating modes.
Contribution
It adapts and extends space adiabatic perturbation theory for quantum cosmology, providing a systematic framework to analyze quantum backreactions between matter and geometry.
Findings
Identifies correction terms in quantum Friedmann equations due to backreactions.
Adapts SAPT to hybrid quantum cosmology models.
Highlights potential quantum effects near the big bang.
Abstract
The search for quantum gravity fingerprints in currently available cosmological data that have their origin from the Planck era is of growing interest due to major recent progress both in the theoretical modelling as well as the observational precision. Unsurprisingly, the theoretical predictions are very sensitive to the quantum effects that occur close to the classical big bang singularity. It is therefore of substantial interest to describe these effects as precisely as possible. This is the first in a series of papers that aim at improving on the treatment of quantum effects that arise due to backreactions between matter and geometry. The technique we employ is space adiabatic perturbation theory (SAPT) in the form developed in seminal papers by Panati, Spohn and Teufel. SAPT is a generalisation of the more familiar Born Oppenheimer Approximation (BOA) that applies well in systems…
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Taxonomy
TopicsCosmology and Gravitation Theories · Complex Systems and Time Series Analysis · Radioactive Decay and Measurement Techniques
