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Mode coupling on a geometrodynamical quantization of an inflationary universe

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TLDR
In this article, a geometrodynamical quantization of an inflationary universe is considered in order to estimate quantum-gravity effects for the primordial perturbations, and the back-reaction produced by all the modes of the system is included in their computations.
Abstract
A geometrodynamical quantization of an inflationary universe is considered in order to estimate quantum-gravity effects for the primordial perturbations. Contrary to previous studies in the literature, the back-reaction produced by all the modes of the system is included in our computations. Even if at a classical level the assumption that every mode evolves independently provides a good estimate for the dynamics, our results explicitly show that this is not the case when considering quantum-gravity effects. More precisely, both the self-interaction, as well as the back-reaction from other modes, provide a correction of the same order of magnitude to the usual power spectrum as computed in the approximation of quantum field theory on classical backgrounds. In particular, these quantum-gravity effects introduce certain characteristic scale-dependence on the expression of the power spectrum.

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References
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Journal ArticleDOI

On the modification of the cosmic microwave background anisotropy spectrum from canonical quantum gravity

TL;DR: In this article, the authors evaluate the modifications to the cosmic microwave background anisotropy spectrum that result from a semiclassical expansion of the Wheeler-DeWitt equation and show that there is an ambiguity in the choice of solution to the equations describing the quantum gravitational effects.
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Non-Gaussianity from excited initial inflationary states

TL;DR: In this article, a model independent way, the authors restrict excited to mean a Bogoliubov transformation of the Bunch Davies state and show that most excited initial inflationary states for single field inflationary models with negligible superhorizon evolution do not produce an observable squeezed limit f ≥ 0.1.
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Quantum-gravitational effects on gauge-invariant scalar and tensor perturbations during inflation: The de Sitter case

TL;DR: In this paper, the power spectra of a de Sitter universe with quantum-gravitational corrections to the power spectrum of scalar and tensor perturbations during inflation was analyzed.
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Inflation and Quantum Gravity in a Born-Oppenheimer Context

TL;DR: In this article, a general equation describing the lowest order corrections coming from quantum gravitational effects to the spectrum of cosmological scalar fluctuations is obtained, explicitly estimated for the case of a de Sitter evolution.
Journal ArticleDOI

Time in quantum cosmology

TL;DR: In this paper, a cosmological model with two global internal times shows that time reparametrization invariance, and therefore covariance, is not guaranteed by deparameterization.
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