Inflation and CMB Anisotropy from Quantum Metric Fluctuations
Leonid Marochnik, Daniel Usikov

TL;DR
This paper presents a quantum gravity-based model explaining the origin of inflation and dark energy through graviton fluctuations, naturally leading to accelerated expansion and observable CMB anisotropies without scalar fields.
Contribution
It introduces a model where quantum metric fluctuations cause inflation and dark energy, eliminating the need for scalar fields or cosmological constants.
Findings
De Sitter expansion arises naturally from quantum gravity equations.
Graviton fluctuations account for CMB anisotropy and polarization.
The model predicts opposite signs of 1+w during inflation and dark energy epochs.
Abstract
We propose a model of cosmological evolution of the early and late Universe which is consistent with observational data and naturally explains the origin of inflation and dark energy. We show that the de Sitter accelerated expansion of the FLRW space with no matter fields (hereinafter, empty space) is its natural state, and the model does not require either a scalar field or cosmological constant or any other hypotheses. This is due to the fact that the de Sitter state is an exact solution of the rigorous mathematically consistent equations of one-loop quantum gravity for the empty FLRW space that are finite off the mass shell. Space without matter fields is not empty, as it always has the natural quantum fluctuations of the metric, i.e. gravitons. Therefore, the empty (in this sense) space is filled with gravitons, which have the backreaction effect on its evolution over time forming a…
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