The cosmological constant from Planckian fluctuations and the averaging procedure
Stefano Viaggiu

TL;DR
This paper explores a semiclassical approach to the cosmological constant, using averaging of quantum fluctuations at Planckian scales to derive a small, frozen de Sitter universe, linking quantum effects to cosmological observations.
Contribution
It generalizes the Buchert formalism to include quantum fluctuations and proposes a mechanism for the emergence of a small cosmological constant from Planckian averaging.
Findings
A classical de Sitter universe emerges with a small cosmological constant.
Quantum fluctuations at Planckian scales can be averaged to produce effective classical cosmology.
Spatial curvature and backreaction effects are suppressed during evolution.
Abstract
In this paper I continue the investigation in \cite{1,1b} concerning my proposal on the nature of the cosmological constant. In particular, I study both mathematically and physically the quantum Planckian context and I provide, in order to depict quantum fluctuations and in absence of a complete quantum gravity theory, a semiclassical solution where an effective inhomogeneous metric at Planckian scales or above is averaged. In such a framework, a generalization of the well known Buchert formalism \cite{2} is obtained with the foliation in terms of the mean value of the time operator in a maximally localizing state of a quantum spacetime \cite{3,4,5,6} and in a cosmological context \cite{7}. As a result, after introducing a decoherence length scale where quantum fluctuations are averaged on, a classical de Sitter universe emerges with a small…
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