Analyzing quantum gravity spillover in the semiclassical regime
Harkirat Singh Sahota, Kinjalk Lochan

TL;DR
This paper investigates the effectiveness of using quantum-corrected effective geometries in semiclassical quantum gravity models for dust and dark energy dominated universes, analyzing expectation values of geometric observables.
Contribution
It provides a detailed analysis of the validity of the effective geometry approach in semiclassical quantum gravity for different cosmological models.
Findings
Expectation value of Hubble parameter matches semiclassical expression in dust universe.
Relative difference in Ricci scalar expectation value is maximum at singularity and decreases over time.
Quantum effects persist at late times in dark energy dominated universe.
Abstract
One of the standard approaches of incorporating the quantum gravity (QG) effects into the semiclassical analysis is to adopt the notion of a quantum-corrected spacetime arising from the QG model. This procedure assumes that the expectation value of the metric variable effectively captures the relevant QG subtleties in the semiclassical regime. We investigate the viability of this effective geometry approach for the case of dust dominated and a dark energy dominated universe. We write the phase space expressions for the geometric observables and construct corresponding Hermitian operators. A general class of operator ordering of these observables is considered, and their expectation values are calculated for a unitarily evolving wave packet. In the case of dust dominated universe, the expectation value of the Hubble parameter matches the "semiclassical" expression, the expression…
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Taxonomy
TopicsCosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics
