Quantum gravity, space-time structure, and cosmology
Martin Bojowald

TL;DR
This paper discusses how loop quantum gravity modifies our understanding of space-time, suggesting quantum corrections preserve covariance and introduce observable effects, transforming cosmological models and the nature of space-time at Planck densities.
Contribution
It presents a cohesive view of loop quantum gravity's physical implications, emphasizing the interplay of operator calculations and effective theory, and highlights its potential for falsifiable predictions.
Findings
Quantum corrections modify space-time without destroying covariance.
Observable effects in cosmology are more promising than higher-curvature theories.
At Planck densities, space-time ceases to exist, replaced by a 4D space without evolution.
Abstract
A set of diverse but mutually consistent results obtained in different settings has spawned a new view of loop quantum gravity and its physical implications, based on the interplay of operator calculations and effective theory: Quantum corrections modify, but do not destroy, space-time and the notion of covariance. Potentially observable effects much more promising than those of higher-curvature effective actions result; loop quantum gravity has turned into a falsifiable framework, with interesting ingredients for new cosmic world views. At Planckian densities, space-time disappears and is replaced by 4-dimensional space without evolution.
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