General covariant transition amplitudes in quantum cosmology
Francesca Vidotto

TL;DR
This paper develops a fully covariant path integral framework for quantum cosmology by integrating recent Loop Quantum Gravity results, enabling non-perturbative quantum transition amplitudes that connect canonical and covariant approaches.
Contribution
It introduces two strategies to define a covariant path integral in quantum cosmology directly from Loop Quantum Gravity, avoiding symmetry reduction prior to quantization.
Findings
Constructed a covariant path integral from full Spinfoam theory.
Connected canonical Loop Quantum Cosmology with covariant formulations.
Includes quantum fluctuations beyond standard perturbation theory.
Abstract
The path-integral approach to cosmology consists in the computation of transition amplitudes between states of the quantum geometry of the universe. In the past, the concrete computation of these transitions amplitudes has been performed in a perturbative regime, breaking the full general covariance of the theory. Here I present how it is possible to define a general covariant path integral in quantum cosmology, by relying on the most recent results of the canonical and covariant formulations of Loop Quantum Gravity. I present two strategies that have been implemented. The first starts from the full Spinfoam theory, i.e. the path-integral framework for Loop Quantum Gravity, and defines a cosmological system. This is not obtained from symmetry reduced variables that are successively quantized, but directly considering the approximations that are characteristic of the full theory. The…
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
