A new perspective on cosmology in Loop Quantum Gravity
Emanuele Alesci, Francesco Cianfrani

TL;DR
This paper introduces a novel cosmological model derived from Loop Quantum Gravity, establishing a direct connection between the full theory and inhomogeneous Bianchi I models to facilitate testing and understanding of quantum cosmology.
Contribution
It presents a new method to derive cosmological models from Loop Quantum Gravity by projecting the full theory onto a Bianchi I sector, linking quantum gravity with cosmological applications.
Findings
A new quantum cosmological model based on Loop Quantum Gravity.
A direct link established between full theory and cosmological sector.
Potential insights into Loop Quantum Cosmology and its relation to the full theory.
Abstract
We present a new cosmological model derived from Loop Quantum Gravity. The formulation is based on a projection of the kinematical Hilbert space of the full theory down to a subspace representing the proper arena for an inhomogeneous Bianchi I model. This procedure gives a direct link between the full theory and its cosmological sector. The emerging quantum cosmological model represents a simplified arena on which the complete canonical quantization program can be tested. The achievements of this analysis could also shed light on Loop Quantum Cosmology and its relation with the full theory.
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