Loop quantum cosmology of Bianchi I models
Abhay Ashtekar, Edward Wilson-Ewing

TL;DR
This paper extends loop quantum cosmology to anisotropic Bianchi I models, resolving singularities and providing insights into generic space-like singularities and their relation to simpler models.
Contribution
The work develops a complete quantum description of Bianchi I models in LQC, overcoming previous limitations and establishing a precise connection to Friedmann models.
Findings
Big bang singularity is resolved by quantum geometry effects.
Quantum dynamics of Bianchi I projects exactly onto Friedmann models.
Rich Planck scale physics due to Weyl curvature in anisotropic models.
Abstract
The "improved dynamics" of loop quantum cosmology is extended to include anisotropies of the Bianchi I model. As in the isotropic case, a massless scalar field serves as a relational time parameter. However, the extension is non-trivial because one has to face several conceptual subtleties as well as technical difficulties. These include: a better understanding of the relation between loop quantum gravity (LQG) and loop quantum cosmology (LQC); handling novel features associated with the non-local field strength operator in presence of anisotropies; and finding dynamical variables that make the action of the Hamiltonian constraint manageable. Our analysis provides a conceptually complete description that overcomes limitations of earlier works. We again find that the big bang singularity is resolved by quantum geometry effects but, because of the presence of Weyl curvature, Planck scale…
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