Effective loop quantum cosmology as a higher-derivative scalar-tensor theory
arXiv:1703.10812 · doi:10.1088/1361-6382/aa8f2f
Abstract
Recently, Chamseddine and Mukhanov introduced a higher-derivative scalar-tensor theory which leads to a modified Friedmann equation allowing for bouncing solutions. As we note in the present work, this Friedmann equation turns out to reproduce exactly the loop quantum cosmology effective dynamics for a flat isotropic and homogeneous space-time. We generalize this result to obtain a class of scalar-tensor theories, belonging to the family of mimetic gravity, which all reproduce the loop quantum cosmology effective dynamics for flat, closed and open isotropic and homogeneous space-times.
22 pages. v2: minor clarifications added, references updated
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