Non-bouncing solutions in loop quantum cosmology

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According to the Belinskii-Khalatnikov-Lifshitz scenario, a collapsing universe approaching a spacelike singularity can be approximated by homogeneous cosmological dynamics, but only if asymptotically small spatial regions are considered. It is shown here that the relevant small-volume behavior in solvable models of loop quantum cosmology is crucially different from the large-volume behavior exclusively studied so far. While bouncing solutions exist and may even be generic within a given quantum representation, they are not generic if quantization ambiguities such as choices of representations are taken into account. The analysis reveals an interesting interplay between sl(2,R)-representation theory and canonical effective theory.

Original languageEnglish (US)
Article number029
JournalJournal of Cosmology and Astroparticle Physics
Issue number7
StatePublished - Jul 2020

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics


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