Testing loop quantum cosmology
arXiv:1612.04551 · doi:10.1016/j.crhy.2017.02.004
Abstract
Loop quantum cosmology predicts that quantum gravity effects resolve the big-bang singularity and replace it by a cosmic bounce. Furthermore, loop quantum cosmology can also modify the form of primordial cosmological perturbations, for example by reducing power at large scales in inflationary models or by suppressing the tensor-to-scalar ratio in the matter bounce scenario; these two effects are potential observational tests for loop quantum cosmology. In this article, I review these predictions and others, and also briefly discuss three open problems in loop quantum cosmology: its relation to loop quantum gravity, the trans-Planckian problem, and a possible transition from a Lorentzian to a Euclidean space-time around the bounce point.
20 pages. Invited review for special edition "Testing quantum gravity with cosmology" of Comptes Rendus Physique
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Cited by in corpus (48)
- A Short Review of Loop Quantum Gravity
- Towards Cosmological Dynamics from Loop Quantum Gravity
- Effective loop quantum cosmology as a higher-derivative scalar-tensor theory
- Hybrid Loop Quantum Cosmology: An Overview
- Primordial scalar power spectrum from the hybrid approach in loop cosmologies
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- Probability of Warm Inflation in Loop Quantum Cosmology
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