Exhaustive investigation of the duration of inflation in effective anisotropic loop quantum cosmology
arXiv:1405.1753 · doi:10.1088/0264-9381/32/3/035010
Abstract
This article addresses the issue of estimating the duration in inflation in bouncing cosmology when anisotropies, inevitably playing an important role, are taken into account. It is shown that in Bianchi-I loop quantum cosmology, the higher the shear, the shorter the period of inflation. In a range of parameters, the probability distribution function of the duration of inflation is however peaked at values compatible with data, but not much higher. This makes the whole bounce/inflationary scenario consistent and phenomenologically appealing as all the information from the bounce might then not have been fully washed out.
9 pagaes, 6 figures
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Cited by in corpus (10)
- An Overview on the Nature of the Bounce in LQC and PQM
- Warm bounce in loop quantum cosmology and the prediction for the duration of inflation
- Unavoidable shear from quantum fluctuations in contracting cosmologies
- Constraining the Barbero-Immirzi parameter from the duration of inflation in loop quantum cosmology
- A pure general relativistic non-singular bouncing origin for the Universe
- Cosmological implications of generalized holonomy corrections
- Impact of generalized holonomy corrections on the cosmological primordial power spectra
- -attractor potentials in loop quantum cosmology
- Quantum geometric formulation of Brans-Dicke theory for Bianchi I spacetime
- Ekpyrosis in Quantum Gravitational Anisotropic Bouncing Models