The Dapor–Liegener model of loop quantum cosmology: a dynamical analysis

Abstract The Dapor–Liegener model of loop quantum cosmology (LQC), which depicts an emergent universe from a de Sitter regime in the contracting phase is studied from the mathematical viewpoint of dynamical systems and compared with the standard model of LQC. Dealing with perturbations, on the contr...

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Main Author: Jaume de Haro
Format: Article
Language:English
Published: SpringerOpen 2018-11-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-6402-z
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author Jaume de Haro
author_facet Jaume de Haro
author_sort Jaume de Haro
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description Abstract The Dapor–Liegener model of loop quantum cosmology (LQC), which depicts an emergent universe from a de Sitter regime in the contracting phase is studied from the mathematical viewpoint of dynamical systems and compared with the standard model of LQC. Dealing with perturbations, on the contrary to standard LQC where at early times all the scales are inside the Hubble radius, we show that it is impossible to implement the matter bounce scenario due to the fact that an emergent de Sitter regime in the contracting phase implies that all the scales are outside of the Hubble radius in a past epoch.
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spelling doaj.art-ee96a9d2e2cf4b30ae5387b4265d6e212022-12-21T19:54:59ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-11-0178111910.1140/epjc/s10052-018-6402-zThe Dapor–Liegener model of loop quantum cosmology: a dynamical analysisJaume de Haro0Departament de Matemàtiques, Universitat Politècnica de CatalunyaAbstract The Dapor–Liegener model of loop quantum cosmology (LQC), which depicts an emergent universe from a de Sitter regime in the contracting phase is studied from the mathematical viewpoint of dynamical systems and compared with the standard model of LQC. Dealing with perturbations, on the contrary to standard LQC where at early times all the scales are inside the Hubble radius, we show that it is impossible to implement the matter bounce scenario due to the fact that an emergent de Sitter regime in the contracting phase implies that all the scales are outside of the Hubble radius in a past epoch.http://link.springer.com/article/10.1140/epjc/s10052-018-6402-z
spellingShingle Jaume de Haro
The Dapor–Liegener model of loop quantum cosmology: a dynamical analysis
European Physical Journal C: Particles and Fields
title The Dapor–Liegener model of loop quantum cosmology: a dynamical analysis
title_full The Dapor–Liegener model of loop quantum cosmology: a dynamical analysis
title_fullStr The Dapor–Liegener model of loop quantum cosmology: a dynamical analysis
title_full_unstemmed The Dapor–Liegener model of loop quantum cosmology: a dynamical analysis
title_short The Dapor–Liegener model of loop quantum cosmology: a dynamical analysis
title_sort dapor liegener model of loop quantum cosmology a dynamical analysis
url http://link.springer.com/article/10.1140/epjc/s10052-018-6402-z
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