Averaging generalized scalar field cosmologies IV: locally rotationally symmetric Bianchi V model

Abstract This research focuses on scalar field cosmologies with a generalized harmonic potential. Our attention is centred on the anisotropic LRS Bianchi I and III metrics, Bianchi V metrics, and their isotropic limits. We provide a comprehensive overview of the first two metrics classes and offer n...

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Main Authors: Alfredo D. Millano, Genly Leon
Format: Article
Language:English
Published: SpringerOpen 2024-01-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-023-12366-1
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author Alfredo D. Millano
Genly Leon
author_facet Alfredo D. Millano
Genly Leon
author_sort Alfredo D. Millano
collection DOAJ
description Abstract This research focuses on scalar field cosmologies with a generalized harmonic potential. Our attention is centred on the anisotropic LRS Bianchi I and III metrics, Bianchi V metrics, and their isotropic limits. We provide a comprehensive overview of the first two metrics classes and offer new findings for Bianchi V metrics. We show that the Hubble parameter is a time-dependent perturbation parameter that controls the magnitude of the error between full-system and time-averaged solutions as it decreases, such that those complete and time-averaged systems have the same asymptotic behaviour. Therefore, oscillations entering the system can be controlled and smoothed out, simplifying the problem.
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spelling doaj.art-b1f1ff7f934544579b4768823908a0aa2024-03-31T11:33:12ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522024-01-0184112210.1140/epjc/s10052-023-12366-1Averaging generalized scalar field cosmologies IV: locally rotationally symmetric Bianchi V modelAlfredo D. Millano0Genly Leon1Departamento de Matemáticas, Universidad Católica del NorteDepartamento de Matemáticas, Universidad Católica del NorteAbstract This research focuses on scalar field cosmologies with a generalized harmonic potential. Our attention is centred on the anisotropic LRS Bianchi I and III metrics, Bianchi V metrics, and their isotropic limits. We provide a comprehensive overview of the first two metrics classes and offer new findings for Bianchi V metrics. We show that the Hubble parameter is a time-dependent perturbation parameter that controls the magnitude of the error between full-system and time-averaged solutions as it decreases, such that those complete and time-averaged systems have the same asymptotic behaviour. Therefore, oscillations entering the system can be controlled and smoothed out, simplifying the problem.https://doi.org/10.1140/epjc/s10052-023-12366-1
spellingShingle Alfredo D. Millano
Genly Leon
Averaging generalized scalar field cosmologies IV: locally rotationally symmetric Bianchi V model
European Physical Journal C: Particles and Fields
title Averaging generalized scalar field cosmologies IV: locally rotationally symmetric Bianchi V model
title_full Averaging generalized scalar field cosmologies IV: locally rotationally symmetric Bianchi V model
title_fullStr Averaging generalized scalar field cosmologies IV: locally rotationally symmetric Bianchi V model
title_full_unstemmed Averaging generalized scalar field cosmologies IV: locally rotationally symmetric Bianchi V model
title_short Averaging generalized scalar field cosmologies IV: locally rotationally symmetric Bianchi V model
title_sort averaging generalized scalar field cosmologies iv locally rotationally symmetric bianchi v model
url https://doi.org/10.1140/epjc/s10052-023-12366-1
work_keys_str_mv AT alfredodmillano averaginggeneralizedscalarfieldcosmologiesivlocallyrotationallysymmetricbianchivmodel
AT genlyleon averaginggeneralizedscalarfieldcosmologiesivlocallyrotationallysymmetricbianchivmodel