Stability of a Viable Non-Minimal Bounce

The main difficulties in constructing a viable early Universe bouncing model are: to bypass the observational and theoretical no-go theorem, to construct a stable non-singular bouncing phase, and perhaps, the major concern of it is to construct a stable attractor solution which can evade the Belinsk...

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Main Author: Debottam Nandi
Format: Article
Language:English
Published: MDPI AG 2021-03-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/7/3/62
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author Debottam Nandi
author_facet Debottam Nandi
author_sort Debottam Nandi
collection DOAJ
description The main difficulties in constructing a viable early Universe bouncing model are: to bypass the observational and theoretical no-go theorem, to construct a stable non-singular bouncing phase, and perhaps, the major concern of it is to construct a stable attractor solution which can evade the Belinsky–Khalatnikov–Lifshitz (BKL) instability as well. In this article, in the homogeneous and isotropic background, we extensively study the stability analysis of the recently proposed viable non-minimal bouncing theory in the presence of an additional barotropic fluid and show that, the bouncing solution remains stable and can evade BKL instability for a wide range of the model parameter. We provide the expressions that explain the behavior of the Universe in the vicinity of the required fixed point i.e., the bouncing solution and compare our results with the minimal theory and show that ekpyrosis is the most stable solution in any scenario.
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spelling doaj.art-be09c91dced344ac9f6bc3becc6871e62023-11-21T09:49:57ZengMDPI AGUniverse2218-19972021-03-01736210.3390/universe7030062Stability of a Viable Non-Minimal BounceDebottam Nandi0Department of Physics, Indian Institute of Technology Madras, Chennai 600036, IndiaThe main difficulties in constructing a viable early Universe bouncing model are: to bypass the observational and theoretical no-go theorem, to construct a stable non-singular bouncing phase, and perhaps, the major concern of it is to construct a stable attractor solution which can evade the Belinsky–Khalatnikov–Lifshitz (BKL) instability as well. In this article, in the homogeneous and isotropic background, we extensively study the stability analysis of the recently proposed viable non-minimal bouncing theory in the presence of an additional barotropic fluid and show that, the bouncing solution remains stable and can evade BKL instability for a wide range of the model parameter. We provide the expressions that explain the behavior of the Universe in the vicinity of the required fixed point i.e., the bouncing solution and compare our results with the minimal theory and show that ekpyrosis is the most stable solution in any scenario.https://www.mdpi.com/2218-1997/7/3/62bounceinflationconformal transformationmodified gravitynon-minimal couplingstability
spellingShingle Debottam Nandi
Stability of a Viable Non-Minimal Bounce
Universe
bounce
inflation
conformal transformation
modified gravity
non-minimal coupling
stability
title Stability of a Viable Non-Minimal Bounce
title_full Stability of a Viable Non-Minimal Bounce
title_fullStr Stability of a Viable Non-Minimal Bounce
title_full_unstemmed Stability of a Viable Non-Minimal Bounce
title_short Stability of a Viable Non-Minimal Bounce
title_sort stability of a viable non minimal bounce
topic bounce
inflation
conformal transformation
modified gravity
non-minimal coupling
stability
url https://www.mdpi.com/2218-1997/7/3/62
work_keys_str_mv AT debottamnandi stabilityofaviablenonminimalbounce