Dynamical system analysis of FLRW models with Modified Chaplygin gas

Abstract We investigate Friedmann–Lamaitre–Robertson–Walker (FLRW) models with modified Chaplygin gas and cosmological constant, using dynamical system methods. We assume $$p=(\gamma -1)\mu -\dfrac{A}{\mu ^\alpha }$$ p = ( γ - 1 ) μ - A μ α as equation of state where $$\mu$$ μ is the matter-energy d...

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Main Authors: Ali Osman Yılmaz, Ertan Güdekli
Format: Article
Language:English
Published: Nature Portfolio 2021-02-01
Series:Scientific Reports
Online Access:https://doi.org/10.1038/s41598-020-80396-w
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author Ali Osman Yılmaz
Ertan Güdekli
author_facet Ali Osman Yılmaz
Ertan Güdekli
author_sort Ali Osman Yılmaz
collection DOAJ
description Abstract We investigate Friedmann–Lamaitre–Robertson–Walker (FLRW) models with modified Chaplygin gas and cosmological constant, using dynamical system methods. We assume $$p=(\gamma -1)\mu -\dfrac{A}{\mu ^\alpha }$$ p = ( γ - 1 ) μ - A μ α as equation of state where $$\mu$$ μ is the matter-energy density, p is the pressure, $$\alpha$$ α is a parameter which can take on values $$0<\alpha \le 1$$ 0 < α ≤ 1 as well as A and $$\gamma$$ γ are positive constants. We draw the state spaces and analyze the nature of the singularity at the beginning, as well as the fate of the universe in the far future. In particular, we address the question whether there is a solution which is stable for all the cases.
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spelling doaj.art-ff106acd3a9a4ca88a8aadf7244248892022-12-21T21:20:53ZengNature PortfolioScientific Reports2045-23222021-02-011111910.1038/s41598-020-80396-wDynamical system analysis of FLRW models with Modified Chaplygin gasAli Osman Yılmaz0Ertan Güdekli1Department of Physics, Istanbul UniversityDepartment of Physics, Istanbul UniversityAbstract We investigate Friedmann–Lamaitre–Robertson–Walker (FLRW) models with modified Chaplygin gas and cosmological constant, using dynamical system methods. We assume $$p=(\gamma -1)\mu -\dfrac{A}{\mu ^\alpha }$$ p = ( γ - 1 ) μ - A μ α as equation of state where $$\mu$$ μ is the matter-energy density, p is the pressure, $$\alpha$$ α is a parameter which can take on values $$0<\alpha \le 1$$ 0 < α ≤ 1 as well as A and $$\gamma$$ γ are positive constants. We draw the state spaces and analyze the nature of the singularity at the beginning, as well as the fate of the universe in the far future. In particular, we address the question whether there is a solution which is stable for all the cases.https://doi.org/10.1038/s41598-020-80396-w
spellingShingle Ali Osman Yılmaz
Ertan Güdekli
Dynamical system analysis of FLRW models with Modified Chaplygin gas
Scientific Reports
title Dynamical system analysis of FLRW models with Modified Chaplygin gas
title_full Dynamical system analysis of FLRW models with Modified Chaplygin gas
title_fullStr Dynamical system analysis of FLRW models with Modified Chaplygin gas
title_full_unstemmed Dynamical system analysis of FLRW models with Modified Chaplygin gas
title_short Dynamical system analysis of FLRW models with Modified Chaplygin gas
title_sort dynamical system analysis of flrw models with modified chaplygin gas
url https://doi.org/10.1038/s41598-020-80396-w
work_keys_str_mv AT aliosmanyılmaz dynamicalsystemanalysisofflrwmodelswithmodifiedchaplygingas
AT ertangudekli dynamicalsystemanalysisofflrwmodelswithmodifiedchaplygingas