Dark Energy as a Natural Property of Cosmic Polytropes—A Tutorial

A conventional approach to the dark energy (DE) concept is reviewed and discussed. According to it, there is absolutely no need for a novel DE component in the universe, provided that its matter–energy content is represented by a perfect fluid whose volume elements perform polytropic flows. When the...

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Main Authors: Kostas Kleidis, Nikolaos K. Spyrou
Format: Article
Language:English
Published: MDPI AG 2023-02-01
Series:Dynamics
Subjects:
Online Access:https://www.mdpi.com/2673-8716/3/1/6
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author Kostas Kleidis
Nikolaos K. Spyrou
author_facet Kostas Kleidis
Nikolaos K. Spyrou
author_sort Kostas Kleidis
collection DOAJ
description A conventional approach to the dark energy (DE) concept is reviewed and discussed. According to it, there is absolutely no need for a novel DE component in the universe, provided that its matter–energy content is represented by a perfect fluid whose volume elements perform polytropic flows. When the (thermodynamic) energy of the associated internal motions is taken into account as an additional source of the universal gravitational field, it compensates the DE needed to compromise spatial flatness in an accelerating universe. The unified model which is driven by a polytropic fluid not only interprets the observations associated with universe expansion but successfully confronts all the current issues of cosmological significance, thus arising as a viable alternative to the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mo>Λ</mo></semantics></math></inline-formula>CDM model.
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spelling doaj.art-1c4f3adfedc142a89a13fc46ca370ca52023-11-17T10:40:10ZengMDPI AGDynamics2673-87162023-02-0131719510.3390/dynamics3010006Dark Energy as a Natural Property of Cosmic Polytropes—A TutorialKostas Kleidis0Nikolaos K. Spyrou1Department of Mechanical Engineering, International Hellenic University, Serres Campus, 621 24 Serres, GreeceDepartment of Astronomy, Aristotle University of Thessaloniki, 541 24 Thessaloniki, GreeceA conventional approach to the dark energy (DE) concept is reviewed and discussed. According to it, there is absolutely no need for a novel DE component in the universe, provided that its matter–energy content is represented by a perfect fluid whose volume elements perform polytropic flows. When the (thermodynamic) energy of the associated internal motions is taken into account as an additional source of the universal gravitational field, it compensates the DE needed to compromise spatial flatness in an accelerating universe. The unified model which is driven by a polytropic fluid not only interprets the observations associated with universe expansion but successfully confronts all the current issues of cosmological significance, thus arising as a viable alternative to the <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mo>Λ</mo></semantics></math></inline-formula>CDM model.https://www.mdpi.com/2673-8716/3/1/6dark matterdark energyaccelerating universepolytropic flows
spellingShingle Kostas Kleidis
Nikolaos K. Spyrou
Dark Energy as a Natural Property of Cosmic Polytropes—A Tutorial
Dynamics
dark matter
dark energy
accelerating universe
polytropic flows
title Dark Energy as a Natural Property of Cosmic Polytropes—A Tutorial
title_full Dark Energy as a Natural Property of Cosmic Polytropes—A Tutorial
title_fullStr Dark Energy as a Natural Property of Cosmic Polytropes—A Tutorial
title_full_unstemmed Dark Energy as a Natural Property of Cosmic Polytropes—A Tutorial
title_short Dark Energy as a Natural Property of Cosmic Polytropes—A Tutorial
title_sort dark energy as a natural property of cosmic polytropes a tutorial
topic dark matter
dark energy
accelerating universe
polytropic flows
url https://www.mdpi.com/2673-8716/3/1/6
work_keys_str_mv AT kostaskleidis darkenergyasanaturalpropertyofcosmicpolytropesatutorial
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