Impact of dark energy on the equation of state in light of the latest cosmological data
Abstract We reconstruct the effective equation of state (EoS) within the framework of the general theory of relativity in a homogeneous and isotropic Friedmann–Lemaître–Robertson–Walker universe, which is assumed to be composed of matter and dark energy (DE). Our analysis employs a dataset consistin...
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Veröffentlicht in: | Progress of Theoretical and Experimental Physics 2023-09, Vol.2023 (9), p.1 |
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creator | Myrzakulov, N Koussour, M Alfedeel, Alnadhief H A Hassan, E I |
description | Abstract
We reconstruct the effective equation of state (EoS) within the framework of the general theory of relativity in a homogeneous and isotropic Friedmann–Lemaître–Robertson–Walker universe, which is assumed to be composed of matter and dark energy (DE). Our analysis employs a dataset consisting of 31 cosmic chronometer data points, six data points of baryon acoustic oscillations, and 1048 type Ia supernovae from the Pantheon sample, and we determine the best-fitting values of the model parameters through Markov chain Monte Carlo simulation. We then use these parameter values to calculate various cosmological parameters, such as the DE EoS parameter, the energy density, the deceleration parameter, the state-finder parameters, and the Om(z) diagnostic. All the analyzed cosmological parameters show behavior consistent with the accelerated universe scenario. |
doi_str_mv | 10.1093/ptep/ptad110 |
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We reconstruct the effective equation of state (EoS) within the framework of the general theory of relativity in a homogeneous and isotropic Friedmann–Lemaître–Robertson–Walker universe, which is assumed to be composed of matter and dark energy (DE). Our analysis employs a dataset consisting of 31 cosmic chronometer data points, six data points of baryon acoustic oscillations, and 1048 type Ia supernovae from the Pantheon sample, and we determine the best-fitting values of the model parameters through Markov chain Monte Carlo simulation. We then use these parameter values to calculate various cosmological parameters, such as the DE EoS parameter, the energy density, the deceleration parameter, the state-finder parameters, and the Om(z) diagnostic. All the analyzed cosmological parameters show behavior consistent with the accelerated universe scenario.</description><identifier>ISSN: 2050-3911</identifier><identifier>EISSN: 2050-3911</identifier><identifier>DOI: 10.1093/ptep/ptad110</identifier><language>eng</language><publisher>Oxford University Press</publisher><subject>Analysis ; Dark energy ; Markov processes ; Monte Carlo method</subject><ispartof>Progress of Theoretical and Experimental Physics, 2023-09, Vol.2023 (9), p.1</ispartof><rights>The Author(s) 2023. Published by Oxford University Press on behalf of the Physical Society of Japan. 2023</rights><rights>COPYRIGHT 2023 Oxford University Press</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c335t-5b948bafd4c05c24b34dcd20b249b3b33d29ac5e2457f0da9e8caf0fc5239bfc3</cites><orcidid>0000-0002-8036-268X ; 0000-0002-4188-0572 ; 0000-0001-8691-9939</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,864,1604,27924,27925</link.rule.ids></links><search><creatorcontrib>Myrzakulov, N</creatorcontrib><creatorcontrib>Koussour, M</creatorcontrib><creatorcontrib>Alfedeel, Alnadhief H A</creatorcontrib><creatorcontrib>Hassan, E I</creatorcontrib><title>Impact of dark energy on the equation of state in light of the latest cosmological data</title><title>Progress of Theoretical and Experimental Physics</title><description>Abstract
We reconstruct the effective equation of state (EoS) within the framework of the general theory of relativity in a homogeneous and isotropic Friedmann–Lemaître–Robertson–Walker universe, which is assumed to be composed of matter and dark energy (DE). Our analysis employs a dataset consisting of 31 cosmic chronometer data points, six data points of baryon acoustic oscillations, and 1048 type Ia supernovae from the Pantheon sample, and we determine the best-fitting values of the model parameters through Markov chain Monte Carlo simulation. We then use these parameter values to calculate various cosmological parameters, such as the DE EoS parameter, the energy density, the deceleration parameter, the state-finder parameters, and the Om(z) diagnostic. All the analyzed cosmological parameters show behavior consistent with the accelerated universe scenario.</description><subject>Analysis</subject><subject>Dark energy</subject><subject>Markov processes</subject><subject>Monte Carlo method</subject><issn>2050-3911</issn><issn>2050-3911</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>TOX</sourceid><recordid>eNp9kE1OwzAQhS0EElXpjgN4x4bA2E5IvawqfipVYgMSu2jin9SQxCF2F70NZ-FkuLQLVmikmdHM997iEXLJ4IaBFLdDNENqqBmDEzLhUEAmJGOnf_ZzMgvhHQAYlCXkbELeVt2AKlJvqcbxg5rejM2O-p7GjaHmc4vR-f77K_1DxGio62nrms2vYo-06RgiVT50vvWNU9gmp4gX5MxiG8zsOKfk9eH-ZfmUrZ8fV8vFOlNCFDErapnPa7Q6V1Aontci10pzqHkua1ELoblEVRieF6UFjdLMFVqwquBC1laJKbk5-DbYmsr11scRVSptOqd8b6xL90VZilKWjN8lwfVBoEYfwmhsNYyuw3FXMaj2SVb7JKtjkgm_OuB-O_xP_gD2IXeO</recordid><startdate>20230901</startdate><enddate>20230901</enddate><creator>Myrzakulov, N</creator><creator>Koussour, M</creator><creator>Alfedeel, Alnadhief H A</creator><creator>Hassan, E I</creator><general>Oxford University Press</general><scope>TOX</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>IAO</scope><orcidid>https://orcid.org/0000-0002-8036-268X</orcidid><orcidid>https://orcid.org/0000-0002-4188-0572</orcidid><orcidid>https://orcid.org/0000-0001-8691-9939</orcidid></search><sort><creationdate>20230901</creationdate><title>Impact of dark energy on the equation of state in light of the latest cosmological data</title><author>Myrzakulov, N ; Koussour, M ; Alfedeel, Alnadhief H A ; Hassan, E I</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c335t-5b948bafd4c05c24b34dcd20b249b3b33d29ac5e2457f0da9e8caf0fc5239bfc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Analysis</topic><topic>Dark energy</topic><topic>Markov processes</topic><topic>Monte Carlo method</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Myrzakulov, N</creatorcontrib><creatorcontrib>Koussour, M</creatorcontrib><creatorcontrib>Alfedeel, Alnadhief H A</creatorcontrib><creatorcontrib>Hassan, E I</creatorcontrib><collection>Oxford University Press Open Access</collection><collection>CrossRef</collection><collection>Gale Academic OneFile</collection><jtitle>Progress of Theoretical and Experimental Physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Myrzakulov, N</au><au>Koussour, M</au><au>Alfedeel, Alnadhief H A</au><au>Hassan, E I</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Impact of dark energy on the equation of state in light of the latest cosmological data</atitle><jtitle>Progress of Theoretical and Experimental Physics</jtitle><date>2023-09-01</date><risdate>2023</risdate><volume>2023</volume><issue>9</issue><spage>1</spage><pages>1-</pages><issn>2050-3911</issn><eissn>2050-3911</eissn><abstract>Abstract
We reconstruct the effective equation of state (EoS) within the framework of the general theory of relativity in a homogeneous and isotropic Friedmann–Lemaître–Robertson–Walker universe, which is assumed to be composed of matter and dark energy (DE). Our analysis employs a dataset consisting of 31 cosmic chronometer data points, six data points of baryon acoustic oscillations, and 1048 type Ia supernovae from the Pantheon sample, and we determine the best-fitting values of the model parameters through Markov chain Monte Carlo simulation. We then use these parameter values to calculate various cosmological parameters, such as the DE EoS parameter, the energy density, the deceleration parameter, the state-finder parameters, and the Om(z) diagnostic. All the analyzed cosmological parameters show behavior consistent with the accelerated universe scenario.</abstract><pub>Oxford University Press</pub><doi>10.1093/ptep/ptad110</doi><orcidid>https://orcid.org/0000-0002-8036-268X</orcidid><orcidid>https://orcid.org/0000-0002-4188-0572</orcidid><orcidid>https://orcid.org/0000-0001-8691-9939</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Analysis Dark energy Markov processes Monte Carlo method |
title | Impact of dark energy on the equation of state in light of the latest cosmological data |
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