Constraining deceleration, jerk and transition redshift using cosmic chronometers, Type Ia supernovae and ISW effect
In this study we present constraints on the deceleration (q) and jerk (j) parameters using the late time integrated Sachs-Wolfe effect, type Ia supernovae, and H(z) data . We first directly measure the deceleration and jerk parameters using the cosmic chronometers data with the Taylor series express...
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description | In this study we present constraints on the deceleration (q) and jerk (j) parameters using the late time integrated Sachs-Wolfe effect, type Ia supernovae, and H(z) data . We first directly measure the deceleration and jerk parameters using the cosmic chronometers data with the Taylor series expression of H(z).However, due to the unusual variations in the deceleration parameter with slight changes in other parameters like snap (s) and lerk (l), we found that direct measurements using the series expression of the H(z) is not a suitable method for non-Lambda-CDM models and so we will need to derive the deceleration parameter after constraining density parameters and dark energy equation of state parameters. Then we present derived values of the deceleration parameter from Lambda CDM, WCDM and CPL models. We also discuss the transition redshift (zt) in relation with the deceleration parameter. |
doi_str_mv | 10.48550/arxiv.2108.05409 |
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We first directly measure the deceleration and jerk parameters using the cosmic chronometers data with the Taylor series expression of H(z).However, due to the unusual variations in the deceleration parameter with slight changes in other parameters like snap (s) and lerk (l), we found that direct measurements using the series expression of the H(z) is not a suitable method for non-Lambda-CDM models and so we will need to derive the deceleration parameter after constraining density parameters and dark energy equation of state parameters. Then we present derived values of the deceleration parameter from Lambda CDM, WCDM and CPL models. We also discuss the transition redshift (zt) in relation with the deceleration parameter.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2108.05409</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Chronometers ; Constraining ; Dark energy ; Deceleration ; Equations of state ; Mathematical models ; Measuring instruments ; Parameters ; Physics - Cosmology and Nongalactic Astrophysics ; Red shift ; Supernovae ; Taylor series</subject><ispartof>arXiv.org, 2022-02</ispartof><rights>2022. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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We also discuss the transition redshift (zt) in relation with the deceleration parameter.</description><subject>Chronometers</subject><subject>Constraining</subject><subject>Dark energy</subject><subject>Deceleration</subject><subject>Equations of state</subject><subject>Mathematical models</subject><subject>Measuring instruments</subject><subject>Parameters</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Red shift</subject><subject>Supernovae</subject><subject>Taylor series</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotkEtLAzEUhYMgWGp_gCsDbjs1k9dMllJ8FAouLLgcMpMbm9omY5Ip9t_bh6sL555zOHwI3ZVkxmshyKOOv24_oyWpZ0Rwoq7QiDJWFjWn9AZNUtoQQqisqBBshPI8-JSjdt75L2yggy1EnV3wU7yB-I21N_j498mdRBzBpLWzGQ_pFOhC2rkOd-sYfNhBhpimeHXoAS80TkMP0Ye9hnPL4uMTg7XQ5Vt0bfU2weT_jtHq5Xk1fyuW76-L-dOy0EqoQkhOmAUqWVmpurS2NZTximsmaauUNLRteVkRqloqdUdM3QI3lDCQwnag2RjdX2rPSJo-up2Oh-aEpjmjOToeLo4-hp8BUm42YYj-uKmhQhIlalYy9ged8WgH</recordid><startdate>20220217</startdate><enddate>20220217</enddate><creator>ur Rahman, Syed Faisal</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20220217</creationdate><title>Constraining deceleration, jerk and transition redshift using cosmic chronometers, Type Ia supernovae and ISW effect</title><author>ur Rahman, Syed Faisal</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a959-56403fe26317981ffbd23474a362b996d2bb417029b26ac0d8be4d203e65fcea3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Chronometers</topic><topic>Constraining</topic><topic>Dark energy</topic><topic>Deceleration</topic><topic>Equations of state</topic><topic>Mathematical models</topic><topic>Measuring instruments</topic><topic>Parameters</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Red shift</topic><topic>Supernovae</topic><topic>Taylor series</topic><toplevel>online_resources</toplevel><creatorcontrib>ur Rahman, Syed Faisal</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>ur Rahman, Syed Faisal</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Constraining deceleration, jerk and transition redshift using cosmic chronometers, Type Ia supernovae and ISW effect</atitle><jtitle>arXiv.org</jtitle><date>2022-02-17</date><risdate>2022</risdate><eissn>2331-8422</eissn><abstract>In this study we present constraints on the deceleration (q) and jerk (j) parameters using the late time integrated Sachs-Wolfe effect, type Ia supernovae, and H(z) data . We first directly measure the deceleration and jerk parameters using the cosmic chronometers data with the Taylor series expression of H(z).However, due to the unusual variations in the deceleration parameter with slight changes in other parameters like snap (s) and lerk (l), we found that direct measurements using the series expression of the H(z) is not a suitable method for non-Lambda-CDM models and so we will need to derive the deceleration parameter after constraining density parameters and dark energy equation of state parameters. Then we present derived values of the deceleration parameter from Lambda CDM, WCDM and CPL models. We also discuss the transition redshift (zt) in relation with the deceleration parameter.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2108.05409</doi><oa>free_for_read</oa></addata></record> |
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subjects | Chronometers Constraining Dark energy Deceleration Equations of state Mathematical models Measuring instruments Parameters Physics - Cosmology and Nongalactic Astrophysics Red shift Supernovae Taylor series |
title | Constraining deceleration, jerk and transition redshift using cosmic chronometers, Type Ia supernovae and ISW effect |
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