Dynamical system analysis and observational constraints of cosmological models in mimetic gravity
We study the dynamics of homogeneous and isotropic Friedmann-Lema\^itre-Robertson-Walker cosmological models with positive spatial curvature within the context of mimetic gravity theory by employing dynamical system techniques. Our analysis yields phase-space trajectories that describe physically re...
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creator | Fritis, Alberto Villalobos-Silva, Daniel Vásquez, Yerko López-Caraballo, Carlos H Helo, Juan Carlos |
description | We study the dynamics of homogeneous and isotropic
Friedmann-Lema\^itre-Robertson-Walker cosmological models with positive spatial
curvature within the context of mimetic gravity theory by employing dynamical
system techniques. Our analysis yields phase-space trajectories that describe
physically relevant solutions, capturing various stages of cosmic evolution. We
also employ Bayesian statistical analysis to constrain the cosmological
parameters of the models, utilizing data from Type Ia supernovae and Hubble
parameter data sets. The observational data sets provide support for the
viability of mimetic gravity models, which can effectively describe the
late-time accelerated expansion of the universe. |
doi_str_mv | 10.48550/arxiv.2312.07765 |
format | Article |
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Friedmann-Lema\^itre-Robertson-Walker cosmological models with positive spatial
curvature within the context of mimetic gravity theory by employing dynamical
system techniques. Our analysis yields phase-space trajectories that describe
physically relevant solutions, capturing various stages of cosmic evolution. We
also employ Bayesian statistical analysis to constrain the cosmological
parameters of the models, utilizing data from Type Ia supernovae and Hubble
parameter data sets. The observational data sets provide support for the
viability of mimetic gravity models, which can effectively describe the
late-time accelerated expansion of the universe.</description><identifier>DOI: 10.48550/arxiv.2312.07765</identifier><language>eng</language><subject>Physics - General Relativity and Quantum Cosmology ; Physics - High Energy Physics - Theory</subject><creationdate>2023-12</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2312.07765$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2312.07765$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Fritis, Alberto</creatorcontrib><creatorcontrib>Villalobos-Silva, Daniel</creatorcontrib><creatorcontrib>Vásquez, Yerko</creatorcontrib><creatorcontrib>López-Caraballo, Carlos H</creatorcontrib><creatorcontrib>Helo, Juan Carlos</creatorcontrib><title>Dynamical system analysis and observational constraints of cosmological models in mimetic gravity</title><description>We study the dynamics of homogeneous and isotropic
Friedmann-Lema\^itre-Robertson-Walker cosmological models with positive spatial
curvature within the context of mimetic gravity theory by employing dynamical
system techniques. Our analysis yields phase-space trajectories that describe
physically relevant solutions, capturing various stages of cosmic evolution. We
also employ Bayesian statistical analysis to constrain the cosmological
parameters of the models, utilizing data from Type Ia supernovae and Hubble
parameter data sets. The observational data sets provide support for the
viability of mimetic gravity models, which can effectively describe the
late-time accelerated expansion of the universe.</description><subject>Physics - General Relativity and Quantum Cosmology</subject><subject>Physics - High Energy Physics - Theory</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj81qwzAQhHXpoSR9gJ6qF7ArS5bkHEP6C4FccjerHweBZRVJmOrtq7qFhd2ZZQY-hB470vYD5-QZ4rdbW8o62hIpBb9H8FIW8E7DjFNJ2XoMC8wluVQPg4NKNq6QXagu1mFJOYJbcsJhqjL5MIfblvbB2Dlht2DvvM1O41uE1eWyR3cTzMk-_O8dur69Xk8fzfny_nk6nhsQkjcTN5QwafqODMySOsLYjkxkEL1SSlJGBT0wyYiWHeN8EkrwXtfPQVELwHbo6a92Yxy_ovMQy_jLOm6s7AcutFC_</recordid><startdate>20231212</startdate><enddate>20231212</enddate><creator>Fritis, Alberto</creator><creator>Villalobos-Silva, Daniel</creator><creator>Vásquez, Yerko</creator><creator>López-Caraballo, Carlos H</creator><creator>Helo, Juan Carlos</creator><scope>GOX</scope></search><sort><creationdate>20231212</creationdate><title>Dynamical system analysis and observational constraints of cosmological models in mimetic gravity</title><author>Fritis, Alberto ; Villalobos-Silva, Daniel ; Vásquez, Yerko ; López-Caraballo, Carlos H ; Helo, Juan Carlos</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a675-f5d2037d41083e03e06de10f0864bbb72326293730c71355f6b654cbb79b2eaa3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Physics - General Relativity and Quantum Cosmology</topic><topic>Physics - High Energy Physics - Theory</topic><toplevel>online_resources</toplevel><creatorcontrib>Fritis, Alberto</creatorcontrib><creatorcontrib>Villalobos-Silva, Daniel</creatorcontrib><creatorcontrib>Vásquez, Yerko</creatorcontrib><creatorcontrib>López-Caraballo, Carlos H</creatorcontrib><creatorcontrib>Helo, Juan Carlos</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Fritis, Alberto</au><au>Villalobos-Silva, Daniel</au><au>Vásquez, Yerko</au><au>López-Caraballo, Carlos H</au><au>Helo, Juan Carlos</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Dynamical system analysis and observational constraints of cosmological models in mimetic gravity</atitle><date>2023-12-12</date><risdate>2023</risdate><abstract>We study the dynamics of homogeneous and isotropic
Friedmann-Lema\^itre-Robertson-Walker cosmological models with positive spatial
curvature within the context of mimetic gravity theory by employing dynamical
system techniques. Our analysis yields phase-space trajectories that describe
physically relevant solutions, capturing various stages of cosmic evolution. We
also employ Bayesian statistical analysis to constrain the cosmological
parameters of the models, utilizing data from Type Ia supernovae and Hubble
parameter data sets. The observational data sets provide support for the
viability of mimetic gravity models, which can effectively describe the
late-time accelerated expansion of the universe.</abstract><doi>10.48550/arxiv.2312.07765</doi><oa>free_for_read</oa></addata></record> |
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subjects | Physics - General Relativity and Quantum Cosmology Physics - High Energy Physics - Theory |
title | Dynamical system analysis and observational constraints of cosmological models in mimetic gravity |
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