Dynamical system analysis for a nonminimal torsion-matter coupled gravity
Autor(a) principal: | |
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Data de Publicação: | 2016 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
Texto Completo: | http://dx.doi.org/10.1103/PhysRevD.93.024034 http://hdl.handle.net/11449/172721 |
Resumo: | In this work, we perform a detailed dynamical analysis for the cosmological applications of a nonminimal torsion-matter coupled gravity. Two alternative formalisms are proposed, which enable one to choose between the easier approach for a given problem, and furthermore, we analyze six specific models. In general, we extract fixed points corresponding either to dark-matter-dominated, scaling decelerated solutions, or to dark-energy-dominated accelerated solutions. Additionally, we find that there is a small parameter region in which the model can experience the transition from the matter epoch to the dark-energy era. These features are in agreement with the observed evolution of the Universe, and make the theory a successful candidate for the description of nature. |
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Dynamical system analysis for a nonminimal torsion-matter coupled gravityIn this work, we perform a detailed dynamical analysis for the cosmological applications of a nonminimal torsion-matter coupled gravity. Two alternative formalisms are proposed, which enable one to choose between the easier approach for a given problem, and furthermore, we analyze six specific models. In general, we extract fixed points corresponding either to dark-matter-dominated, scaling decelerated solutions, or to dark-energy-dominated accelerated solutions. Additionally, we find that there is a small parameter region in which the model can experience the transition from the matter epoch to the dark-energy era. These features are in agreement with the observed evolution of the Universe, and make the theory a successful candidate for the description of nature.Centro Multidisciplinar de Astrofisica - CENTRA Instituto Superior Tecnico IST Universidade de Lisboa-UL, Avenida Rovisco Pais 1Instituto de Astrofísica e Ciências Do Espaço Faculdade de Ciências da Universidade de Lisboa, Edifício C8, Campo GrandeDepartamento de Matemática ICE Universidade Federal de Juiz de for AInstituto de Física Teórica UNESP-Universidade Estadual Paulista Caixa, Postal 70532-2CASPER Physics Department Baylor UniversityInstituto de Física Pontificia Universidad de Católica de Valparaíso, Casilla 4950Instituto de Física Teórica UNESP-Universidade Estadual Paulista Caixa, Postal 70532-2Universidade de Lisboa-ULFaculdade de Ciências da Universidade de LisboaUniversidade Federal de Juiz de for AUniversidade Estadual Paulista (Unesp)Baylor UniversityPontificia Universidad de Católica de ValparaísoCarloni, SanteLobo, Francisco S. N.Otalora, Giovanni [UNESP]Saridakis, Emmanuel N.2018-12-11T17:01:54Z2018-12-11T17:01:54Z2016-01-19info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://dx.doi.org/10.1103/PhysRevD.93.024034Physical Review D, v. 93, n. 2, 2016.2470-00292470-0010http://hdl.handle.net/11449/17272110.1103/PhysRevD.93.0240342-s2.0-849612896562-s2.0-84961289656.pdfScopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review D1,8011,801info:eu-repo/semantics/openAccess2023-12-07T06:19:53Zoai:repositorio.unesp.br:11449/172721Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T19:43:59.507182Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Dynamical system analysis for a nonminimal torsion-matter coupled gravity |
title |
Dynamical system analysis for a nonminimal torsion-matter coupled gravity |
spellingShingle |
Dynamical system analysis for a nonminimal torsion-matter coupled gravity Carloni, Sante |
title_short |
Dynamical system analysis for a nonminimal torsion-matter coupled gravity |
title_full |
Dynamical system analysis for a nonminimal torsion-matter coupled gravity |
title_fullStr |
Dynamical system analysis for a nonminimal torsion-matter coupled gravity |
title_full_unstemmed |
Dynamical system analysis for a nonminimal torsion-matter coupled gravity |
title_sort |
Dynamical system analysis for a nonminimal torsion-matter coupled gravity |
author |
Carloni, Sante |
author_facet |
Carloni, Sante Lobo, Francisco S. N. Otalora, Giovanni [UNESP] Saridakis, Emmanuel N. |
author_role |
author |
author2 |
Lobo, Francisco S. N. Otalora, Giovanni [UNESP] Saridakis, Emmanuel N. |
author2_role |
author author author |
dc.contributor.none.fl_str_mv |
Universidade de Lisboa-UL Faculdade de Ciências da Universidade de Lisboa Universidade Federal de Juiz de for A Universidade Estadual Paulista (Unesp) Baylor University Pontificia Universidad de Católica de Valparaíso |
dc.contributor.author.fl_str_mv |
Carloni, Sante Lobo, Francisco S. N. Otalora, Giovanni [UNESP] Saridakis, Emmanuel N. |
description |
In this work, we perform a detailed dynamical analysis for the cosmological applications of a nonminimal torsion-matter coupled gravity. Two alternative formalisms are proposed, which enable one to choose between the easier approach for a given problem, and furthermore, we analyze six specific models. In general, we extract fixed points corresponding either to dark-matter-dominated, scaling decelerated solutions, or to dark-energy-dominated accelerated solutions. Additionally, we find that there is a small parameter region in which the model can experience the transition from the matter epoch to the dark-energy era. These features are in agreement with the observed evolution of the Universe, and make the theory a successful candidate for the description of nature. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-01-19 2018-12-11T17:01:54Z 2018-12-11T17:01:54Z |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://dx.doi.org/10.1103/PhysRevD.93.024034 Physical Review D, v. 93, n. 2, 2016. 2470-0029 2470-0010 http://hdl.handle.net/11449/172721 10.1103/PhysRevD.93.024034 2-s2.0-84961289656 2-s2.0-84961289656.pdf |
url |
http://dx.doi.org/10.1103/PhysRevD.93.024034 http://hdl.handle.net/11449/172721 |
identifier_str_mv |
Physical Review D, v. 93, n. 2, 2016. 2470-0029 2470-0010 10.1103/PhysRevD.93.024034 2-s2.0-84961289656 2-s2.0-84961289656.pdf |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
Physical Review D 1,801 1,801 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
Scopus reponame:Repositório Institucional da UNESP instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808129110255337472 |