Modeling Dark Sector in Horndeski Gravity at First-Order Formalism

We investigate a cosmological scenario by finding solutions using first-order formalism in the Horndeski gravity that constrains the superpotential and implies that no free choice of scalar potential is allowed. Despite this, we show that a de Sitter phase at late-time cosmology can be realized, whe...

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Main Authors: F. F. Santos, R. M. P. Neves, F. A. Brito
Format: Article
Language:English
Published: Wiley 2019-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2019/3486805
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author F. F. Santos
R. M. P. Neves
F. A. Brito
author_facet F. F. Santos
R. M. P. Neves
F. A. Brito
author_sort F. F. Santos
collection DOAJ
description We investigate a cosmological scenario by finding solutions using first-order formalism in the Horndeski gravity that constrains the superpotential and implies that no free choice of scalar potential is allowed. Despite this, we show that a de Sitter phase at late-time cosmology can be realized, where the dark energy sector can be identified. The scalar field equation of state tends to the cosmological scenario at present time and allows us to conclude that it can simulate the dark energy in the Horndeski gravity.
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institution Kabale University
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series Advances in High Energy Physics
spelling doaj-art-b0897cafb3a24da68f5cde10454b983e2025-02-03T05:50:56ZengWileyAdvances in High Energy Physics1687-73571687-73652019-01-01201910.1155/2019/34868053486805Modeling Dark Sector in Horndeski Gravity at First-Order FormalismF. F. Santos0R. M. P. Neves1F. A. Brito2Departamento de Física, Universidade Federal da Paraíba, Caixa Postal 5008, 58051-970 João Pessoa PB, BrazilDepartamento de Física, Universidade Federal da Paraíba, Caixa Postal 5008, 58051-970 João Pessoa PB, BrazilDepartamento de Física, Universidade Federal da Paraíba, Caixa Postal 5008, 58051-970 João Pessoa PB, BrazilWe investigate a cosmological scenario by finding solutions using first-order formalism in the Horndeski gravity that constrains the superpotential and implies that no free choice of scalar potential is allowed. Despite this, we show that a de Sitter phase at late-time cosmology can be realized, where the dark energy sector can be identified. The scalar field equation of state tends to the cosmological scenario at present time and allows us to conclude that it can simulate the dark energy in the Horndeski gravity.http://dx.doi.org/10.1155/2019/3486805
spellingShingle F. F. Santos
R. M. P. Neves
F. A. Brito
Modeling Dark Sector in Horndeski Gravity at First-Order Formalism
Advances in High Energy Physics
title Modeling Dark Sector in Horndeski Gravity at First-Order Formalism
title_full Modeling Dark Sector in Horndeski Gravity at First-Order Formalism
title_fullStr Modeling Dark Sector in Horndeski Gravity at First-Order Formalism
title_full_unstemmed Modeling Dark Sector in Horndeski Gravity at First-Order Formalism
title_short Modeling Dark Sector in Horndeski Gravity at First-Order Formalism
title_sort modeling dark sector in horndeski gravity at first order formalism
url http://dx.doi.org/10.1155/2019/3486805
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AT rmpneves modelingdarksectorinhorndeskigravityatfirstorderformalism
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