Coupled quintessence with a generalized interaction term

Detalhes bibliográficos
Autor(a) principal: Potting, Robertus
Data de Publicação: 2022
Outros Autores: Sá, Paulo
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10400.1/18798
Resumo: We investigate a cosmological model in which dark energy, represented by a quintessential scalar field, is directly coupled to a dark-matter perfect fluid. We are interested in solutions of cosmological relevance, namely those for which a dark-matter-dominated era long enough to allow for structure formation is followed by an era of accelerated expansion driven by dark energy. For the coupling between these two dark components of the Universe, we choose forms that generalize the one most commonly used in the literature. Resorting to powerful methods of qualitative analysis of dynamical systems, we show that, for certain generalized forms of the coupling, final states of our coupled quintessential model correspond to solutions in which the evolution of the Universe is completely dominated by dark energy. In this case, there are no scaling solutions. Interestingly, however, for certain values of a relevant parameter, during the approach to the final state of evolution, the cosmological parameters change so slowly that, for all practical purposes, the solution appears to be stuck in a state corresponding to a scaling solution.
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spelling Coupled quintessence with a generalized interaction termDark energyDark matterCosmological evolutionWe investigate a cosmological model in which dark energy, represented by a quintessential scalar field, is directly coupled to a dark-matter perfect fluid. We are interested in solutions of cosmological relevance, namely those for which a dark-matter-dominated era long enough to allow for structure formation is followed by an era of accelerated expansion driven by dark energy. For the coupling between these two dark components of the Universe, we choose forms that generalize the one most commonly used in the literature. Resorting to powerful methods of qualitative analysis of dynamical systems, we show that, for certain generalized forms of the coupling, final states of our coupled quintessential model correspond to solutions in which the evolution of the Universe is completely dominated by dark energy. In this case, there are no scaling solutions. Interestingly, however, for certain values of a relevant parameter, during the approach to the final state of evolution, the cosmological parameters change so slowly that, for all practical purposes, the solution appears to be stuck in a state corresponding to a scaling solution.World ScientificSapientiaPotting, RobertusSá, Paulo2023-05-17T00:30:12Z2022-05-172022-05-17T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10400.1/18798eng10.1142/S02182718225011151793-6594info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2023-07-24T10:31:09Zoai:sapientia.ualg.pt:10400.1/18798Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-19T20:08:31.672472Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv Coupled quintessence with a generalized interaction term
title Coupled quintessence with a generalized interaction term
spellingShingle Coupled quintessence with a generalized interaction term
Potting, Robertus
Dark energy
Dark matter
Cosmological evolution
title_short Coupled quintessence with a generalized interaction term
title_full Coupled quintessence with a generalized interaction term
title_fullStr Coupled quintessence with a generalized interaction term
title_full_unstemmed Coupled quintessence with a generalized interaction term
title_sort Coupled quintessence with a generalized interaction term
author Potting, Robertus
author_facet Potting, Robertus
Sá, Paulo
author_role author
author2 Sá, Paulo
author2_role author
dc.contributor.none.fl_str_mv Sapientia
dc.contributor.author.fl_str_mv Potting, Robertus
Sá, Paulo
dc.subject.por.fl_str_mv Dark energy
Dark matter
Cosmological evolution
topic Dark energy
Dark matter
Cosmological evolution
description We investigate a cosmological model in which dark energy, represented by a quintessential scalar field, is directly coupled to a dark-matter perfect fluid. We are interested in solutions of cosmological relevance, namely those for which a dark-matter-dominated era long enough to allow for structure formation is followed by an era of accelerated expansion driven by dark energy. For the coupling between these two dark components of the Universe, we choose forms that generalize the one most commonly used in the literature. Resorting to powerful methods of qualitative analysis of dynamical systems, we show that, for certain generalized forms of the coupling, final states of our coupled quintessential model correspond to solutions in which the evolution of the Universe is completely dominated by dark energy. In this case, there are no scaling solutions. Interestingly, however, for certain values of a relevant parameter, during the approach to the final state of evolution, the cosmological parameters change so slowly that, for all practical purposes, the solution appears to be stuck in a state corresponding to a scaling solution.
publishDate 2022
dc.date.none.fl_str_mv 2022-05-17
2022-05-17T00:00:00Z
2023-05-17T00:30:12Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10400.1/18798
url http://hdl.handle.net/10400.1/18798
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 10.1142/S0218271822501115
1793-6594
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dc.publisher.none.fl_str_mv World Scientific
publisher.none.fl_str_mv World Scientific
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