Inflation in non-minimal matter-curvature coupling theories

Bibliographic Details
Main Author: Rosa, João Pedro Trancoso Gomes
Publication Date: 2017
Other Authors: Gomes, Cláudio, Bertolami, Orfeu
Format: Article
Language: eng
Source: Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)
Download full: http://hdl.handle.net/10773/18248
Summary: We study inflationary scenarios driven by a scalar field in the presence of a non-minimal coupling between matter and curvature. We show that the Friedmann equation can be significantly modified when the energy density during inflation exceeds a critical value determined by the non-minimal coupling, which in turn may considerably modify the spectrum of primordial perturbations and the inflationary dynamics. In particular, we show that these models are characterised by a consistency relation between the tensor-to-scalar ratio and the tensor spectral index that can differ significantly from the predictions of general relativity. We also give examples of observational predictions for some of the most commonly considered potentials and use the results of the Planck collaboration to set limits on the scale of the non-minimal coupling.
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spelling Inflation in non-minimal matter-curvature coupling theoriesInflationModified gravityWe study inflationary scenarios driven by a scalar field in the presence of a non-minimal coupling between matter and curvature. We show that the Friedmann equation can be significantly modified when the energy density during inflation exceeds a critical value determined by the non-minimal coupling, which in turn may considerably modify the spectrum of primordial perturbations and the inflationary dynamics. In particular, we show that these models are characterised by a consistency relation between the tensor-to-scalar ratio and the tensor spectral index that can differ significantly from the predictions of general relativity. We also give examples of observational predictions for some of the most commonly considered potentials and use the results of the Planck collaboration to set limits on the scale of the non-minimal coupling.IOP Publishing2017-08-29T10:36:26Z2017-01-01T00:00:00Z2017info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/18248eng1475-751610.1088/1475-7516/2017/06/021Rosa, João Pedro Trancoso GomesGomes, CláudioBertolami, Orfeuinfo:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2024-05-06T04:02:06Zoai:ria.ua.pt:10773/18248Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-28T13:55:05.110172Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse
dc.title.none.fl_str_mv Inflation in non-minimal matter-curvature coupling theories
title Inflation in non-minimal matter-curvature coupling theories
spellingShingle Inflation in non-minimal matter-curvature coupling theories
Rosa, João Pedro Trancoso Gomes
Inflation
Modified gravity
title_short Inflation in non-minimal matter-curvature coupling theories
title_full Inflation in non-minimal matter-curvature coupling theories
title_fullStr Inflation in non-minimal matter-curvature coupling theories
title_full_unstemmed Inflation in non-minimal matter-curvature coupling theories
title_sort Inflation in non-minimal matter-curvature coupling theories
author Rosa, João Pedro Trancoso Gomes
author_facet Rosa, João Pedro Trancoso Gomes
Gomes, Cláudio
Bertolami, Orfeu
author_role author
author2 Gomes, Cláudio
Bertolami, Orfeu
author2_role author
author
dc.contributor.author.fl_str_mv Rosa, João Pedro Trancoso Gomes
Gomes, Cláudio
Bertolami, Orfeu
dc.subject.por.fl_str_mv Inflation
Modified gravity
topic Inflation
Modified gravity
description We study inflationary scenarios driven by a scalar field in the presence of a non-minimal coupling between matter and curvature. We show that the Friedmann equation can be significantly modified when the energy density during inflation exceeds a critical value determined by the non-minimal coupling, which in turn may considerably modify the spectrum of primordial perturbations and the inflationary dynamics. In particular, we show that these models are characterised by a consistency relation between the tensor-to-scalar ratio and the tensor spectral index that can differ significantly from the predictions of general relativity. We also give examples of observational predictions for some of the most commonly considered potentials and use the results of the Planck collaboration to set limits on the scale of the non-minimal coupling.
publishDate 2017
dc.date.none.fl_str_mv 2017-08-29T10:36:26Z
2017-01-01T00:00:00Z
2017
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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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10773/18248
url http://hdl.handle.net/10773/18248
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 1475-7516
10.1088/1475-7516/2017/06/021
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.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)
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