Non-slow-roll dynamics in α-attractors

Detalhes bibliográficos
Autor(a) principal: Kumar, K. Sravan
Data de Publicação: 2016
Outros Autores: Marto, João, Moniz, Paulo, Das, Suratna
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10400.6/6501
Resumo: In this paper we consider the α−attractor model and study inflation under a non-slow-roll dynamics. More precisely, we follow the approach recently proposed by Gong and Sasaki [1] by means of assuming N=N(phi). Within this framework we obtain a family of functions describing the local shape of the potential during inflation. We study a specific model and find an inflationary scenario predicting an attractor at ns≈0.967 and r≈5.5×10^(−4). We further show that considering a non-slow-roll dynamics, the α−attractor model can be broaden to a wider class of models that remain compatible with value of r<0.1. We further explore the model parameter space with respect to large and small field inflation and conclude that the inflaton dynamics is connected to the α− parameter, which is also related to the Kähler manifold curvature in the supergravity (SUGRA) embedding of this model. We also comment on the stabilization of the inflaton's trajectory.
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spelling Non-slow-roll dynamics in α-attractorsInflationIn this paper we consider the α−attractor model and study inflation under a non-slow-roll dynamics. More precisely, we follow the approach recently proposed by Gong and Sasaki [1] by means of assuming N=N(phi). Within this framework we obtain a family of functions describing the local shape of the potential during inflation. We study a specific model and find an inflationary scenario predicting an attractor at ns≈0.967 and r≈5.5×10^(−4). We further show that considering a non-slow-roll dynamics, the α−attractor model can be broaden to a wider class of models that remain compatible with value of r<0.1. We further explore the model parameter space with respect to large and small field inflation and conclude that the inflaton dynamics is connected to the α− parameter, which is also related to the Kähler manifold curvature in the supergravity (SUGRA) embedding of this model. We also comment on the stabilization of the inflaton's trajectory.IOP PublishinguBibliorumKumar, K. SravanMarto, JoãoMoniz, PauloDas, Suratna2018-11-26T16:08:49Z20162016-01-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10400.6/6501engK. Sravan Kumar et al JCAP04(2016)00510.1088/1475-7516/2016/04/005metadata only accessinfo: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:RCAAP2023-12-15T09:45:01Zoai:ubibliorum.ubi.pt:10400.6/6501Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T00:47:12.787955Repositório 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 Non-slow-roll dynamics in α-attractors
title Non-slow-roll dynamics in α-attractors
spellingShingle Non-slow-roll dynamics in α-attractors
Kumar, K. Sravan
Inflation
title_short Non-slow-roll dynamics in α-attractors
title_full Non-slow-roll dynamics in α-attractors
title_fullStr Non-slow-roll dynamics in α-attractors
title_full_unstemmed Non-slow-roll dynamics in α-attractors
title_sort Non-slow-roll dynamics in α-attractors
author Kumar, K. Sravan
author_facet Kumar, K. Sravan
Marto, João
Moniz, Paulo
Das, Suratna
author_role author
author2 Marto, João
Moniz, Paulo
Das, Suratna
author2_role author
author
author
dc.contributor.none.fl_str_mv uBibliorum
dc.contributor.author.fl_str_mv Kumar, K. Sravan
Marto, João
Moniz, Paulo
Das, Suratna
dc.subject.por.fl_str_mv Inflation
topic Inflation
description In this paper we consider the α−attractor model and study inflation under a non-slow-roll dynamics. More precisely, we follow the approach recently proposed by Gong and Sasaki [1] by means of assuming N=N(phi). Within this framework we obtain a family of functions describing the local shape of the potential during inflation. We study a specific model and find an inflationary scenario predicting an attractor at ns≈0.967 and r≈5.5×10^(−4). We further show that considering a non-slow-roll dynamics, the α−attractor model can be broaden to a wider class of models that remain compatible with value of r<0.1. We further explore the model parameter space with respect to large and small field inflation and conclude that the inflaton dynamics is connected to the α− parameter, which is also related to the Kähler manifold curvature in the supergravity (SUGRA) embedding of this model. We also comment on the stabilization of the inflaton's trajectory.
publishDate 2016
dc.date.none.fl_str_mv 2016
2016-01-01T00:00:00Z
2018-11-26T16:08:49Z
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dc.relation.none.fl_str_mv K. Sravan Kumar et al JCAP04(2016)005
10.1088/1475-7516/2016/04/005
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