Problems of the Supergravity Approximation to String Inflation

Detalhes bibliográficos
Autor(a) principal: Năstase, Horaţiu [UNESP]
Data de Publicação: 2019
Tipo de documento: Conjunto de dados
Idioma: eng
Título da fonte: Repositório Institucional da UNESP (dados de pesquisa)
Texto Completo: http://dx.doi.org/10.1007/978-3-030-15077-8_25
http://hdl.handle.net/11449/200501
Resumo: Because string theory itself is not very calculable, there are few truly stringy models of cosmology. Therefore, one mostly considers the low energy limit of string theory, supergravity, as an effective field theory, and in this chapter we want to note the problems we encounter when we try to obtain inflation in this effective field theory. As usual, for phenomenological reasons we only consider N= 1 supersymmetry, considering that the rest has been lost at a high scale. In N= 1 supersymmetry, besides the supergravity multiplet, we have the chiral multiplet Φ and the vector multiplet Va.
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spelling Problems of the Supergravity Approximation to String InflationBecause string theory itself is not very calculable, there are few truly stringy models of cosmology. Therefore, one mostly considers the low energy limit of string theory, supergravity, as an effective field theory, and in this chapter we want to note the problems we encounter when we try to obtain inflation in this effective field theory. As usual, for phenomenological reasons we only consider N= 1 supersymmetry, considering that the rest has been lost at a high scale. In N= 1 supersymmetry, besides the supergravity multiplet, we have the chiral multiplet Φ and the vector multiplet Va.Instituto de Física Teórica UNESPInstituto de Física Teórica UNESPUniversidade Estadual Paulista (Unesp)Năstase, Horaţiu [UNESP]2020-12-12T02:08:16Z2020-12-12T02:08:16Z2019-01-01Capítulo de livroinfo:eu-repo/semantics/datasetinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/dataset299-309http://dx.doi.org/10.1007/978-3-030-15077-8_25Fundamental Theories of Physics, v. 197, p. 299-309.2365-64250168-1222http://hdl.handle.net/11449/20050110.1007/978-3-030-15077-8_252-s2.0-85085218808Scopusreponame:Repositório Institucional da UNESP (dados de pesquisa)instname:Universidade Estadual Paulista (UNESP)instacron:UNSPengFundamental Theories of Physicsinfo:eu-repo/semantics/openAccess2021-10-23T14:33:33Zoai:repositorio.unesp.br:11449/200501Repositório de Dados de PesquisaPUBhttp://repositorio.unesp.br/oai/requestrepositoriounesp@unesp.bropendoar:2021-10-23T14:33:33Repositório Institucional da UNESP (dados de pesquisa) - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Problems of the Supergravity Approximation to String Inflation
title Problems of the Supergravity Approximation to String Inflation
spellingShingle Problems of the Supergravity Approximation to String Inflation
Năstase, Horaţiu [UNESP]
title_short Problems of the Supergravity Approximation to String Inflation
title_full Problems of the Supergravity Approximation to String Inflation
title_fullStr Problems of the Supergravity Approximation to String Inflation
title_full_unstemmed Problems of the Supergravity Approximation to String Inflation
title_sort Problems of the Supergravity Approximation to String Inflation
author Năstase, Horaţiu [UNESP]
author_facet Năstase, Horaţiu [UNESP]
author_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (Unesp)
dc.contributor.author.fl_str_mv Năstase, Horaţiu [UNESP]
description Because string theory itself is not very calculable, there are few truly stringy models of cosmology. Therefore, one mostly considers the low energy limit of string theory, supergravity, as an effective field theory, and in this chapter we want to note the problems we encounter when we try to obtain inflation in this effective field theory. As usual, for phenomenological reasons we only consider N= 1 supersymmetry, considering that the rest has been lost at a high scale. In N= 1 supersymmetry, besides the supergravity multiplet, we have the chiral multiplet Φ and the vector multiplet Va.
publishDate 2019
dc.date.none.fl_str_mv 2019-01-01
2020-12-12T02:08:16Z
2020-12-12T02:08:16Z
dc.type.driver.fl_str_mv Capítulo de livro
info:eu-repo/semantics/dataset
info:eu-repo/semantics/publishedVersion
dc.type.driver.none.fl_str_mv info:eu-repo/semantics/dataset
format dataset
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1007/978-3-030-15077-8_25
Fundamental Theories of Physics, v. 197, p. 299-309.
2365-6425
0168-1222
http://hdl.handle.net/11449/200501
10.1007/978-3-030-15077-8_25
2-s2.0-85085218808
url http://dx.doi.org/10.1007/978-3-030-15077-8_25
http://hdl.handle.net/11449/200501
identifier_str_mv Fundamental Theories of Physics, v. 197, p. 299-309.
2365-6425
0168-1222
10.1007/978-3-030-15077-8_25
2-s2.0-85085218808
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Fundamental Theories of Physics
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 299-309
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP (dados de pesquisa)
instname:Universidade Estadual Paulista (UNESP)
instacron:UNSP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNSP
institution UNSP
reponame_str Repositório Institucional da UNESP (dados de pesquisa)
collection Repositório Institucional da UNESP (dados de pesquisa)
repository.name.fl_str_mv Repositório Institucional da UNESP (dados de pesquisa) - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv repositoriounesp@unesp.br
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