Problems of the Supergravity Approximation to String Inflation
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Tipo de documento: | Capítulo de livro |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UNESP |
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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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]2020-12-12T02:08:16Z2020-12-12T02:08:16Z2019-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/bookPart299-309http://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 UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengFundamental Theories of Physicsinfo:eu-repo/semantics/openAccess2021-10-23T14:33:33Zoai:repositorio.unesp.br:11449/200501Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T21:20:11.767637Repositório Institucional da UNESP - 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.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/bookPart |
format |
bookPart |
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 instname:Universidade Estadual Paulista (UNESP) instacron:UNESP |
instname_str |
Universidade Estadual Paulista (UNESP) |
instacron_str |
UNESP |
institution |
UNESP |
reponame_str |
Repositório Institucional da UNESP |
collection |
Repositório Institucional da UNESP |
repository.name.fl_str_mv |
Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP) |
repository.mail.fl_str_mv |
|
_version_ |
1808129310382358528 |