Brane (-Antibrane) 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_26 http://hdl.handle.net/11449/200475 |
Resumo: | In this chapter we will examine the possibility that we have inflation due to branes, or perhaps a brane-antibrane system. In string theory, we have branes as we saw, in particular Dp-branes. They move in a higher dimensional space (usually 10 dimensions), and then from the point of view of their worldvolume, the positions in the extra dimensions behave as scalars. If moreover we adopt a point of view that our 3+1 dimensional world lives on the worldvolume of these branes (a scenario known as “braneworld”), then the extra dimensions are 3+1 dimensional scalars. It is therefore natural to ask whether one of them, X(ξa), can be the inflaton. |
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Brane (-Antibrane) InflationIn this chapter we will examine the possibility that we have inflation due to branes, or perhaps a brane-antibrane system. In string theory, we have branes as we saw, in particular Dp-branes. They move in a higher dimensional space (usually 10 dimensions), and then from the point of view of their worldvolume, the positions in the extra dimensions behave as scalars. If moreover we adopt a point of view that our 3+1 dimensional world lives on the worldvolume of these branes (a scenario known as “braneworld”), then the extra dimensions are 3+1 dimensional scalars. It is therefore natural to ask whether one of them, X(ξa), can be the inflaton.Instituto de Física Teórica UNESPInstituto de Física Teórica UNESPUniversidade Estadual Paulista (Unesp)Năstase, Horaţiu [UNESP]2020-12-12T02:07:38Z2020-12-12T02:07:38Z2019-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/bookPart311-320http://dx.doi.org/10.1007/978-3-030-15077-8_26Fundamental Theories of Physics, v. 197, p. 311-320.2365-64250168-1222http://hdl.handle.net/11449/20047510.1007/978-3-030-15077-8_262-s2.0-85085190635Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengFundamental Theories of Physicsinfo:eu-repo/semantics/openAccess2021-10-23T14:26:36Zoai:repositorio.unesp.br:11449/200475Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T15:37:35.703142Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false |
dc.title.none.fl_str_mv |
Brane (-Antibrane) Inflation |
title |
Brane (-Antibrane) Inflation |
spellingShingle |
Brane (-Antibrane) Inflation Năstase, Horaţiu [UNESP] |
title_short |
Brane (-Antibrane) Inflation |
title_full |
Brane (-Antibrane) Inflation |
title_fullStr |
Brane (-Antibrane) Inflation |
title_full_unstemmed |
Brane (-Antibrane) Inflation |
title_sort |
Brane (-Antibrane) 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 |
In this chapter we will examine the possibility that we have inflation due to branes, or perhaps a brane-antibrane system. In string theory, we have branes as we saw, in particular Dp-branes. They move in a higher dimensional space (usually 10 dimensions), and then from the point of view of their worldvolume, the positions in the extra dimensions behave as scalars. If moreover we adopt a point of view that our 3+1 dimensional world lives on the worldvolume of these branes (a scenario known as “braneworld”), then the extra dimensions are 3+1 dimensional scalars. It is therefore natural to ask whether one of them, X(ξa), can be the inflaton. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-01-01 2020-12-12T02:07:38Z 2020-12-12T02:07:38Z |
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_26 Fundamental Theories of Physics, v. 197, p. 311-320. 2365-6425 0168-1222 http://hdl.handle.net/11449/200475 10.1007/978-3-030-15077-8_26 2-s2.0-85085190635 |
url |
http://dx.doi.org/10.1007/978-3-030-15077-8_26 http://hdl.handle.net/11449/200475 |
identifier_str_mv |
Fundamental Theories of Physics, v. 197, p. 311-320. 2365-6425 0168-1222 10.1007/978-3-030-15077-8_26 2-s2.0-85085190635 |
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 |
311-320 |
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_ |
1808128541166927872 |