KK Compactification of Supergravity Models

Detalhes bibliográficos
Autor(a) principal: Năstase, Horaţiu [UNESP]
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_15
http://hdl.handle.net/11449/200480
Resumo: In this chapter, we will study the KK compactification of supergravity models in higher dimensions. Supergravity models in higher dimensions have: -a graviton, described by the metric gμν (which can be written as eμaηabeνb ), except for the coupling to fermions, which is written in terms of ωμab(e). -gravitino(s) (Figure presented.) ψμαi, one for each supersymmetry. Indeed, each supersymmetry ϵi takes us from the graviton to a different gravitino, δeμa=ϵ¯iγaψμi. -other fields: scalars ϕI, vectors AμI, spinors λαI, and also antisymmetric tensors Aμ1..μr. The antisymmetric tensors are generalizations of the gauge fields (Maxwell fields) Aμ, that have also a field strength, (Formula Presented), and so satisfy a gauge invariance (Formula Presented). The gauge invariant action for the antisymmetric tensor field is (Formula Presented).
id UNSP_d71034b1be9f65e07463acc9d4c357ba
oai_identifier_str oai:repositorio.unesp.br:11449/200480
network_acronym_str UNSP
network_name_str Repositório Institucional da UNESP
repository_id_str 2946
spelling KK Compactification of Supergravity ModelsIn this chapter, we will study the KK compactification of supergravity models in higher dimensions. Supergravity models in higher dimensions have: -a graviton, described by the metric gμν (which can be written as eμaηabeνb ), except for the coupling to fermions, which is written in terms of ωμab(e). -gravitino(s) (Figure presented.) ψμαi, one for each supersymmetry. Indeed, each supersymmetry ϵi takes us from the graviton to a different gravitino, δeμa=ϵ¯iγaψμi. -other fields: scalars ϕI, vectors AμI, spinors λαI, and also antisymmetric tensors Aμ1..μr. The antisymmetric tensors are generalizations of the gauge fields (Maxwell fields) Aμ, that have also a field strength, (Formula Presented), and so satisfy a gauge invariance (Formula Presented). The gauge invariant action for the antisymmetric tensor field is (Formula Presented).Instituto de Física Teórica UNESPInstituto de Física Teórica UNESPUniversidade Estadual Paulista (Unesp)Năstase, Horaţiu [UNESP]2020-12-12T02:07:45Z2020-12-12T02:07:45Z2019-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/bookPart181-190http://dx.doi.org/10.1007/978-3-030-15077-8_15Fundamental Theories of Physics, v. 197, p. 181-190.2365-64250168-1222http://hdl.handle.net/11449/20048010.1007/978-3-030-15077-8_152-s2.0-85085195970Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengFundamental Theories of Physicsinfo:eu-repo/semantics/openAccess2021-10-23T14:26:44Zoai:repositorio.unesp.br:11449/200480Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T13:53:02.107578Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv KK Compactification of Supergravity Models
title KK Compactification of Supergravity Models
spellingShingle KK Compactification of Supergravity Models
Năstase, Horaţiu [UNESP]
title_short KK Compactification of Supergravity Models
title_full KK Compactification of Supergravity Models
title_fullStr KK Compactification of Supergravity Models
title_full_unstemmed KK Compactification of Supergravity Models
title_sort KK Compactification of Supergravity Models
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 study the KK compactification of supergravity models in higher dimensions. Supergravity models in higher dimensions have: -a graviton, described by the metric gμν (which can be written as eμaηabeνb ), except for the coupling to fermions, which is written in terms of ωμab(e). -gravitino(s) (Figure presented.) ψμαi, one for each supersymmetry. Indeed, each supersymmetry ϵi takes us from the graviton to a different gravitino, δeμa=ϵ¯iγaψμi. -other fields: scalars ϕI, vectors AμI, spinors λαI, and also antisymmetric tensors Aμ1..μr. The antisymmetric tensors are generalizations of the gauge fields (Maxwell fields) Aμ, that have also a field strength, (Formula Presented), and so satisfy a gauge invariance (Formula Presented). The gauge invariant action for the antisymmetric tensor field is (Formula Presented).
publishDate 2019
dc.date.none.fl_str_mv 2019-01-01
2020-12-12T02:07:45Z
2020-12-12T02:07:45Z
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_15
Fundamental Theories of Physics, v. 197, p. 181-190.
2365-6425
0168-1222
http://hdl.handle.net/11449/200480
10.1007/978-3-030-15077-8_15
2-s2.0-85085195970
url http://dx.doi.org/10.1007/978-3-030-15077-8_15
http://hdl.handle.net/11449/200480
identifier_str_mv Fundamental Theories of Physics, v. 197, p. 181-190.
2365-6425
0168-1222
10.1007/978-3-030-15077-8_15
2-s2.0-85085195970
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 181-190
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_ 1808128286257053696