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KK Compactification of Supergravity Models

dc.contributor.authorNăstase, Horaţiu [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2020-12-12T02:07:45Z
dc.date.available2020-12-12T02:07:45Z
dc.date.issued2019-01-01
dc.description.abstractIn 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).en
dc.description.affiliationInstituto de Física Teórica UNESP
dc.description.affiliationUnespInstituto de Física Teórica UNESP
dc.format.extent181-190
dc.identifierhttp://dx.doi.org/10.1007/978-3-030-15077-8_15
dc.identifier.citationFundamental Theories of Physics, v. 197, p. 181-190.
dc.identifier.doi10.1007/978-3-030-15077-8_15
dc.identifier.issn2365-6425
dc.identifier.issn0168-1222
dc.identifier.scopus2-s2.0-85085195970
dc.identifier.urihttp://hdl.handle.net/11449/200480
dc.language.isoeng
dc.relation.ispartofFundamental Theories of Physics
dc.sourceScopus
dc.titleKK Compactification of Supergravity Modelsen
dc.typeCapítulo de livro
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulopt

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