KK Compactification of Supergravity Models
dc.contributor.author | Năstase, Horaţiu [UNESP] | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.date.accessioned | 2020-12-12T02:07:45Z | |
dc.date.available | 2020-12-12T02:07:45Z | |
dc.date.issued | 2019-01-01 | |
dc.description.abstract | 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). | en |
dc.description.affiliation | Instituto de Física Teórica UNESP | |
dc.description.affiliationUnesp | Instituto de Física Teórica UNESP | |
dc.format.extent | 181-190 | |
dc.identifier | http://dx.doi.org/10.1007/978-3-030-15077-8_15 | |
dc.identifier.citation | Fundamental Theories of Physics, v. 197, p. 181-190. | |
dc.identifier.doi | 10.1007/978-3-030-15077-8_15 | |
dc.identifier.issn | 2365-6425 | |
dc.identifier.issn | 0168-1222 | |
dc.identifier.scopus | 2-s2.0-85085195970 | |
dc.identifier.uri | http://hdl.handle.net/11449/200480 | |
dc.language.iso | eng | |
dc.relation.ispartof | Fundamental Theories of Physics | |
dc.source | Scopus | |
dc.title | KK Compactification of Supergravity Models | en |
dc.type | Capítulo de livro | |
unesp.campus | Universidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulo | pt |