HEAL DSpace

Reducing the heterotic supergravity on nearly-Kähler coset spaces

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dc.contributor.author Chatzistavrakidis, A en
dc.contributor.author Manousselis, P en
dc.contributor.author Zoupanos, G en
dc.date.accessioned 2014-03-01T01:31:47Z
dc.date.available 2014-03-01T01:31:47Z
dc.date.issued 2009 en
dc.identifier.issn 0015-8208 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/19922
dc.subject Dimensional reduction en
dc.subject Heterotic supergravity en
dc.subject Nearly-Kähler manifolds en
dc.subject.classification Physics, Multidisciplinary en
dc.subject.other YANG-MILLS THEORY en
dc.subject.other DIMENSIONAL REDUCTION en
dc.subject.other SUPERSTRING THEORIES en
dc.subject.other GAUGE-THEORIES en
dc.subject.other COMPACTIFICATION en
dc.subject.other TORSION en
dc.subject.other CONSISTENCY en
dc.title Reducing the heterotic supergravity on nearly-Kähler coset spaces en
heal.type journalArticle en
heal.identifier.primary 10.1002/prop.200900012 en
heal.identifier.secondary http://dx.doi.org/10.1002/prop.200900012 en
heal.language English en
heal.publicationDate 2009 en
heal.abstract We study the dimensional reduction of the N{script} = 1, ten-dimensional Heterotic Supergravity to four dimensions, at leading order in α′, when the internal space is a nearly-Kähler manifold. Nearly-Kähler manifolds in six dimensions are all the non-symmetric coset spaces and a group manifold. Here we reduce the theory using as internal manifolds the three six-dimensional non-symmetric coset spaces, omitting the case of the group manifold in the prospect of obtaining chiral fermions when the gauge fields will be included. We determine the effective actions for these cases, which turn out to describe N{script} = 1 four-dimensional super-gravities of the no-scale type and we study the various possibilities concerning their vacuum. © 2009 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim. en
heal.publisher WILEY-V C H VERLAG GMBH en
heal.journalName Fortschritte der Physik en
dc.identifier.doi 10.1002/prop.200900012 en
dc.identifier.isi ISI:000267277200023 en
dc.identifier.volume 57 en
dc.identifier.issue 5-7 en
dc.identifier.spage 527 en
dc.identifier.epage 534 en


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