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Flat-brane compactifications in supergravity induced by scalars

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dc.contributor.author Kehagias, A en
dc.contributor.author Mattheopoulou, C en
dc.date.accessioned 2014-03-01T01:28:24Z
dc.date.available 2014-03-01T01:28:24Z
dc.date.issued 2008 en
dc.identifier.issn 0550-3213 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/18843
dc.subject Compactification en
dc.subject Intersecting branes en
dc.subject Modular group en
dc.subject Stringy cosmic strings en
dc.subject Supergravity en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other COSMOLOGICAL CONSTANT PROBLEM en
dc.subject.other NONCOMPACT EXTRA DIMENSIONS en
dc.subject.other N=2 SUPERGRAVITY en
dc.subject.other YANG-MILLS en
dc.subject.other VECTOR MULTIPLETS en
dc.subject.other STRING THEORY en
dc.subject.other SIGMA-MODEL en
dc.subject.other DUALITY en
dc.subject.other COUPLINGS en
dc.subject.other MANIFOLDS en
dc.title Flat-brane compactifications in supergravity induced by scalars en
heal.type journalArticle en
heal.identifier.primary 10.1016/j.nuclphysb.2007.12.027 en
heal.identifier.secondary http://dx.doi.org/10.1016/j.nuclphysb.2007.12.027 en
heal.language English en
heal.publicationDate 2008 en
heal.abstract We discuss flat compactifications of supergravities in diverse dimensions in the presence of branes. The compactification is induced by the scalar fields of supergravity and it is such that there is no relic cosmological constant on the brane, rendering this way the latter flat. We discuss in particular the D = 4, N = 2, 4 and D = 8, N = 1 supergravities with n = 1, 2, 3 vector multiplets where the scalar manifolds are Grassmannian cosets of the form SO (2, n) / SO (2) × SO (n). By introducing branes at certain points in the transverse space, finite energy solutions to the field equations are constructed. Some of the solutions we present may be interpreted as intersecting branes. © 2008 Elsevier B.V. All rights reserved. en
heal.publisher ELSEVIER SCIENCE BV en
heal.journalName Nuclear Physics B en
dc.identifier.doi 10.1016/j.nuclphysb.2007.12.027 en
dc.identifier.isi ISI:000255310000005 en
dc.identifier.volume 797 en
dc.identifier.issue 1-2 en
dc.identifier.spage 117 en
dc.identifier.epage 136 en


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