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Towards realistic standard model from D-brane configurations

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dc.contributor.author Leontaris, GK en
dc.contributor.author Tracas, ND en
dc.contributor.author Vlachos, ND en
dc.contributor.author Korakianitis, O en
dc.date.accessioned 2014-03-01T01:27:29Z
dc.date.available 2014-03-01T01:27:29Z
dc.date.issued 2007 en
dc.identifier.issn 1550-7998 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/18473
dc.subject Change Process en
dc.subject Effective Field Theory en
dc.subject Gauge Symmetry en
dc.subject Low Energy en
dc.subject Renormalization Group en
dc.subject Spectrum en
dc.subject Standard Model en
dc.subject.classification Astronomy & Astrophysics en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other LEPTON-FLAVOR VIOLATION en
dc.subject.other SUPERSYMMETRY en
dc.subject.other ORIENTIFOLDS en
dc.subject.other COSMOLOGY en
dc.subject.other GRAVITY en
dc.title Towards realistic standard model from D-brane configurations en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevD.76.115009 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevD.76.115009 en
heal.identifier.secondary 115009 en
heal.language English en
heal.publicationDate 2007 en
heal.abstract Effective low energy models arising in the context of D-brane configurations with standard model (SM) gauge symmetry extended by several gauged Abelian factors are discussed. The models are classified according to their hypercharge embeddings consistent with the SM spectrum hypercharge assignment. Particular cases are analyzed according to their perspectives and viability as low energy effective field theory candidates. The resulting string scale is determined by means of a two-loop renormalization group calculation. Their implications in Yukawa couplings, neutrinos and flavor changing processes are also presented. © 2007 The American Physical Society. en
heal.publisher AMER PHYSICAL SOC en
heal.journalName Physical Review D - Particles, Fields, Gravitation and Cosmology en
dc.identifier.doi 10.1103/PhysRevD.76.115009 en
dc.identifier.isi ISI:000251987200059 en
dc.identifier.volume 76 en
dc.identifier.issue 11 en


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