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dc.contributor.author권오갑-
dc.date.accessioned2016-08-29T12:08:54Z-
dc.date.available2016-08-29T12:08:54Z-
dc.date.issued2015-
dc.identifier.issn1550-7998-
dc.identifier.otherOAK-14678-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/230473-
dc.description.abstractWe consider a deformed single-field inflation model in terms of three SO(3) symmetric moduli fields. We find that spatially linear solutions for the moduli fields induce a phase transition during the early stage of the inflation and the suppression of scalar power spectrum at large scales. This suppression can be an origin of anomalies for large-scale perturbation modes in the cosmological observation. © 2015 American Physical Society.-
dc.languageEnglish-
dc.publisherAmerican Physical Society-
dc.titleLarge scale suppression of scalar power on a spatial condensation-
dc.typeArticle-
dc.relation.issue6-
dc.relation.volume91-
dc.relation.indexSCI-
dc.relation.indexSCIE-
dc.relation.indexSCOPUS-
dc.relation.journaltitlePhysical Review D - Particles, Fields, Gravitation and Cosmology-
dc.identifier.doi10.1103/PhysRevD.91.063521-
dc.identifier.wosidWOS:000351428400003-
dc.identifier.scopusid2-s2.0-84927627842-
dc.author.googleKouwn S.-
dc.author.googleKwon O.-K.-
dc.author.googleOh P.-
dc.contributor.scopusid권오갑(27172330000)-
dc.date.modifydate20220915161534-


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