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dc.contributor.author김성구-
dc.date.accessioned2018-06-02T08:14:36Z-
dc.date.available2018-06-02T08:14:36Z-
dc.date.issued1999-
dc.identifier.issn0556-2821-
dc.identifier.otherOAK-17436-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/244196-
dc.description.abstractWe show that the quantum dynamics of a real scalar field for a large class of potentials in the symmetric Gaussian state, where nonperturbative quantum contributions are taken into account, can be described equivalently by a two-dimensional nonlinear dynamical system with a definite angular momentum [U(1) charge of a complex theory]. A proposal is put forward that the symmetric Gaussian state with a nearly minimal uncertainty and a large quantum fluctuation, as an initial condition, naturally explains most of the essential features of the early stage of the inflationary universe. ©1998 The American Physical Society.-
dc.languageEnglish-
dc.titleQuantum inflaton dynamics-
dc.typeArticle-
dc.relation.issue2-
dc.relation.volume59-
dc.relation.indexSCOPUS-
dc.relation.startpage1-
dc.relation.lastpage4-
dc.relation.journaltitlePhysical Review D - Particles, Fields, Gravitation and Cosmology-
dc.identifier.scopusid2-s2.0-16444366315-
dc.author.googleBak D.-
dc.author.googleKim S.P.-
dc.author.googleKim S.K.-
dc.author.googleSoh K.-S.-
dc.author.googleYee J.H.-
dc.contributor.scopusid김성구(22967145800)-
dc.date.modifydate20180601100402-


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