Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 김성구 | - |
dc.date.accessioned | 2016-08-28T11:08:23Z | - |
dc.date.available | 2016-08-28T11:08:23Z | - |
dc.date.issued | 1988 | - |
dc.identifier.issn | 0556-2821 | - |
dc.identifier.other | OAK-12776 | - |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/228850 | - |
dc.description.abstract | The effective potential for a scalar theory in the static Einstein universe is calculated using the Gaussian approximation in a field-theoretic Schrödinger picture. There occurs an infrared divergence in the slope of the effective potential at the would-be symmetry-breaking minimum and the effective potential is complex in a region including this would-be minimum. Spontaneous symmetry breaking, therefore, cannot occur in the static Einstein universe. © 1988 The American Physical Society. | - |
dc.language | English | - |
dc.title | Symmetry behavior in the Einstein universe: Gaussian approximation in the Schrödinger picture | - |
dc.type | Article | - |
dc.relation.issue | 6 | - |
dc.relation.volume | 38 | - |
dc.relation.index | SCOPUS | - |
dc.relation.startpage | 1853 | - |
dc.relation.lastpage | 1858 | - |
dc.relation.journaltitle | Physical Review D | - |
dc.identifier.doi | 10.1103/PhysRevD.38.1853 | - |
dc.identifier.scopusid | 2-s2.0-24244454611 | - |
dc.author.google | Kim S.K. | - |
dc.author.google | Namgung W. | - |
dc.author.google | Soh K.S. | - |
dc.author.google | Yee J.H. | - |
dc.contributor.scopusid | 김성구(22967145800) | - |
dc.date.modifydate | 20180104081001 | - |