Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 권오갑 | - |
dc.date.accessioned | 2016-08-29T12:08:54Z | - |
dc.date.available | 2016-08-29T12:08:54Z | - |
dc.date.issued | 2015 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.other | OAK-14678 | - |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/230473 | - |
dc.description.abstract | We 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.language | English | - |
dc.publisher | American Physical Society | - |
dc.title | Large scale suppression of scalar power on a spatial condensation | - |
dc.type | Article | - |
dc.relation.issue | 6 | - |
dc.relation.volume | 91 | - |
dc.relation.index | SCI | - |
dc.relation.index | SCIE | - |
dc.relation.index | SCOPUS | - |
dc.relation.journaltitle | Physical Review D - Particles, Fields, Gravitation and Cosmology | - |
dc.identifier.doi | 10.1103/PhysRevD.91.063521 | - |
dc.identifier.wosid | WOS:000351428400003 | - |
dc.identifier.scopusid | 2-s2.0-84927627842 | - |
dc.author.google | Kouwn S. | - |
dc.author.google | Kwon O.-K. | - |
dc.author.google | Oh P. | - |
dc.contributor.scopusid | 권오갑(27172330000) | - |
dc.date.modifydate | 20220915161534 | - |