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dc.contributor.author공진욱*
dc.date.accessioned2022-02-21T16:30:08Z-
dc.date.available2022-02-21T16:30:08Z-
dc.date.issued2022*
dc.identifier.issn1475-7516*
dc.identifier.otherOAK-30929*
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/260512-
dc.description.abstractWe suggest a new method to reconstruct, within canonical single-field inflation, the inflaton potential directly from the primordial power spectrum which may deviate significantly from near scale-invariance. Our approach relies on a more generalized slow-roll approximation than the standard one, and can probe the properties of the inflaton potential reliably. We give a few examples for reconstructing potential and discuss the validity of our method.*
dc.languageEnglish*
dc.publisherIOP Publishing Ltd*
dc.subjectcosmological perturbation theory*
dc.subjectinflation*
dc.subjectphysics of the early universe*
dc.titlePotential reconstruction from general power spectrum in single-field inflation*
dc.typeArticle*
dc.relation.issue1*
dc.relation.indexSCIE*
dc.relation.indexSCOPUS*
dc.relation.journaltitleJOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS*
dc.identifier.doi10.1088/1475-7516/2022/01/012*
dc.identifier.wosidWOS:000740821300001*
dc.identifier.scopusid2-s2.0-85123682520*
dc.author.googleChoi, Ki-Young*
dc.author.googleGong, Jinn-Ouk*
dc.author.googleKang, Su-beom*
dc.author.googleRaveendran, Rathul Nath*
dc.contributor.scopusid공진욱(7402707824)*
dc.date.modifydate20231214113754*
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사범대학 > 과학교육과 > Journal papers
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