Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 공진욱 | * |
dc.date.accessioned | 2022-02-21T16:30:08Z | - |
dc.date.available | 2022-02-21T16:30:08Z | - |
dc.date.issued | 2022 | * |
dc.identifier.issn | 1475-7516 | * |
dc.identifier.other | OAK-30929 | * |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/260512 | - |
dc.description.abstract | We 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.language | English | * |
dc.publisher | IOP Publishing Ltd | * |
dc.subject | cosmological perturbation theory | * |
dc.subject | inflation | * |
dc.subject | physics of the early universe | * |
dc.title | Potential reconstruction from general power spectrum in single-field inflation | * |
dc.type | Article | * |
dc.relation.issue | 1 | * |
dc.relation.index | SCIE | * |
dc.relation.index | SCOPUS | * |
dc.relation.journaltitle | JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | * |
dc.identifier.doi | 10.1088/1475-7516/2022/01/012 | * |
dc.identifier.wosid | WOS:000740821300001 | * |
dc.identifier.scopusid | 2-s2.0-85123682520 | * |
dc.author.google | Choi, Ki-Young | * |
dc.author.google | Gong, Jinn-Ouk | * |
dc.author.google | Kang, Su-beom | * |
dc.author.google | Raveendran, Rathul Nath | * |
dc.contributor.scopusid | 공진욱(7402707824) | * |
dc.date.modifydate | 20231214113754 | * |