Next-to-leading-order power correction to photon-pion transition form factor
| dc.citation.epage | 0 | en_US |
| dc.citation.issue | 1 | en_US |
| dc.citation.spage | 0 | en_US |
| dc.citation.volume | 66 | en_US |
| dc.citation.woscount | 4 | en_US |
| dc.contributor.author | Yeh, TW | en_US |
| dc.contributor.department | 物理研究所 | zh_TW |
| dc.contributor.department | Institute of Physics | en_US |
| dc.date.accessioned | 2019-04-03T06:39:52Z | |
| dc.date.available | 2019-04-03T06:39:52Z | |
| dc.date.issued | 2002-07-01 | en_US |
| dc.description.abstract | We propose an approach to calculate the next-to-leading-order power corrections to the photon-pion transition form factor F-pigamma(Q(2)). The effects of the next-to-leading-order power corrections are analyzed. | en_US |
| dc.identifier.doi | 10.1103/PhysRevD.66.014002 | en_US |
| dc.identifier.issn | 2470-0010 | en_US |
| dc.identifier.journal | PHYSICAL REVIEW D | en_US |
| dc.identifier.uri | http://dx.doi.org/10.1103/PhysRevD.66.014002 | en_US |
| dc.identifier.uri | https://ir.lib.nycu.edu.tw/handle/11536/28700 | |
| dc.identifier.wosnumber | WOS:000177338600024 | en_US |
| dc.language.iso | en_US | en_US |
| dc.title | Next-to-leading-order power correction to photon-pion transition form factor | en_US |
| dc.type | Article | en_US |