Direct measurement of the astrophysical reaction O-14(alpha,p)F-17
DC Field | Value | Language |
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dc.contributor.author | Notani, M. | - |
dc.contributor.author | Kubono, S. | - |
dc.contributor.author | Teranishi, T. | - |
dc.contributor.author | Yanagisawa, Y. | - |
dc.contributor.author | Michimasa, S. | - |
dc.contributor.author | Ue, K. | - |
dc.contributor.author | He, J.J. | - |
dc.contributor.author | Iwasaki, H. | - |
dc.contributor.author | Baba, H. | - |
dc.contributor.author | Tamaki, M. | - |
dc.contributor.author | Minemura, T. | - |
dc.contributor.author | Shimoura, S. | - |
dc.contributor.author | Hokoiwa, N. | - |
dc.contributor.author | Wakabayashi, Y. | - |
dc.contributor.author | Sasaki, T. | - |
dc.contributor.author | Fukuchi, T. | - |
dc.contributor.author | Odahara, A. | - |
dc.contributor.author | Gono, Y. | - |
dc.contributor.author | Fulop, Z. | - |
dc.contributor.author | Lee, E.K. | - |
dc.contributor.author | Hahn, K.I. | - |
dc.contributor.author | Moon, J.Y. | - |
dc.contributor.author | Yun, C.C. | - |
dc.contributor.author | Lee, J.H. | - |
dc.contributor.author | Lee, Chun Sik | - |
dc.contributor.author | Kato, S. | - |
dc.date.accessioned | 2022-01-10T03:41:17Z | - |
dc.date.available | 2022-01-10T03:41:17Z | - |
dc.date.issued | 2004-06 | - |
dc.identifier.issn | 0375-9474 | - |
dc.identifier.issn | 1873-1554 | - |
dc.identifier.uri | https://scholarworks.bwise.kr/cau/handle/2019.sw.cau/53092 | - |
dc.description.abstract | The stellar reaction O-14(alpha,p)F-17, that critically determines the onset of the high-temperature rp-process, has been studied through a direct measurement with a low-energy radioactive O-14 beam and a gaseous helium target cooled down to 30 K. The reaction cross section was measured directly by means of a thick target technique in the energy range of Ec.m.(O-14+alpha) = 0.8-3.8 MeV. The O-14(alpha,p)F-17* reaction leading to the first excited state in F-17 was clearly observed for the first time, suggesting an increase of about 50% for the stellar reaction rate through resonances at around 7.1 MeV in Ne-18. | - |
dc.format.extent | 5 | - |
dc.language | 영어 | - |
dc.language.iso | ENG | - |
dc.publisher | ELSEVIER SCIENCE BV | - |
dc.title | Direct measurement of the astrophysical reaction O-14(alpha,p)F-17 | - |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.nuclphysa.2004.04.076 | - |
dc.identifier.bibliographicCitation | NUCLEAR PHYSICS A, v.738, no.1-4 SUPPL., pp 411 - 415 | - |
dc.description.isOpenAccess | N | - |
dc.identifier.wosid | 000222479600076 | - |
dc.identifier.scopusid | 2-s2.0-4444346116 | - |
dc.citation.endPage | 415 | - |
dc.citation.number | 1-4 SUPPL. | - |
dc.citation.startPage | 411 | - |
dc.citation.title | NUCLEAR PHYSICS A | - |
dc.citation.volume | 738 | - |
dc.type.docType | Article; Proceedings Paper | - |
dc.publisher.location | 네델란드 | - |
dc.subject.keywordPlus | HOT CNO CYCLE | - |
dc.subject.keywordPlus | ALPHA | - |
dc.subject.keywordPlus | STATES | - |
dc.subject.keywordPlus | NE-18 | - |
dc.subject.keywordPlus | O-14 | - |
dc.relation.journalResearchArea | Physics | - |
dc.relation.journalWebOfScienceCategory | Physics, Nuclear | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
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