Study of stellar reactions in explosive hydrogen burning with CRIB
DC Field | Value | Language |
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dc.contributor.author | Kubono, S. | - |
dc.contributor.author | Teranishi, T. | - |
dc.contributor.author | Notani, M. | - |
dc.contributor.author | Yamaguchi, H. | - |
dc.contributor.author | Saito, A. | - |
dc.contributor.author | He, J.J. | - |
dc.contributor.author | Wakabayashi, M. | - |
dc.contributor.author | Fujikawa, H. | - |
dc.contributor.author | Amadio, G. | - |
dc.contributor.author | Baba, H. | - |
dc.contributor.author | Fukuchi, T. | - |
dc.contributor.author | Shimoura, S. | - |
dc.contributor.author | Michimasa, S. | - |
dc.contributor.author | Nishimura, S. | - |
dc.contributor.author | Nishimura, M. | - |
dc.contributor.author | Gono, Y. | - |
dc.contributor.author | Odahara, A. | - |
dc.contributor.author | Kato, S. | - |
dc.contributor.author | Moon, J.Y. | - |
dc.contributor.author | Lee, J.H. | - |
dc.contributor.author | Lee, C.S. | - |
dc.contributor.author | Kim, J.C. | - |
dc.contributor.author | Hahn, K.I. | - |
dc.contributor.author | Ishikawa, T. | - |
dc.contributor.author | Hashimoto, T. | - |
dc.contributor.author | Ishiyama, H. | - |
dc.contributor.author | Watanabe, Y.X. | - |
dc.contributor.author | Tanaka, M.H. | - |
dc.contributor.author | Miyatake, H. | - |
dc.contributor.author | Fulop, Z. | - |
dc.contributor.author | Guimaraes, V. | - |
dc.contributor.author | Lichtenthaler, R. | - |
dc.date.accessioned | 2022-01-11T02:41:41Z | - |
dc.date.available | 2022-01-11T02:41:41Z | - |
dc.date.issued | 2005-07 | - |
dc.identifier.issn | 0375-9474 | - |
dc.identifier.issn | 1873-1554 | - |
dc.identifier.uri | https://scholarworks.bwise.kr/cau/handle/2019.sw.cau/53213 | - |
dc.description.abstract | With using low-energy RI beams from an in-flight RIB separator, CRIB, the most crucial stellar reaction O-14(alpha,p)F-17 for the onset of the high-temperature rp-process was directly investigated and the transitions through the states at around 6.2 MeV in Ne-18 were first observed, confirming the importance predicted before. The (alpha,p) reaction leading to the first excited state in F-17 was also found to have a large contribution. A proton resonance search experiment of Mg-23 + p was also discussed, which is a part of our series of resonance search studies relevant to the early stage of the rp-process. | - |
dc.language | 영어 | - |
dc.language.iso | ENG | - |
dc.publisher | ELSEVIER SCIENCE BV | - |
dc.title | Study of stellar reactions in explosive hydrogen burning with CRIB | - |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.nuclphysa.2005.05.132 | - |
dc.identifier.bibliographicCitation | NUCLEAR PHYSICS A, v.758, no.1-4 SPEC. ISS., pp 733C - 736C | - |
dc.description.isOpenAccess | N | - |
dc.identifier.wosid | 000230660500159 | - |
dc.identifier.scopusid | 2-s2.0-20944436381 | - |
dc.citation.endPage | 736C | - |
dc.citation.number | 1-4 SPEC. ISS. | - |
dc.citation.startPage | 733C | - |
dc.citation.title | NUCLEAR PHYSICS A | - |
dc.citation.volume | 758 | - |
dc.type.docType | Article; Proceedings Paper | - |
dc.publisher.location | 네델란드 | - |
dc.subject.keywordPlus | RADIOACTIVE NUCLEAR BEAMS | - |
dc.subject.keywordPlus | HOT CNO CYCLE | - |
dc.subject.keywordPlus | ASTROPHYSICS | - |
dc.subject.keywordPlus | NE-18 | - |
dc.relation.journalResearchArea | Physics | - |
dc.relation.journalWebOfScienceCategory | Physics, Nuclear | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
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