Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 한인식 | * |
dc.date.accessioned | 2016-08-27T02:08:49Z | - |
dc.date.available | 2016-08-27T02:08:49Z | - |
dc.date.issued | 2003 | * |
dc.identifier.issn | 0375-9474 | * |
dc.identifier.other | OAK-1434 | * |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/215582 | - |
dc.description.abstract | The O-14(alpha,p)F-17 reaction is an important part of the hot CNO cycle. We have measured cross sections for the F-17(pp)F-17(gs), F-17(p,p(1))F-17(495)*, and F-17(p,alpha)O-14 reactions in inverse kinematics using radioactive F-17 beams from the Holifield Radioactive Ion Beam Facility. The properties of states in Ne-18, including those important for the O-14(alpha,p)F-17 reaction rate, were determined from an R-matrix analysis of the measured cross sections. An improved O-14(alpha,p)F-17 reaction rate has been determined. The hot CNO cycle of reactions is important in explosive astrophysical environments such as novae and X-ray bursts. In this cycle, proton captures by C-12 and N-13 in succession lead to the production of O-14. Destruction of O-14 occurs by O-14(beta(+))N-14 and by the O-14 (alpha,p)F-17 reaction. The slow rate of this reaction can limit energy generation and result in substantial abundances of the O-14 isotope in novae [1] and X-ray bursts [2]. | * |
dc.language | English | * |
dc.publisher | ELSEVIER SCIENCE BV | * |
dc.title | The O-14(alpha,p)F-17 reaction rate | * |
dc.type | Article | * |
dc.type | Proceedings Paper | * |
dc.relation.volume | 718 | * |
dc.relation.index | SCI | * |
dc.relation.index | SCIE | * |
dc.relation.index | SCOPUS | * |
dc.relation.startpage | 127C | * |
dc.relation.lastpage | 130C | * |
dc.relation.journaltitle | NUCLEAR PHYSICS A | * |
dc.identifier.doi | 10.1016/S0375-9747(03)00689-4 | * |
dc.identifier.wosid | WOS:000182314300018 | * |
dc.author.google | Blackmon, JC | * |
dc.author.google | Bardayan, DW | * |
dc.author.google | Bradfield-Smith, W | * |
dc.author.google | Brummitt, R | * |
dc.author.google | Champagne, AE | * |
dc.author.google | Chen, AA | * |
dc.author.google | Davinson, T | * |
dc.author.google | Dessieux, L | * |
dc.author.google | Guidry, MW | * |
dc.author.google | Hahn, KI | * |
dc.author.google | Hale, GM | * |
dc.author.google | Hix, WR | * |
dc.author.google | Kozub, RL | * |
dc.author.google | Ma, Z | * |
dc.author.google | Parker, PD | * |
dc.author.google | Rajbaidya, G | * |
dc.author.google | Runkle, RC | * |
dc.author.google | Rowland, CM | * |
dc.author.google | Shotter, AC | * |
dc.author.google | Smith, MS | * |
dc.author.google | Van Wormer, LA | * |
dc.author.google | Visser, DW | * |
dc.author.google | Woods, PJ | * |
dc.contributor.scopusid | 한인식(7201832280;57205469686;57192312712) | * |
dc.date.modifydate | 20240415134453 | * |