Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | 한인식 | * |
dc.date.accessioned | 2016-08-28T11:08:05Z | - |
dc.date.available | 2016-08-28T11:08:05Z | - |
dc.date.issued | 2012 | * |
dc.identifier.isbn | 9780735410961 | * |
dc.identifier.issn | 0094-243X | * |
dc.identifier.other | OAK-13943 | * |
dc.identifier.uri | https://dspace.ewha.ac.kr/handle/2015.oak/229884 | - |
dc.description.abstract | Astrophysical stellar reactions at extremely high temperatures involve a variety of problems both in nuclear reactions and nuclear structures. Specifically, the problems in the νpprocess were discussed in this talk based on our recent experimental results with low-energy RI beams and a simulation study. The νp-process is one of the key processes for investigating the mechanism of type II supernovae, and the process could be possibly responsible for "the excess production" of p-nuclei around mass 90-100. Alpha cluster resonances have been discovered experimentally to play a crucial role for the stellar (α, p) reactions just above the alpha threshold. Neutron induced reactions in the proton-rich nuclear regions in the νp-process are also suggested to play an important role, which involve nuclear structures of high level density at high excitation energies, probably giant resonances. The discussion also covered the p-nuclei production through the νp-process at around mass 100. © 2012 American Institute of Physics. | * |
dc.description.sponsorship | University of Tokyo, Center of Nuclear Study | * |
dc.language | English | * |
dc.title | Experimental challenge to nuclear physics problems in the νp-process | * |
dc.type | Conference Paper | * |
dc.relation.volume | 1484 | * |
dc.relation.index | SCOPUS | * |
dc.relation.startpage | 189 | * |
dc.relation.lastpage | 196 | * |
dc.relation.journaltitle | AIP Conference Proceedings | * |
dc.identifier.doi | 10.1063/1.4763394 | * |
dc.identifier.scopusid | 2-s2.0-84874547393 | * |
dc.author.google | Kubono S. | * |
dc.author.google | Binh D.N. | * |
dc.author.google | Hayakawa S. | * |
dc.author.google | Hashimoto T. | * |
dc.author.google | Kahl D.M. | * |
dc.author.google | Yamaguchi H. | * |
dc.author.google | Wakabayashi Y. | * |
dc.author.google | Teranishi T. | * |
dc.author.google | Iwasa N. | * |
dc.author.google | Komatsubara T. | * |
dc.author.google | Kato S. | * |
dc.author.google | Chen A. | * |
dc.author.google | Cherubini S. | * |
dc.author.google | Choi S.H. | * |
dc.author.google | Hahn I.S. | * |
dc.author.google | He J.J. | * |
dc.author.google | Khiem L.H. | * |
dc.author.google | Lee C.S. | * |
dc.author.google | Kwon Y.K. | * |
dc.author.google | Wanajo S. | * |
dc.author.google | Janka H.-T. | * |
dc.contributor.scopusid | 한인식(7201832280;57205469686;57192312712) | * |
dc.date.modifydate | 20240415134453 | * |