View : 693 Download: 0

Full metadata record

DC Field Value Language
dc.contributor.author한인식*
dc.date.accessioned2018-12-14T16:30:22Z-
dc.date.available2018-12-14T16:30:22Z-
dc.date.issued2018*
dc.identifier.issn0374-4884*
dc.identifier.issn1976-8524*
dc.identifier.otherOAK-22913*
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/247563-
dc.description.abstractThe intense gamma-rays from classical novae are emitted due to the beta-decay of F-18 which is produced by the Hot-CNO cycle. The reaction rate of F-18(p,alpha)O-15 affects the prediction of the abundance of F-18. The main contribution to this reaction rate is from the resonances in Ne-19 near and above the proton threshold. Hence, many experiments and theoretical works have been performed on the low-lying F-18+p resonances. One of the methods for investigating Ne-19 parameters is studying the mirror nucleus F-19. alpha elastic scattering experiment was performed with a 7 MeV/u N-15 beam for investigating the resonance parameters in F-19 using the thick target method in inverse kinematics at the radioactive beam facility CRIB of the Center for Nuclear Study, the University of Tokyo. The excitation function of F-19 was obtained for the excitation energy E (x) = 6.7 - 7.7 MeV, and the parameters of the resonance states in F-19 were determined using an R-matrix analysis.*
dc.languageEnglish*
dc.publisherKOREAN PHYSICAL SOC*
dc.subjectF-19 structure*
dc.subjectAlpha scattering*
dc.subjectN-15 beam*
dc.titleStudy of F-19 Levels with E (x)=6.7-7.7 MeV by the N-15+alpha Scattering Experiment*
dc.typeArticle*
dc.relation.issue3*
dc.relation.volume73*
dc.relation.indexSCIE*
dc.relation.indexSCOPUS*
dc.relation.indexKCI*
dc.relation.startpage265*
dc.relation.lastpage270*
dc.relation.journaltitleJOURNAL OF THE KOREAN PHYSICAL SOCIETY*
dc.identifier.doi10.3938/jkps.73.265*
dc.identifier.wosidWOS:000441602400004*
dc.identifier.scopusid2-s2.0-85051704376*
dc.author.googleKim, D.*
dc.author.googleKim, G. W.*
dc.author.googlePark, S. Y.*
dc.author.googleKim, A.*
dc.author.googleHahn, K. I.*
dc.author.googleAbe, K.*
dc.author.googleBeliuskina, O.*
dc.author.googleHayakawa, S.*
dc.author.googleImai, N.*
dc.author.googleKitamura, N.*
dc.author.googleSakaguchi, Y.*
dc.author.googleYamaguchi, H.*
dc.author.googleCha, S. M.*
dc.author.googleChae, K. Y.*
dc.author.googleKwag, M. S.*
dc.author.googleHong, S. W.*
dc.author.googleLee, E. J.*
dc.author.googleLee, J. H.*
dc.author.googleLee, E. K.*
dc.author.googleMoon, J. Y.*
dc.author.googleBae, S. H.*
dc.author.googleChoi, S. H.*
dc.author.googleKubono, S.*
dc.author.googlePanin, V.*
dc.author.googleWakabayashi, Y.*
dc.author.googleIwasa, N.*
dc.author.googleKahl, D.*
dc.author.googleChen, A. A.*
dc.contributor.scopusid한인식(7201832280;57205469686;57192312712)*
dc.date.modifydate20240415134453*
Appears in Collections:
사범대학 > 과학교육과 > Journal papers
Files in This Item:
There are no files associated with this item.
Export
RIS (EndNote)
XLS (Excel)
XML


qrcode

BROWSE