DSpace at EWHA: Beam production of 18Ne with in-flight method for alpha scattering at CRIB

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DC Field	Value	Language
dc.contributor.author	한인식	*
dc.date.accessioned	2018-12-14T16:31:09Z	-
dc.date.available	2018-12-14T16:31:09Z	-
dc.date.issued	2018	*
dc.identifier.issn	0168-9002	*
dc.identifier.other	OAK-22465	*
dc.identifier.uri	https://dspace.ewha.ac.kr/handle/2015.oak/247828	-
dc.description.abstract	We conducted a measurement of 18Ne + α scattering in inverse kinematics, in order to search for experimental evidence of α-cluster structure in 22Mg above the alpha threshold (Ethr=8.14MeV) and determine the astrophysical rates of the 18Ne(α p)21Na reaction under the conditions of break-out from the Hot-CNO cycle. A high intensity 18Ne beam at 2.54 AMeV was successfully produced at CRIB (CNS Radioactive Ion Beam separator) of the Center for Nuclear Study, the University of Tokyo. This paper presents the in-flight production of the radioactive 18Ne beam by using the production reaction 3He(16O, 18Ne)n with a windowed cryogenic gas target, which was employed in the mentioned resonant α-scattering experiment. © 2018 Elsevier B.V.	*
dc.description.sponsorship	University of Tokyo	*
dc.language	English	*
dc.publisher	Elsevier B.V.	*
dc.subject	Alpha cluster	*
dc.subject	Alpha scattering	*
dc.subject	Inverse kinematics	*
dc.subject	RI beam production	*
dc.title	Beam production of 18Ne with in-flight method for alpha scattering at CRIB	*
dc.type	Article	*
dc.relation.volume	897	*
dc.relation.index	SCIE	*
dc.relation.index	SCOPUS	*
dc.relation.startpage	8	*
dc.relation.lastpage	13	*
dc.relation.journaltitle	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment	*
dc.identifier.doi	10.1016/j.nima.2018.04.043	*
dc.identifier.wosid	WOS:000433206800002	*
dc.identifier.scopusid	2-s2.0-85046722853	*
dc.author.google	Duy N.N.	*
dc.author.google	Chae K.Y.	*
dc.author.google	Cha S.M.	*
dc.author.google	Yamaguchi H.	*
dc.author.google	Abe K.	*
dc.author.google	Bae S.H.	*
dc.author.google	Binh D.N.	*
dc.author.google	Choi S.H.	*
dc.author.google	Hahn K.I.	*
dc.author.google	Hayakawa S.	*
dc.author.google	Hong B.	*
dc.author.google	Iwasa N.	*
dc.author.google	Kahl D.	*
dc.author.google	Khiem L.H.	*
dc.author.google	Kim A.	*
dc.author.google	Kim D.H.	*
dc.author.google	Kim E.J.	*
dc.author.google	Kim G.W.	*
dc.author.google	Kim M.J.	*
dc.author.google	Kwak K.	*
dc.author.google	Kwag M.S.	*
dc.author.google	Lee E.J.	*
dc.author.google	Lim S.I.	*
dc.author.google	Moon B.	*
dc.author.google	Moon J.Y.	*
dc.author.google	Park S.Y.	*
dc.author.google	Phong V.H.	*
dc.author.google	Shimizu H.	*
dc.author.google	Yang L.	*
dc.author.google	Ge Z.	*
dc.author.google	Hao T.V.N.	*
dc.contributor.scopusid	한인식(7201832280;57205469686;57192312712)	*
dc.date.modifydate	20240415134453	*