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Observation of heavy cluster emission from radioactive U-230 nuclei
Pan, QY; Yuan, SG; Yang, WF; Li, ZW; Ma, TT; Guo, JS; Liu, MY; Liu, HY; Xu, SW; Gan, ZG; Kong, DM; Qiao, JM; Luo, ZH; Zhang, MT; Wang, SH; Kong DM(孔登明); Qiao JM(乔际民); Luo ZH(罗紫华); Zhang MT(张沐天); Wang SH(王书鸿)
1999
Source PublicationHIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
Volume23Issue:11Pages:1039-1043
Corresponding AuthorChinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China ; Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China
SubtypeArticle
AbstractPa-230 was produced with the reaction Th-232 (p, 3n) 230Pa in the irradiation powder targets of ThO2 with 35 MeV proton beam. Sources of (230)pa -->(beta-) U-230 were prepared by radiochemical method. Using solid-state track registration detectors, two events of U-230 decay with heavy cluster emission have been observed. The preliminary branching ratio to alpha-decay comes out to be B = lambda(Ne)/lambda(alpha) = (1.3 +/- 0.8) x 10(-14).
Keywordpolyethylene-terephthalate (lavsan) solid-state track registration detector chemical etching decay of heavy cluster branching ratio
Subject AreaPhysics
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Language英语
WOS Research AreaPhysics
WOS SubjectPhysics, Nuclear ; Physics, Particles & Fields
WOS IDWOS:000084082400002
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Document Type期刊论文
Identifierhttp://ir.ihep.ac.cn/handle/311005/238941
Collection粒子天体物理中心
加速器中心
Affiliation中国科学院高能物理研究所
First Author AffilicationInstitute of High Energy
Recommended Citation
GB/T 7714
Pan, QY,Yuan, SG,Yang, WF,et al. Observation of heavy cluster emission from radioactive U-230 nuclei[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,1999,23(11):1039-1043.
APA Pan, QY.,Yuan, SG.,Yang, WF.,Li, ZW.,Ma, TT.,...&王书鸿.(1999).Observation of heavy cluster emission from radioactive U-230 nuclei.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,23(11),1039-1043.
MLA Pan, QY,et al."Observation of heavy cluster emission from radioactive U-230 nuclei".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 23.11(1999):1039-1043.
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