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Systematic study for grey particles in relativistic nucleus plus emulsion (Ag) interactions
Wang, XR; Tai A(台安); Tai, A; Sa, BH; Cai, X
1999
发表期刊SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY
卷号42期号:8页码:845-851
通讯作者Huazhong Normal Univ, Inst Particle Phys, Wuhan 430070, Peoples R China ; Acad Sinica, Inst High Energy Phys, Beijing 100039, Peoples R China ; China Inst Atom Energy, Beijing 102413, Peoples R China ; Free Univ Berlin, FB Phys, D-14195 Berlin, Germany
文章类型Article
摘要The hadronic and string cascade model and the corresponding event generator LUCIAE are used to study systematically the production of the grey particles in (14.6, 60 and 200 A GeV)0 + Em, (200A GeV)Si + Em, (200A GeV)S + Em and (11.6A GeV)Au + Em reactions. The dependences of the mean multiplicity, the multiplicity distributions and the polar angular distributions of the grey particles on the incident energy, the projectile mass and the collision centrality observed in emulsion experiments, respectively, are all reproduced by LUCIAE calculations. In addition the effects of the rescattering on the grey particle production are also investigated.
关键词relativistic heavy ion collision grey particle emulsion experiments LUCIAE model
学科领域Mathematics
DOI10.1007/BF02884272
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语种英语
WOS研究方向Mathematics
WOS类目Mathematics, Applied ; Mathematics
WOS记录号WOS:000082515600007
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被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/238596
专题理论物理室
作者单位中国科学院高能物理研究所
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GB/T 7714
Wang, XR,Tai A,Tai, A,et al. Systematic study for grey particles in relativistic nucleus plus emulsion (Ag) interactions[J]. SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY,1999,42(8):845-851.
APA Wang, XR,台安,Tai, A,Sa, BH,&Cai, X.(1999).Systematic study for grey particles in relativistic nucleus plus emulsion (Ag) interactions.SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY,42(8),845-851.
MLA Wang, XR,et al."Systematic study for grey particles in relativistic nucleus plus emulsion (Ag) interactions".SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY 42.8(1999):845-851.
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