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Dependence of Multiparticle Processes on the Interaction-Region Size in Collisions of High-Energy Protons and Nuclei

机译:多粒程过程对高能质子和核碰撞中的相互作用区域尺寸的依赖性

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摘要

The problem of the dependence of multiparticle reaction-product formation on the interactionregion size is considered both at cosmic-ray and accelerator energies. In cosmic rays, a comparative analysis of interactions induced by protons and light nuclei was performed on the basis of data obtained by the Stratosphere Collaboration. At accelerator energies, the problem was studied by employing data of the EMU Collaboration. The results revealed a substantial distinction between the production processes in these event groups. An analysis of interactions between light nuclei, (C, O, Ne) + (C/N/O); between intermediate and light nuclei, (Si, S) + (C/N/O); and between heavy nuclei, (Au, Pb) + (Ag/Br), showed that there is a sizable enhancement of fluctuations as the size of the interaction region becomes smaller. A sharp growth of multiplicity and pseudorapidity correlations in the most central interactions, (C, O, Ne) + (C/N/O), is interpreted as a manifestation of internal virtual alpha-particle clustering of light nuclei.
机译:在宇宙射线和加速器能量上认为多粒子反应 - 产物形成对相互作用的依赖性的问题。在宇宙射线中,基于平流层协作获得的数据进行质子和光髓诱导的相互作用的对比分析。在加速器能量下,通过使用EMU协作的数据研究了问题。结果表明,这些事件组中的生产过程之间的实质性区别。轻质核,(C,O,Ne)+(C / N / O)之间的相互作用分析;中间和光核,(Si,S)+(C / N / O);在重核之间,(Au,Pb)+(Ag / Br)之间表明,随着相互作用区域的尺寸变小,波动的大大增强。在最中心相互作用中的多样性和初度相关性的急剧增长,(C,O,Ne)+(C / N / O)被解释为光核的内部虚拟α-粒子聚类的表现。

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