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  • 标题:Fluctuations in nuclear collisions
  • 本地全文:下载
  • 作者:C. Pajares
  • 期刊名称:PoS - Proceedings of Science
  • 印刷版ISSN:1824-8039
  • 出版年度:2006
  • 出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
  • 摘要:T. Trainor: I point out that the formula w = w+ n+ n +w􀀀 n􀀀 n +w+􀀀2qn+n􀀀 n explains the difference between w+ and w charged. M. Gorenstein: Grand canonical ensamble reduces w+ and w􀀀 but not w+􀀀, so there are different answers to global charge conservation. T. Trainor: Mitchel presented a correlation lenth from the STAR data which is very small. What is the meaning of that?. On the other hand, this correlation length was considered in rapidity space. I think that also should be considered in azimuthal space to see whether there is a continuation of a small correlation length. In general the culture of looking at rapidity should be corrected to look also at azimuthal space. An example of that is the minijet correlation found by STAR on transverse momentum fluctuations looking at both spaces.
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