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arXiv 0804.4661nucl-ex
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STAR对长程前向-后向多重关联的测量,作为$\sqrt{s_{NN}}=$ 200 GeV重离子碰撞中“稠密部分子物质”的特征。

STAR's measurement of Long-range forward-backward multiplicity correlations as the signature of "dense partonic matter" in the Heavy Ion collisions at $\sqrt{s_{NN}}=$200 GeV.}

Brijesh K Srivastava

摘要:

用STAR探测器测量了$\sqrt{s_{NN}}$ = 200 GeV的Au+Au、Cu+Cu和{ \it p+p}碰撞的前向-后向多重关联。中心重离子碰撞中观察到一个很强的长程相关,而在半外围事件和{ \it pp}碰撞中则消失了。相关强度与参与碰撞的参与者数量之间没有明显的比例关系。双部分子模型和彩色玻璃凝聚体都表明长程关联是由多部分子相互作用引起的。这表明致密的部分子物质可能是在$\sqrt{s_{NN}}$ = 200 GeV的中中心和中心Au+Au碰撞中产生的。

英文摘要:

Forward-backward multiplicity correlations have been measured with the STAR detector for Au+Au, Cu+Cu and {\it p+p} collisions at $\sqrt{s_{NN}}$ = 200 GeV. A strong, long-range correlation is observed for central heavy ion collisions that vanishes in semi-peripheral events and {\it pp} collisions. There is no apparent scaling of correlation strength with the number of participants involved in the collision. Both the Dual Parton Model and the Color Glass condensate indicate that the long range correlations are due to multiple parton interactions. This suggests that the dense partonic matter might have been created in mid-central and central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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