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arXiv 1109.3891nucl-ex
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在STAR上测量翻转核修正因子

Measuring the Upsilon Nuclear Modification Factor at STAR

Rosi Reed

摘要:

在重离子碰撞中,由于重夸克间的相互作用势被德拜屏蔽,相对于质子-质子碰撞,夸克偶素被抑制,这被认为是夸克-胶子等离子体(QGP)的一个特征.然而,除了德拜屏蔽之外的其他效应,如夸克-反夸克重味对的统计重组,或同动子吸收也会影响重离子碰撞中的夸克偶素产生。量化整个夸克偶素介子族的抑制可以给我们一个依赖于温度的模型约束。可以通过计算核修正因子(RAA)来量化对Upperdance的抑制,RAA是Au+Au碰撞中产生的产物与p+p中产生的产物的比率,该比率由二元碰撞的数量缩放。本文给出了sqrt(sNN)= 200 GeV时p+p碰撞和Au+Au碰撞中产生的中快度Upperdum(1 S +2S+3S)的结果。将显示合并的Uppersity(1 S +2S+3S)产量的RAA中心依赖性。

英文摘要:

Suppression of quarkonia in heavy ion collisions with respect to proton-proton collisions due to the Debye screening of the potential between the heavy quarks was hypothesized to be a signature of the Quark Gluon Plasma (QGP). However, other effects besides Debye screening, such as the statistical recombination of quark anti-quark heavy flavor pairs, or co-mover absorption can also affect quarkonia production in heavy ion collisions. Quantifying the suppression of an entire family of quarkonium mesons can give us a model dependent constraint on the temperature. The suppression of Upsilon can be quantified by calculating the Nuclear Modification factor, RAA, which is the ratio of the production in Au+Au collisions to the production in p+p scaled by the number of binary collisions. We present our results for mid-rapidity Upsilon(1S+2S+3S) production in p+p and Au+Au collisions at sqrt(sNN) = 200 GeV. The centrality dependence of RAA will be shown for the combined Upsilon(1S+2S+3S) yield.

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