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Di-jet measurements in heavy-ion collisions at STAR

机译:STAR重离子碰撞中的双喷测量

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Jets are produced from hard scatterings in the early stages of heavy-ion collisions. It is expected that these high-pT partons travel through the hot and dense medium before fragmenting. Therefore they are expected to suffer energy loss in the QGP via gluon radiation and elastic collisions along their path. Measurements of fully reconstructed jets help understand the effect of the energy loss on the jet structure and energy profile. A data-driven characterization of the background in Au+Au is needed in order to compare the results to p+p. The full azimuthal coverage of STAR Time Projection Chamber and Electromagnetic Calorimeter allows measurements of fully reconstructed di-jets, defined by jets that match the online trigger and recoil jets on the away side. A tight selection of the trigger jets allows for a selection of those coming from the surface. Hence, the population of jets on the recoil side is biased towards a maximal energy loss because of the extreme in-medium pathlength. We present measurements of di-jets, exploring their structure and properties in Au+Au and p+p at √s_(NN) = 200 GeV in the STAR experiment.
机译:在重离子碰撞的早期,喷射是由坚硬的散射产生的。预计这些高pT的部分在分裂前会穿过热的稠密介质。因此,预计它们会因胶子辐射和沿其路径的弹性碰撞而在QGP中遭受能量损失。完全重建的射流的测量有助于了解能量损失对射流结构和能量分布的影响。为了将结果与p + p进行比较,需要对Au + Au中的背景进行数据驱动的表征。 STAR时间投影腔室和电磁热量计的全方位角覆盖范围允许对完全重建的双喷头进行测量,该双喷头由与在线扳机和反冲喷头相匹配的喷头定义。扳机喷头的选择严格,可以选择来自地面的喷头。因此,由于极度中等的光程,反冲侧的射流偏向于最大的能量损失。我们介绍了双喷口的测量,在STAR实验中探索了它们在√s_(NN)= 200 GeV下在Au + Au和p + p中的结构和性质。

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