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arXiv 1107.4630nucl-exhep-ex
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在$\sqrt{s_{NN}}$ =62.4 GeV与STAR的AuAu碰撞中的$ρ^{0}$光产生

$ρ^{0}$ Photoproduction in AuAu Collisions at $\sqrt{s_{NN}}$=62.4 GeV with STAR

G. Agakishiev

摘要:

在相对论性重离子碰撞中,当一个原子核发射的虚光子从另一个原子核散射时,可以光生矢量介子。STAR协作先前已经提出了测量相干$ρ^0$光生在质量中心的能量为130 GeV和200 GeV的金-金碰撞。在这里,我们提出了在62.4 GeV的横截面的测量,我们发现,在62.4 GeV的相干$ρ^0$光生核分裂的横截面是$10.5\pm1.5\pm 1.6$ MB。200 GeV和62.4 GeV之间的截面比为$2.8\pm0.6$,小于大多数理论模型预测的。然而,这是成比例地比以前观察到的$15\pm 55$ %增加130 GeV和200 GeV之间。

英文摘要:

Vector mesons may be photoproduced in relativistic heavy-ion collisions when a virtual photon emitted by one nucleus scatters from the other nucleus, emerging as a vector meson. The STAR Collaboration has previously presented measurements of coherent $ρ^0$ photoproduction at center of mass energies of 130 GeV and 200 GeV in AuAu collisions. Here, we present a measurement of the cross section at 62.4 GeV; we find that the cross section for coherent $ρ^0$ photoproduction with nuclear breakup is $10.5\pm1.5\pm 1.6$ mb at 62.4 GeV. The cross-section ratio between 200 GeV and 62.4 GeV is $2.8\pm0.6$, less than is predicted by most theoretical models. It is, however, proportionally much larger than the previously observed $15\pm 55$% increase between 130 GeV and 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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