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Dynamics of strongly interacting parton-hadron matter

机译:强相互作用的Parton-强子物质的动力学

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In this study we investigate the dynamics of strongly interacting parton-hadron matter by calculating the centrality dependence of direct photons produced in Au+Au collisions at root S-NN = 200 GeV within the Parton-Hadron-String Dynamics (PHSD) transport approach. As sources for 'direct' photons, we incorporate the interactions of quarks and gluons as well as hadronic interactions (pi+pi -> rho+gamma, p+pi -> pi+gamma, meson-meson bremsstrahlung m + m -> m-m + gamma, meson baryon bremsstrahlung m + B -> m + B + gamma), the decays of phi and a(1) mesons and the photons produced in the initial hard collisions ('pQCD'). Our calculations suggest that the channel decomposition of the observed spectrum changes with centrality with an increasing (dominant) contribution of hadronic sources for more peripheral reactions. Furthermore, the 'thermal' photon yield is found to scale roughly with the number of participant nucleons as N-part(alpha) with alpha approximate to 1.5, whereas the partonic contribution scales with an exponent alpha(p) approximate to 1.75. Additionally, we provide predictions for the centrality dependence of the direct photon elliptic flow v(2) (P-T). The direct photon v(2) is seen to be larger in peripheral collisions compared to the most central ones since the photons from the hot deconfined matter in the early stages of the collision carry a much smaller elliptic flow than those from the final hadronic interactions. (c) 2014 Elsevier B.V. All rights reserved.
机译:在这项研究中,我们通过计算Parton-Hadron-String动力学(PHSD)传输方法中在根S-NN = 200 GeV的Au + Au碰撞中产生的直接光子的中心依赖性,来研究强相互作用的Parton-强子物质的动力学。作为“直接”光子的来源,我们结合了夸克和胶子的相互作用以及强子相互作用(pi + pi-> rho +γ,p + pi-> pi +γ,介子-介子致发光m + m-> mm +γ,介子重子致辐射m + B-> m + B +γ),phi和a(1)介子的衰变以及在最初的硬碰撞('pQCD')中产生的光子。我们的计算表明,观察到的光谱的通道分解随中心性的变化而变化,强子源对更多的周围反应的贡献增加(主要)。此外,发现“热”光子的产量大致与参与核子的数量成比例,即α约为1.5的N部分(α),而部分贡献的比例则约为1.75的指数α(p)。此外,我们提供了对直接光子椭圆流v(2)(P-T)的中心性依赖性的预测。与外围碰撞相比,直接碰撞的光子v(2)比最中心的碰撞要大,这是因为在碰撞早期,来自热受限物质的光子所携带的椭圆流比最终强子相互作用的光子小得多。 (c)2014 Elsevier B.V.保留所有权利。

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