Examination of directed flow as a signature of the softest point of the equation of state in QCD matter

IF 3.2 2区 物理与天体物理 Q2 PHYSICS, NUCLEAR Physical Review C Pub Date : 2016-01-28 DOI:10.1103/PhysRevC.94.034906
Y. Nara, H. Niemi, A. Ohnishi, H. Stoecker
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引用次数: 45

Abstract

We analyze the directed flow of protons and pions in high-energy heavy-ion collisions in the incident energy range from $\sqrt{{s}_{NN}}=7.7$ to 27 GeV within a microscopic transport model. Standard hadronic transport approaches do not describe the collapse of directed flow below $\sqrt{{s}_{NN}}\ensuremath{\simeq}20$ GeV. By contrast, a model that simulates effects of a softening of the equation of state descibes well the behavior of directed flow data recently obtained by the STAR Collaboration [Phys. Rev. Lett. 112, 162301 (2014)]. We give a detailed analysis of how directed flow is generated. Particularly, we found that softening of the effective equation of state at the overlapping region of two nuclei, i.e., the reaction stages where the system reaches high baryon density state, is needed to explain the observed collapse of proton directed flow within a hadronic transport approach.
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QCD物质中定向流动作为状态方程最软点特征的检验
本文在微观输运模型中分析了入射能量为$\sqrt{{s}_{NN}}=7.7$ ~ 27gev的高能重离子碰撞中质子和介子的定向流动。标准强子输运方法不能描述定向流在$\sqrt{{s}_{NN}}\ensuremath{\simeq}20$ GeV以下的崩溃。相比之下,一个模拟状态方程软化效应的模型很好地描述了最近由STAR合作[物理学家]获得的定向流数据的行为。科学通报,2012,(2)。我们详细分析了定向流是如何产生的。特别是,我们发现在两核重叠区域,即系统达到高重子密度状态的反应阶段,需要软化有效状态方程来解释在强子输运方法中观察到的质子定向流崩溃。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Physical Review C
Physical Review C PHYSICS, NUCLEAR-
CiteScore
5.80
自引率
35.50%
发文量
863
期刊介绍: Physical Review C (PRC) is a leading journal in theoretical and experimental nuclear physics, publishing more than two-thirds of the research literature in the field. PRC covers experimental and theoretical results in all aspects of nuclear physics, including: Nucleon-nucleon interaction, few-body systems Nuclear structure Nuclear reactions Relativistic nuclear collisions Hadronic physics and QCD Electroweak interaction, symmetries Nuclear astrophysics
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