更正:在RHIC中√sNN = 3 GeV Au+Au碰撞中部分子集体的消失[物理学]。列托人。[au:] [B]

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
STAR Collaboration , D. Isenhower , J.L. Drachenberg , M. Daugherity , L. Adamczyk , L. Fulek , M. Przybycien , R. Sikora , I. Alekseev , D.N. Svirida , I.G. Bordyuzhin , D.G. Underwood , H.M. Spinka , M. Zurek , A. Hamed , F.M. Fawzi , M.S. Abdallah , J. Jia , A. Jentsch , A. Kiselev , T. Liu
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引用次数: 0

摘要

我们报告了在sNN = 3 GeV的Au+Au碰撞中强子(π±,K±,KS0, p, ϕ, Λ和Ξ−)的定向流v1和椭圆流v2的测量,以及在27和54.4 GeV的(π±,K±,p和p)的v2与STAR实验。而在两个高能量的中中心碰撞中,成分夸克数(NCQ)标度保持不变,在3 GeV时,所有强子的中快速度v2都为负,NCQ标度不存在。此外,几乎所有观测到的强子在中速时的v1斜率都是正的,这意味着重子相互作用是排斥性的。在输运模型计算中,重子平均场可以再现3 GeV时负v2和正v1斜率的特征。这些结果表明,这种碰撞中的介质很可能具有重子相互作用的特征。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Erratum: Disappearance of partonic collectivity in √ sNN = 3 GeV Au+Au collisions at RHIC [Phys. Lett. B 827, 137003 (2022)]
We report on the measurements of directed flow v1 and elliptic flow v2 for hadrons (π±, K±, KS0, p, ϕ, Λ and Ξ) from Au+Au collisions at sNN = 3 GeV and v2 for (π±, K±, p and p) at 27 and 54.4 GeV with the STAR experiment. While at the two higher energy midcentral collisions the number-of-constituent-quark (NCQ) scaling holds, at 3 GeV the v2 at midrapidity is negative for all hadrons and the NCQ scaling is absent. In addition, the v1 slopes at midrapidity for almost all observed hadrons are found to be positive, implying dominant repulsive baryonic interactions. The features of negative v2 and positive v1 slope at 3 GeV can be reproduced with a baryonic mean-field in transport model calculations. These results imply that the medium in such collisions is likely characterized by baryonic interactions.
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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