Abstract

In a multisource thermal model, we analyze the dependence of elliptic flow on the transverse momentum . The model results are compared with the data of , , , and measured in Pb + Au collisions at top SPS energy, 17.3 GeV. It is found that the azimuthal anisotropy in the evolution process of high-energy collisions is correlated highly to the number of participant nucleons.

1. Introduction

Collective flows are a common phenomenon of heavy ion collisions at high energy [15]. In a noncentral collision of two spherical nuclei, the overlapping zone between the two nuclei is not circular but it rather takes an almond shape, where pressure gradients are formed due to the azimuthal anisotropy. Then, the initial spatial anisotropy of the overlapping zone is converted into momentum space anisotropy of the particle distribution. The momentum distribution of emitted particles is quantified in terms of the Fourier expansion for the particle invariant azimuthal distribution [6]. These are defined by where and represent the azimuthal angle of an emitted particle in laboratory reference frame and the azimuthal angle of the reaction plane in the same frame, respectively. The represents the magnitude of the th-order anisotropy. The second-order coefficient of the anisotropy flow is called the elliptic flow, which is related to the almond shape mentioned above. The elliptic flow is one of the key observables measured at the RHIC, where large values of are considered as a sign of collectivity in the system created in the high-energy collisions. Recently, an event-by-event ideal hydrodynamic model is used to study the elliptic flow of thermal photons in Au + Au collisions at RHIC and Pb + Pb collisions at the LHC, and the results show that there is a persistent tension between experimental data and photons of hydrodynamics [7].

In this paper, we will discuss the elliptic flow in Pb + Au collision at  GeV, which is top SPS energy. To extract properties of the matter created in the asymmetry reaction, we improve a multisource thermal model, which was used to describe the particle production in our previous work [8].

2. Azimuthal Anisotropy and Number of Participant Nucleons

The initial transverse coordinate-space anisotropy of the participant region is converted into an azimuthal momentum-space anisotropy [9]. But we obtain the evolution information of such matter by final-state particles measured in detectors [10]. The transverse momentum of the particles has an invariant form in different reference fames: which is called Rayleigh distribution.

When two ultrarelativistic nuclei collide at a nonzero impact parameter, their overlap area in the transverse plane has a short axis which is parallel to the impact parameter and a long axis which is perpendicular to the impact parameter. Considering the mechanics effect, these sources depart from the isotropic emission. The distribution functions of and are where and denote the expansion coefficient of the source and the movement coefficient of the source, respectively. For Maxwell's ideal gas, and , and the nonexpanding source has no contribution to the collective flow. The particle distribution is . In the final state, the normalized distribution of total particles can be expressed as where and denote the contribution of isotropic sources and anisotropic sources, respectively. The is proportional to the number of nucleons participating : where and are the mass numbers of the Pb and Au, respectively.

In the Monte Carlo calculation, the transverse momenta are given by where , , , and denote random numbers in . According to the measurement in experiments, the elliptic flow in the model is defined as It is interesting to note that several different definitions of centralities in collision were given through other quantities because they are not a directly measurable quantity [11]. The centrality can usually be calculated by multiplicity distribution or fractional cross-section or impact parameter , [12]. The and are radii of Pb and Au, respectively. Theoretically, the number of participant nucleons in a collision of Pb + Au at the impact parameter is They can be estimated easily in the geometry method [13]: The nuclear density function is the Woods-Saxon density profile [14]: where refers to normal nuclear density and  fm stands for the nuclear diffusion edge from low energy electron-nucleus scattering experiments [15].

First, in order to check the reliability of the model, Figure 1 presents the transverse momentum spectra of charged pions, charged kaons and protons at midrapidity for Pb-Pb collisions at  GeV. The symbols denote the data measured by NA49 Collaboration [16]. The curves denote our results with and . The calculated results agree with the experimental data except for the region of  GeV/ .

Figure 2 shows elliptic flows of produced in Pb-Au collisions at  GeV. The symbols are the data measured by the CERES Collaboration [17] and NA49 Collaboration [18]. Collision centralities are 5.3–13% of for CERES and top 13% for NA49 data. The curves are our results with , which depends on collision energies and the centrality. The other parameters used in the calculations are and . The observed increases with increasing at the low transverse momentum and saturates in  GeV/ . The modeling results are in approximate agreement with the experimental data. Figures 3 and 4 show elliptic flows of for and produced in Pb-Au collisions at  GeV. The symbols denote the data measured by the CERES Collaboration [17]. The curves denote our results. One sees again that the model can approximately describe the elliptic flows in Pb-Au collisions at the top SPS energy.

In Figure 5, we show differential elliptic flows of protons in Pb-Au collisions at  GeV. In the given centrality, the dependence of on is similar to that for the pion. In Figure 6, we present differential elliptic flows of mesons and hyperons in Pb-Au collisions at  GeV. We also see the same behavior for the same centrality like the above figures. In order to understand the azimuthal anisotropy of final-state particles in the asymmetric collision, Figure 7 gives a comparison to the results of NA49 [19] at the same energy  GeV and gives a comparison to STAR results [20] at  GeV. The NA49 and CERES data are in reasonably good agreement. In order to compare STAR to CERES results, the former have been rescaled to the centrality used in the CERES experiment. The values measured at the RHIC energy are 15–20% higher due to the higher beam energy. Our results are in approximate agreement with the data measured by the three collaborations.

3. Conclusions

In the above discussions, we have investigated the azimuthal anisotropy by using the elliptic flow versus the transverse momentum in Pb + Au collisions at the top SPS energy  GeV. The amplitude of the azimuthal anisotropy can be measured by the elliptic flow, which is a sensitive probe of the matter created in the collisions. We improve the multisource statistical model to discuss the transverse momentum dependence of elliptic flows for the particles produced in the asymmetric system, Pb-Au collision at the top SPS energy. Considering the collision geometry, the modelling results are obtained in the framework of the multisource statistical model. The results agree approximately with the data of the CERN-CERES/NA45 Collaboration. More importantly, this model has partly described the particle production in high-energy collisions [8]. In the descriptions of elliptic flows in the asymmetric system (Pb + Au collision) at SPS energies, the present work is a new successful attempt.

Conflict of Interests

The authors declare that there is no conflict of interests regarding the publication of this paper.

Acknowledgments

This work is supported by the National Natural Science Foundation of China under Grants no. 11247250, no. 11005071, and no. 10975095, the National Fundamental Fund of Personnel Training under Grant no. J1103210, and the Shanxi Provincial Natural Science Foundation under Grants no. 2013021006 and no. 2011011001.