Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2017, Vol. 41> Issue(1) : 014101 DOI: 10.1088/1674-1137/41/1/014101

Energy dependence of resonance production in relativistic heavy ion collisions

  • 1.

      School of Physics and Engineering, Qufu Normal University, Shandong 273165, China

  • 2.

      Department of Physics, Jining University, Shandong 273155, China

  • The production of the hadronic resonances K*0(892), φ(1020), Σ*(1385), and Ξ*(1530) in central AA collisions at √sNN= 17.3, 200, and 2760 GeV is systematically studied. The direct production of these resonances at system hadronization is described by the quark combination model and the effects of hadron multiple-scattering stage are dealt with by a ultra-relativistic quantum molecular dynamics model (UrQMD). We study the contribution of these two production sources to final observation and compare the final spectra with the available experimental data. The pT spectra of K*0(892) calculated directly by quark combination model are explicitly higher than the data at low pT≤1.5 GeV, and taking into account the modification of rescattering effects, the resulting final spectra well agree with the data at all three collision energies. The rescattering effect on φ(1020) production is weak and including it can slightly improve our description at low pT on the basis of overall agreement with the data. We also predict the pT spectra of Σ*(1385) and Ξ*(1530), to be tested by the future experimental data.
      PCAS:
  • 加载中

  • References

    [1] Quark Gluon Plasma 3, edited by R. C. Hwa and X. N. Wang (Singapore:World Scientific, 2004)
    [2] T. Anticic et al (NA49 Collaboration), Phys. Rev. C, 84:064909(2011)
    [3] C. Alt et al (NA49 Collaboration), Phys. Rev. C, 78:044907(2008)
    [4] M. M. Aggarwa et al (STAR Collaboration), Phys. Rev. C, 84:34909(2011)
    [5] B. I. Abelev et al (STAR Collaboration), Phys. Rev. Lett., 97:132301(2006)
    [6] B. B. Abelev et al (ALICE Collaboration), Phys. Rev. C, 91:024609(2015)
    [7] M. Bleicher and J. Aichelin, Phys. Lett. B, 530:81(2002)
    [8] M. Bleicher, Nucl. Phys. A, 715:85c (2003)
    [9] S. Vogel and M. Bleicher, arXiv:nuclth/0505027
    [10] S. Vogel, J. Aichelin, and M. Bleicher, J. Phys. G, 37:094046(2010)
    [11] A. G. Knospe, C. Markert, K. Werner et al, Phys. Rev. C, 93:014911(2016)
    [12] K. Zhang, J. Song, and F. L. Shao, Phys. Rev. C 86:014906(2012)
    [13] K. C. Liu, J. Song, and F.L. Shao, Int. J. Mod. Phys. E, 23:1450060(2014)
    [14] R. J. Fries, B. Mller, C. Nonaka et al, Phys. Rev. Lett., 90:202303(2003)
    [15] V. Greco, C. M. Ko, and P. Lvai, Phys. Rev. Lett., 90:202302(2003)
    [16] R. C. Hwa and C. B. Yang, Phys. Rev. C, 70:024905(2004)
    [17] L. W. Chen and C. M. Ko, Phys. Rev. C, 73:044903(2006)
    [18] F. L. Shao, Q. B. Xie, and Q. Wang, Phys. Rev. C, 71:044903(2005); C. E. Shao, J. Song, F. L. Shao et al, Phys. Rev. C, 80:014909(2009)
    [19] R. Q. Wang, F. L. Shao, J. Song et al, Phys. Rev. C, 86:054906(2012)
    [20] J. Song and F. L. Shao, Phys. Rev. C, 88:027901(2013)
    [21] R. Q. Wang, J. Song, and F. L. Shao, Phys. Rev. C, 91:014909(2015)
    [22] L. X. Sun, R. Q. Wang, J. Song et al, Chin.Phys. C, 36 (1):55(2012)
    [23] J. Song, F. L. Shao, Q. B. Xie et al, Chin. Phys. C, 33(6):481(2009)
    [24] S. A. Bass, M. Belkacem, M. Bleicher et al, Prog. Part. Nucl. Phys., 41:225(1998)
    [25] M. Bleicher, E. Zabrodin, C. Spieles et al, J. Phys. G, 25:1859(1999)
    [26] B. I. Abelev et al (STAR Collaboration), Phys. Rev. Lett., 99:112301(2007)
    [27] B. B. Abelev et al (ALICE Collaboration), Phys. Rev. Lett., 109:252301(2012)
    [28] B. B. Abelev et al (ALICE Collaboration), Phys. Lett. B, 736:196(2014)
    [29] B. B. Abelev et al (ALICE Collaboration), Phys. Lett. B, 728:216(2014)
    [30] B. B. Abelev et al (ALICE Collaboration), Phys. Rev. Lett., 111:222301(2013)
    [31] C. Shen, U. Heinz, P. Huovinen et al, Phys. Rev. C, 84:044903(2011)
    [32] Iu.A. Karpenko and Yu.M. Senyukov, J. Phys. G, 38:124059(2011)
    [33] Iu.A. Karpenko, Yu.M. Sinyukov, and K. Werner Phys. Rev. C, 87:024914(2013)
    [34] P. Bozek, Phys. Rev. C, 85:034901(2012)
    [35] P. Bozek, Acta Phys. Pol. B, 43 (4):689(2012)

  • Access

    加载中

Get Citation
Feng-Lan Shao, Jun Song, Rui-Qin Wang and Mao-Sheng Zhang. Energy dependence of resonance production in relativistic heavy ion collisions[J]. Chinese Physics C, 2017, 41(1): 014101. doi: 10.1088/1674-1137/41/1/014101
Feng-Lan Shao, Jun Song, Rui-Qin Wang and Mao-Sheng Zhang. Energy dependence of resonance production in relativistic heavy ion collisions[J]. Chinese Physics C, 2017, 41(1): 014101.  doi: 10.1088/1674-1137/41/1/014101 shu
Milestone
Received: 2016-08-19
Revised: 2016-09-23
Fund

    Supported by National Natural Science Foundation of China (11575100, 11305076, 11505104)

Article Metric

Article Views(1719)
PDF Downloads(24)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, [email protected]
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Energy dependence of resonance production in relativistic heavy ion collisions

    Corresponding author: Feng-Lan Shao,
  • 1.  School of Physics and Engineering, Qufu Normal University, Shandong 273165, China
  • 2.  Department of Physics, Jining University, Shandong 273155, China
  • Received Date: 2016-08-19
  • Accepted Date: 2016-09-23
  • Available Online: 2017-01-05
Fund Project:  Supported by National Natural Science Foundation of China (11575100, 11305076, 11505104)

Abstract: The production of the hadronic resonances K*0(892), φ(1020), Σ*(1385), and Ξ*(1530) in central AA collisions at √sNN= 17.3, 200, and 2760 GeV is systematically studied. The direct production of these resonances at system hadronization is described by the quark combination model and the effects of hadron multiple-scattering stage are dealt with by a ultra-relativistic quantum molecular dynamics model (UrQMD). We study the contribution of these two production sources to final observation and compare the final spectra with the available experimental data. The pT spectra of K*0(892) calculated directly by quark combination model are explicitly higher than the data at low pT≤1.5 GeV, and taking into account the modification of rescattering effects, the resulting final spectra well agree with the data at all three collision energies. The rescattering effect on φ(1020) production is weak and including it can slightly improve our description at low pT on the basis of overall agreement with the data. We also predict the pT spectra of Σ*(1385) and Ξ*(1530), to be tested by the future experimental data.

    HTML

Reference (35)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: [email protected]

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: [email protected]

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return