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2024年10月30日

Energy dependence of resonance production in relativistic heavy ion collisions

  • 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:
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  • [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)
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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
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Received: 2016-08-19
Revised: 2016-09-23
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    Supported by National Natural Science Foundation of China (11575100, 11305076, 11505104)

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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
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.

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