• [1]

    D. A. Clarke, P. Dimopoulos, F. Di Renzo, J. Goswami, C. Schmidt, S. Singh, and K. Zambello, (2024), arXiv: 2405.10196[hep-lat].

  • [2]

    G. Basar, Phys. Rev. C 110, 015203 (2024), arXiv: 2312.06952[hep-th]

  • [3]

    M. Hippert, J. Grefa, T. A. Manning, J. Noronha, J. Noronha-Hostler, I. Portillo Vazquez, C. Ratti, R. Rougemont, and M. Trujillo, Phys. Rev. D 110, 094006 (2024), arXiv: 2309.00579[nucl-th]

  • [4]

    W.-j. Fu, J. M. Pawlowski, and F. Rennecke, Phys. Rev. D 101, 054032 (2020), arXiv: 1909.02991[hep-ph]

  • [5]

    P. J. Gunkel and C. S. Fischer, Phys. Rev. D 104, 054022 (2021), arXiv: 2106.08356[hep-ph]

  • [6]

    F. Gao and J. M. Pawlowski, Phys. Lett. B 820, 136584 (2021), arXiv: 2010.13705[hep-ph]

  • [7]

    A. Sorensen and P. Sorensen, (2024), arXiv: 2405.10278 [nucl-th].

  • [8]

    H. Shah, M. Hippert, J. Noronha, C. Ratti, and V. Vovchenko, (2024), arXiv: 2410.16206[hep-ph].

  • [9]

    Y. Hatta and M. A. Stephanov, Phys. Rev. Lett. 91, 102003 (2003), [Erratum: Phys.Rev.Lett. 91, 129901 (2003)], arXiv: hep-ph/0302002.

  • [10]

    M. Asakawa and M. Kitazawa, Prog. Part. Nucl. Phys. 90, 299 (2016), arXiv: 1512.05038[nucl-th]

  • [11]

    M. Kitazawa and X. Luo, Phys. Rev. C 96, 024910 (2017), arXiv: 1704.04909[nucl-th]

  • [12]

    X. Luo and N. Xu, Nucl. Sci. Tech. 28, 112 (2017), arXiv: 1701.02105[nucl-ex]

  • [13]

    M. M. Aggarwal et al. (STAR), Phys. Rev. Lett. 105, 022302 (2010), arXiv: 1004.4959[nucl-ex]

  • [14]

    L. Adamczyk et al. (STAR), Phys. Rev. Lett. 112, 032302 (2014), arXiv: 1309.5681[nucl-ex]

  • [15]

    L. Adamczyk et al. (STAR), Phys. Rev. Lett. 113, 092301 (2014), arXiv: 1402.1558[nucl-ex]

  • [16]

    L. Adamczyk et al. (STAR), Phys. Lett. B 785, 551 (2018), arXiv: 1709.00773[nucl-ex]

  • [17]

    J. Adam et al. (STAR), Phys. Rev. C 100, 014902 (2019), arXiv: 1903.05370[nucl-ex]

  • [18]

    J. Adam et al. (STAR), Phys. Rev. Lett. 126, 092301 (2021), arXiv: 2001.02852[nucl-ex]

  • [19]

    M. Abdallah et al. (STAR), Phys. Rev. C 104, 024902 (2021), arXiv: 2101.12413[nucl-ex]

  • [20]

    M. Abdallah et al. (STAR), Phys. Rev. Lett. 127, 262301 (2021), arXiv: 2105.14698[nucl-ex]

  • [21]

    M. S. Abdallah et al. (STAR), Phys. Rev. Lett. 128, 202303 (2022), arXiv: 2112.00240[nucl-ex]

  • [22]

    M. Abdallah et al. (STAR), Phys. Rev. C 107, 024908 (2023), arXiv: 2209.11940[nucl-ex]

  • [23]

    B. Aboona et al. (STAR), Phys. Rev. Lett. 130, 082301 (2023), arXiv: 2207.09837[nucl-ex]

  • [24]

    M. Abdulhamid et al. (STAR), Phys. Lett. B 857, 138966 (2024), arXiv: 2311.00934[nucl-ex]

  • [25]

    M. Abdulhamid et al. (STAR), Phys. Lett. B 855, 138560 (2024), arXiv: 2304.10993[nucl-ex]

  • [26]

    J. Chen, et al., Nucl. Sci. Tech. 35, 214 (2024), arXiv: 2407.02935[nucl-ex]

  • [27]

    M. Abdulhamid et al. (STAR), (2025), arXiv: 2504.00817 [nucl-ex].

  • [28]

    J. Xu, S. Yu, F. Liu, and X. Luo, Phys. Rev. C 94, 024901 (2016), arXiv: 1606.03900[nucl-ex]

  • [29]

    S. A. Bass, et al., Prog. Part. Nucl. Phys. 41, 255 (1998), arXiv: nucl-th/9803035

  • [30]

    M. Bleicher, et al., J. Phys. G 25, 1859 (1999), arXiv: hepph/9909407

  • [31]

    X. Luo, J. Xu, B. Mohanty, and N. Xu, J. Phys. G 40, 105104 (2013), arXiv: 1302.2332[nucl-ex]

  • [32]

    A. Chatterjee, Y. Zhang, J. Zeng, N. R. Sahoo, and X. Luo, Phys. Rev. C 101, 034902 (2020), arXiv: 1910.08004[nucl-ex]

  • [33]

    Y. Ye, Y. Wang, J. Steinheimer, Y. Nara, H.-j. Xu, P. Li, D. Lu, Q. Li, and H. Stoecker, Phys. Rev. C 98, 054620 (2018)

  • [34]

    Y. Ye, Y. Wang, Q. Li, D. Lu, and F. Wang, Phys. Rev. C 101, 034915 (2020), arXiv: 2004.11745[nucl-th]

  • [35]

    A. Chatterjee, Y. Zhang, H. Liu, R. Wang, S. He, and X. Luo, Chin. Phys. C 45, 064003 (2021), arXiv: 2009.03755[nucl-ex]

  • [36]

    M. L. Miller, K. Reygers, S. J. Sanders, and P. Steinberg, Ann. Rev. Nucl. Part. Sci. 57, 205 (2007), arXiv: nuclex/0701025

  • [37]

    X. Luo, Phys. Rev. C 91, 034907 (2015), arXiv: 1410.3914 [physics.data-an]

  • [38]

    CBM Collaboration, “CBM progress report 2023, ” (2023), accessed on 16 June 2025.

  • [39]

    Z. Sweger (STAR Collaboration), “Proton high-order cumulants results from the star fixed-target program, ” https://indico.cern.ch/event/1334113/contributions/6369534/attachments/3048338/5386843/QM2025_Sweger_v64.pdf, Quark Matter 2025, accessed April 9, 2025.