Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Open Access

(3+1)D event-by-event preequilibrium dynamics in heavy-ion collisions

Xiaojian Du1,2,3,4,5, Sören Schlichting6, and Jie Zhu6,7,*

  • *Contact author: jzhu@physik.uni-bielefeld.de

Phys. Rev. D 113, 096009 – Published 11 May, 2026

DOI: https://doi.org/10.1103/hpzj-xx3h

Abstract

So far a major source of uncertainty in the study of heavy-ion collisions arises from the early time dynamics which includes initial state and preequilibrium dynamics. The state-of-the-art framework, KøMPøST [Kurkela et al. Phys. Rev. C 99, 034910 (2019); Kurkela et al. Phys. Rev. Lett. 122, 122302 (2019)], employs nonequilibrium Green’s functions to propagate the initial energy-momentum tensor to the hydrodynamic phase, yet currently only treats transverse plane dynamics under boost-invariant conditions. In this work, we extend KøMPøST to include nonboost-invariant responses to initial conditions, essential for accurately capturing the longitudinal structures observed in heavy-ion collisions. Nonboost-invariant fluctuations on top of a homogeneous background are evolved using (3+1)D response functions calculated in kinetic theory. To assess kinetic theory’s transition towards hydrodynamic evolution, we systematically compare the out-of-equilibrium shear-stress tensor from KøMPøST-3D with estimates based on Navier-Stokes hydrodynamics. Subsequently, a comprehensive (3+1)D framework, mcdipper + KøMPøST-3D + CLVisc + SMASH, is utilized to simulate the complete spacetime evolution of heavy-ion collisions. The sensitivity of key observables, including longitudinal structure of anisotropic flow, to variations in the hydrodynamic initialization time is thoroughly investigated.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (76)

  1. B. Muller, J. Schukraft, and B. Wyslouch, Annu. Rev. Nucl. Part. Sci. 62, 361 (2012).
  2. B. Müller, Phys. Scr. T 158, 014004 (2013).
  3. J. S. Moreland, J. E. Bernhard, and S. A. Bass, Phys. Rev. C 101, 024911 (2020).
  4. W. Ke, J. S. Moreland, J. E. Bernhard, and S. A. Bass, Phys. Rev. C 96, 044912 (2017).
  5. D. Soeder, W. Ke, J. F. Paquet, and S. A. Bass, arXiv:2306.08665.
  6. B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. Lett. 108, 252301 (2012).
  7. B. Schenke, P. Tribedy, and R. Venugopalan, Phys. Rev. C 86, 034908 (2012).
  8. H. Mäntysaari, B. Schenke, C. Shen, and P. Tribedy, Phys. Lett. B 772, 681 (2017).
  9. S. McDonald, S. Jeon, and C. Gale, Phys. Rev. C 108, 064910 (2023).
  10. A. Ipp, M. Leuthner, D. I. Müller, S. Schlichting, K. Schmidt, and P. Singh, Phys. Rev. D 109, 094040 (2024).
  11. M. Kuha, J. Auvinen, K. J. Eskola, H. Hirvonen, Y. Kanakubo, and H. Niemi, Phys. Rev. C 111, 054914 (2025).
  12. H. Hirvonen, M. Kuha, J. Auvinen, K. J. Eskola, Y. Kanakubo, and H. Niemi, Phys. Rev. C 110, 034911 (2024).
  13. C. Shen, Z. Qiu, H. Song, J. Bernhard, S. Bass, and U. Heinz, Comput. Phys. Commun. 199, 61 (2016).
  14. B. Schenke, S. Jeon, and C. Gale, Phys. Rev. C 82, 014903 (2010).
  15. B. Schenke, S. Jeon, and C. Gale, Phys. Rev. Lett. 106, 042301 (2011).
  16. G. Nijs, W. van der Schee, U. Gürsoy, and R. Snellings, Phys. Rev. C 103, 054909 (2021).
  17. S. A. Bass et al., Prog. Part. Nucl. Phys. 41, 255 (1998).
  18. M. Bleicher et al., J. Phys. G 25, 1859 (1999).
  19. A. Wergieluk et al., smash-transport/smash: Smash-3.1, 10.5281/zenodo.10707746 (2024).
  20. J. Weil et al. (SMASH Collaboration), Phys. Rev. C 94, 054905 (2016).
  21. T. Sjostrand, S. Mrenna, and P. Z. Skands, J. High Energy Phys. 05 (2006) 026.
  22. T. Sjostrand, S. Mrenna, and P. Z. Skands, Comput. Phys. Commun. 178, 852 (2008).
  23. M. L. Miller, K. Reygers, S. J. Sanders, and P. Steinberg, Annu. Rev. Nucl. Part. Sci. 57, 205 (2007).
  24. J. S. Moreland, J. E. Bernhard, and S. A. Bass, Phys. Rev. C 92, 011901 (2015).
  25. J.-P. Blaizot, W. Broniowski, and J.-Y. Ollitrault, Phys. Lett. B 738, 166 (2014).
  26. H. Grönqvist, J.-P. Blaizot, and J.-Y. Ollitrault, Phys. Rev. C 94, 034905 (2016).
  27. W. Broniowski, W. Florkowski, M. Chojnacki, and A. Kisiel, Phys. Rev. C 80, 034902 (2009).
  28. J. Liu, C. Shen, and U. Heinz, Phys. Rev. C 91, 064906 (2015); 92, 049904(E) (2015).
  29. J. Vredevoogd and S. Pratt, Phys. Rev. C 79, 044915 (2009).
  30. W. van der Schee, P. Romatschke, and S. Pratt, Phys. Rev. Lett. 111, 222302 (2013).
  31. P. Romatschke, Eur. Phys. J. C 75, 305 (2015).
  32. A. Kurkela, A. Mazeliauskas, J.-F. Paquet, S. Schlichting, and D. Teaney, Phys. Rev. C 99, 034910 (2019).
  33. A. Kurkela, A. Mazeliauskas, J.-F. Paquet, S. Schlichting, and D. Teaney, Phys. Rev. Lett. 122, 122302 (2019).
  34. X.-Y. Wu, L. Du, C. Gale, and S. Jeon, Phys. Rev. C 110, 054904 (2024).
  35. O. Garcia-Montero, A. Mazeliauskas, P. Plaschke, and S. Schlichting, J. High Energy Phys. 03 (2024) 053.
  36. O. Garcia-Montero, P. Plaschke, and S. Schlichting, Phys. Rev. D 111, 034036 (2025).
  37. B. Schenke, C. Shen, and D. Teaney, Phys. Rev. C 102, 034905 (2020).
  38. T. Nunes da Silva, D. Chinellato, M. Hippert, W. Serenone, J. Takahashi, G. S. Denicol, M. Luzum, and J. Noronha, Phys. Rev. C 103, 054906 (2021).
  39. A. Kurkela and Y. Zhu, Phys. Rev. Lett. 115, 182301 (2015).
  40. G. Giacalone, A. Mazeliauskas, and S. Schlichting, Phys. Rev. Lett. 123, 262301 (2019).
  41. A. Kurkela, Nucl. Phys. A956, 136 (2016).
  42. S. Kamata, M. Martinez, P. Plaschke, S. Ochsenfeld, and S. Schlichting, Phys. Rev. D 102, 056003 (2020).
  43. L. Keegan, A. Kurkela, A. Mazeliauskas, and D. Teaney, J. High Energy Phys. 08 (2016) 171.
  44. M. A. York and G. D. Moore, Phys. Rev. D 79, 054011 (2009).
  45. D. Dash, S. Jaiswal, S. Bhadury, and A. Jaiswal, Phys. Rev. C 108, 064913 (2023).
  46. A. Jaiswal, Phys. Rev. C 87, 051901 (2013).
  47. P. B. Arnold, G. D. Moore, and L. G. Yaffe, J. High Energy Phys. 01 (2003) 030.
  48. X. Du and S. Schlichting, Phys. Rev. D 104, 054011 (2021).
  49. X. Du and S. Schlichting, Phys. Rev. Lett. 127, 122301 (2021).
  50. T. Dore, X. Du, S. Schlichting, and J. Zhu (to be published).
  51. X. Du, S. Ochsenfeld, and S. Schlichting, Phys. Lett. B 845, 138161 (2023).
  52. J. Zhu, KøMPøST-3D, https://github.com/KMPST/KoMPoST-3D (2026) (accessed: 2026-04-20).
  53. L. Pang, Q. Wang, and X.-N. Wang, Phys. Rev. C 86, 024911 (2012).
  54. L.-G. Pang, H. Petersen, and X.-N. Wang, Phys. Rev. C 97, 064918 (2018).
  55. X.-Y. Wu, G.-Y. Qin, L.-G. Pang, and X.-N. Wang, Phys. Rev. C 105, 034909 (2022).
  56. O. Garcia-Montero, S. Schlichting, and J. Zhu, Phys. Rev. D 111, 076029 (2025).
  57. O. Garcia-Montero, H. Elfner, and S. Schlichting, Phys. Rev. C 109, 044916 (2024).
  58. J. P. Blaizot, F. Gelis, and R. Venugopalan, Nucl. Phys. A743, 57 (2004).
  59. F. Gelis and A. Peshier, Nucl. Phys. A697, 879 (2002).
  60. F. Gelis and A. Peshier, Nucl. Phys. A707, 175 (2002).
  61. A. Dumitru and L. D. McLerran, Nucl. Phys. A700, 492 (2002).
  62. T. Lappi and S. Schlichting, Phys. Rev. D 97, 034034 (2018).
  63. A. Dumitru and J. Jalilian-Marian, Phys. Rev. Lett. 89, 022301 (2002).
  64. A. Dumitru, A. Hayashigaki, and J. Jalilian-Marian, Nucl. Phys. A765, 464 (2006).
  65. H. Kowalski, L. Motyka, and G. Watt, Phys. Rev. D 74, 074016 (2006).
  66. H. Kowalski and D. Teaney, Phys. Rev. D 68, 114005 (2003).
  67. G. S. Denicol, C. Gale, S. Jeon, A. Monnai, B. Schenke, and C. Shen, Phys. Rev. C 98, 034916 (2018).
  68. G. S. Denicol, S. Jeon, and C. Gale, Phys. Rev. C 90, 024912 (2014).
  69. A. Bazavov et al. (HotQCD Collaboration), Phys. Rev. D 90, 094503 (2014).
  70. S. Borsanyi et al., Nature (London) 539, 69 (2016).
  71. P. Huovinen and H. Petersen, Eur. Phys. J. A 48, 171 (2012).
  72. N. Borghini, R. Krupczak, and H. Roch, Eur. Phys. J. C 84, 1128 (2024).
  73. T. N. da Silva, D. D. Chinellato, A. V. Giannini, M. N. Ferreira, G. S. Denicol, M. Hippert, M. Luzum, J. Noronha, and J. Takahashi (ExTrEMe Collaboration), Phys. Rev. C 107, 044901 (2023).
  74. P. Romatschke, Phys. Rev. Lett. 120, 012301 (2018).
  75. M. Strickland, J. High Energy Phys. 12 (2018) 128.
  76. C. Chattopadhyay, S. Jaiswal, L. Du, U. Heinz, and S. Pal, Phys. Lett. B 824, 136820 (2022).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation