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

Spatial confinement-deconfinement transition in accelerated gluodynamics within lattice simulation

Victor V. Braguta1,*, Vladimir A. Goy2,3,†, Jayanta Dey1,‡, and Artem A. Roenko1,§

  • *Contact author: vvbraguta@theor.jinr.ru
  • †Contact author: vovagoy@gmail.com
  • ‡Contact author: jayanta@theor.jinr.ru
  • §Contact author: roenko@theor.jinr.ru

Phys. Rev. D 113, 094507 – Published 28 May, 2026

DOI: https://doi.org/10.1103/cd98-vnvc

Abstract

In this work we investigate the influence of weak acceleration on the confinement-deconfinement phase transition in gluodynamics. Our study is carried out within lattice simulation in the comoving reference frame of accelerated observer which is parametrized by the Rindler coordinates. We find that finite temperature confinement-deconfinement phase transition turns into spatial crossover in the Rindler spacetime. In other words, spatially separated confinement and deconfinement phases can coexist in the Rindler spacetime within certain intervals of temperature and acceleration. We determine the position of the boundary between the phases as a function of temperature for several accelerations and find that it can be described by the Tolman-Ehrenfest law with rather good accuracy although a minor deviation takes place. Moreover, the critical temperature of the system in the weak acceleration regime is found to remain unchanged as that of the standard homogeneous gluodynamics. Our results imply that the spatial confinement-deconfinement transition might take place in the vicinity of the Schwarzschild black hole horizon.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (60)

  1. G. Y. Prokhorov, D. A. Shohonov, O. V. Teryaev, N. S. Tsegelnik, and V. I. Zakharov, Phys. Rev. C 112, 064907 (2025).
  2. D. Kharzeev and K. Tuchin, Nucl. Phys. A753, 316 (2005).
  3. L. C. B. Crispino, A. Higuchi, and G. E. A. Matsas, Rev. Mod. Phys. 80, 787 (2008).
  4. V. Mukhanov and S. Winitzki, Introduction to Quantum Effects in Gravity (Cambridge University Press, Cambridge, England, 2007).
  5. W. Rindler, Am. J. Phys. 34, 1174 (1966).
  6. W. G. Unruh, Phys. Rev. D 14, 870 (1976).
  7. F. Becattini and E. Grossi, Phys. Rev. D 92, 045037 (2015).
  8. G. Y. Prokhorov, O. V. Teryaev, and V. I. Zakharov, Particles 3, 1 (2020).
  9. G. Y. Prokhorov, O. V. Teryaev, and V. I. Zakharov, arXiv:2304.13151.
  10. R. V. Khakimov, G. Y. Prokhorov, O. V. Teryaev, and V. I. Zakharov, Phys. Rev. D 108, L121701 (2023).
  11. V. E. Ambruş and M. N. Chernodub, Phys. Lett. B 855, 138757 (2024).
  12. M. N. Chernodub, V. A. Goy, A. V. Molochkov, D. V. Stepanov, and A. S. Pochinok, Phys. Rev. Lett. 134, 111904 (2025).
  13. E. T. Akhmedov, K. V. Bazarov, and D. V. Diakonov, Phys. Rev. D 104, 085008 (2021).
  14. D. V. Diakonov and K. V. Bazarov, Theor. Math. Phys. 223, 839 (2025).
  15. E. T. Akhmedov and K. Gubarev, Int. J. Mod. Phys. A 39, 2445004 (2024).
  16. M. Selch, R. A. Abramchuk, and M. A. Zubkov, Phys. Rev. D 109, 016003 (2024).
  17. N. Tsegelnik, arXiv:2601.10668.
  18. M. Bordag and D. N. Voskresensky, Phys. Part. Nucl. Lett. 23, 139 (2026).
  19. F. Becattini, Phys. Rev. D 97, 085013 (2018).
  20. F. Becattini, M. Buzzegoli, and A. Palermo, J. High Energy Phys. 02 (2021) 101.
  21. A. Palermo, M. Buzzegoli, and F. Becattini, J. High Energy Phys. 10 (2021) 077.
  22. T. Ohsaku, Phys. Lett. B 599, 102 (2004).
  23. D. Ebert and V. C. Zhukovsky, Phys. Lett. B 645, 267 (2007).
  24. P. Castorina and M. Finocchiaro, J. Mod. Phys. 3, 1703 (2012).
  25. S. Takeuchi, Phys. Lett. B 750, 209 (2015).
  26. S. Benic and K. Fukushima, arXiv:1503.05790.
  27. A. Dobado, Phys. Rev. D 96, 085009 (2017).
  28. A. Casado-Turrión and A. Dobado, Phys. Rev. D 99, 125018 (2019).
  29. W. Kou and X. Chen, Phys. Lett. B 856, 138942 (2024).
  30. M. N. Chernodub, arXiv:2501.16129.
  31. Z.-B. Zhu, H.-L. Chen, and X.-G. Huang, Phys. Rev. D 113, 034005 (2026).
  32. W. G. Unruh and N. Weiss, Phys. Rev. D 29, 1656 (1984).
  33. D. G. Salluce, M. Pasini, A. Flachi, A. Pittelli, and S. Ansoldi, J. High Energy Phys. 05 (2024) 218.
  34. M. Lüscher, J. High Energy Phys. 08 (2010) 071; 03 (2014) 092(E).
  35. R. Tolman and P. Ehrenfest, Phys. Rev. 36, 1791 (1930).
  36. A. Yamamoto and Y. Hirono, Phys. Rev. Lett. 111, 081601 (2013).
  37. V. V. Braguta, A. Y. Kotov, D. D. Kuznedelev, and A. A. Roenko, JETP Lett. 112, 6 (2020).
  38. V. V. Braguta, A. Y. Kotov, D. D. Kuznedelev, and A. A. Roenko, Phys. Rev. D 103, 094515 (2021).
  39. V. V. Braguta, A. Kotov, A. Roenko, and D. Sychev, Proc. Sci. LATTICE2022 (2023) 190 [arXiv:2212.03224].
  40. J.-C. Yang and X.-G. Huang, arXiv:2307.05755.
  41. V. V. Braguta, I. E. Kudrov, A. A. Roenko, D. A. Sychev, and M. N. Chernodub, JETP Lett. 117, 639 (2023).
  42. V. V. Braguta, M. N. Chernodub, and A. A. Roenko, Phys. Lett. B 855, 138783 (2024).
  43. V. V. Braguta, M. N. Chernodub, Y. A. Gershtein, and A. A. Roenko, J. High Energy Phys. 09 (2025) 079.
  44. S. Benić and A. Yamamoto, Phys. Rev. D 93, 094505 (2016).
  45. G. Curci, P. Menotti, and G. Paffuti, Phys. Lett. 130B, 205 (1983); 135B, 516(E) (1984).
  46. M. Luscher and P. Weisz, Phys. Lett. 158B, 250 (1985).
  47. B. Beinlich, F. Karsch, E. Laermann, and A. Peikert, Eur. Phys. J. C 6, 133 (1999).
  48. S. Borsanyi, R. Kara, Z. Fodor, D. A. Godzieba, P. Parotto, and D. Sexty, Phys. Rev. D 105, 074513 (2022).
  49. O. Kaczmarek, F. Karsch, P. Petreczky, and F. Zantow, Phys. Lett. B 543, 41 (2002).
  50. S. Gupta, K. Huebner, and O. Kaczmarek, Phys. Rev. D 77, 034503 (2008).
  51. M. Fukugita, M. Okawa, and A. Ukawa, Nucl. Phys. B337, 181 (1990).
  52. K. Binder and D. P. Landau, Phys. Rev. B 30, 1477 (1984).
  53. B. Svetitsky and L. G. Yaffe, Nucl. Phys. B210, 423 (1982).
  54. J. Engels, S. Mashkevich, T. Scheideler, and G. Zinovev, Phys. Lett. B 365, 219 (1996).
  55. J.-C. Yang, W.-W. Li, and C.-X. Yue, Phys. Rev. D 110, 054509 (2024).
  56. S. W. Hawking, Commun. Math. Phys. 80, 421 (1981).
  57. http://ckp.nrcki.ru/.
  58. A. Anikina, D. Belyakov, T. Bezhanyan, M. Kirakosyan, A. Kokorev, M. Lyubimova, M. Matveev, D. Podgainy, A. Rahmonova, S. Shadmehri, O. Streltsova, S. Torosyan, M. Vala, and M. Zuev, in Distributed Computer and Communication Networks, edited by V. M. Vishnevsky, K. E. Samouylov, and D. V. Kozyrev (Springer Nature, Switzerland, Cham, 2025), pp. 444–457.
  59. J. M. Luttinger, Phys. Rev. 135, A1505 (1964).
  60. P. M. Lo, B. Friman, O. Kaczmarek, K. Redlich, and C. Sasaki, Phys. Rev. D 88, 074502 (2013).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation