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

Is it worth the effort to find Lefschetz thimbles? Integration contours with numerically optimal signal-to-noise ratios in simple fermionic toy models

Attila Pásztor1,2 and Dávid Pesznyák1,2,3,4,*

  • *Contact author: dpesznyak@student.elte.hu

Phys. Rev. D 113, 014506 – Published 21 January, 2026

DOI: https://doi.org/10.1103/fywf-77b4

Abstract

We perform a detailed analysis of the fermionic sign problem in a series of one-dimensional integrals, that are achieved as extreme (one-site) limits of genuine physics models. Altogether we studied a Hubbard-like, a Gross-Neveu-like, a Thirring-like, and a Chern-Simons-like integral. We compare the Lefschetz-thimble structure for these integrals with contours obtained with the holomorphic flow equations at different flow times and with numerically optimized continuous integration contours, defined by a maximal value of the expectation values of the phases. With the holomorphic flow equation, we perform the large flow-time limit, so that the average phase corresponds to its value on the thimbles. In all of these integrals we observe that the convergence to this value is not monotonic, meaning that there is an optimal flow time where the sign problem is weaker than it is on the thimbles. Furthermore, we find that for all of these toy models, numerical optimization can find continuous contours on which the sign problem is considerably weaker than it is both on the thimbles and at flowed integration contours at the optimal flow time.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (53)

  1. A. Alexandru, G. Basar, P. F. Bedaque, and N. C. Warrington, Rev. Mod. Phys. 94, 015006 (2022).
  2. M. Cristoforetti, F. Di Renzo, and L. Scorzato (Aurora Science Collaboration), Phys. Rev. D 86, 074506 (2012).
  3. M. Cristoforetti, F. Di Renzo, A. Mukherjee, and L. Scorzato, Phys. Rev. D 88, 051501 (2013).
  4. H. Fujii, D. Honda, M. Kato, Y. Kikukawa, S. Komatsu, and T. Sano, J. High Energy Phys. 10 (2013) 147.
  5. A. Alexandru, G. Basar, and P. Bedaque, Phys. Rev. D 93, 014504 (2016).
  6. H. Fujii, S. Kamata, and Y. Kikukawa, J. High Energy Phys. 11 (2015) 078; 02 (2016) 036(E).
  7. F. Di Renzo and G. Eruzzi, Phys. Rev. D 92, 085030 (2015).
  8. F. Di Renzo and G. Eruzzi, Phys. Rev. D 97, 014503 (2018).
  9. M. Ulybyshev, C. Winterowd, and S. Zafeiropoulos, Phys. Rev. D 101, 014508 (2020).
  10. F. Di Renzo, S. Singh, and K. Zambello, Phys. Rev. D 103, 034513 (2021).
  11. T. Kanazawa and Y. Tanizaki, J. High Energy Phys. 03 (2015) 044.
  12. Y. Tanizaki, Y. Hidaka, and T. Hayata, New J. Phys. 18, 033002 (2016).
  13. G. Parisi, Phys. Lett. 131B, 393 (1983).
  14. P. H. Damgaard and H. Huffel, Phys. Rep. 152, 227 (1987).
  15. G. Aarts and I.-O. Stamatescu, J. High Energy Phys. 09 (2008) 018.
  16. A. Mollgaard and K. Splittorff, Phys. Rev. D 88, 116007 (2013).
  17. G. Aarts, E. Seiler, D. Sexty, and I.-O. Stamatescu, J. High Energy Phys. 05 (2017) 044; 01 (2018) 128(E).
  18. E. Seiler, D. Sexty, and I.-O. Stamatescu, Phys. Rev. D 109, 014509 (2024).
  19. G. Aarts, E. Seiler, and I.-O. Stamatescu, Phys. Rev. D 81, 054508 (2010).
  20. G. Aarts, F. A. James, E. Seiler, and I.-O. Stamatescu, Eur. Phys. J. C 71, 1756 (2011).
  21. G. Aarts, L. Bongiovanni, E. Seiler, and D. Sexty, J. High Energy Phys. 10 (2014) 159.
  22. K. Boguslavski, P. Hotzy, and D. I. Müller, Proc. Sci. LATTICE2024 (2025) 026.
  23. A. Alexandru, G. Basar, P. F. Bedaque, G. W. Ridgway, and N. C. Warrington, J. High Energy Phys. 05 (2016) 053.
  24. Y. Tanizaki, H. Nishimura, and J. J. M. Verbaarschot, J. High Energy Phys. 10 (2017) 100.
  25. M. Fukuma and N. Umeda, Prog. Theor. Exp. Phys. 2017, 073B01 (2017).
  26. M. Fukuma and N. Matsumoto, Prog. Theor. Exp. Phys. 2021, 023B08 (2021).
  27. A. Alexandru, G. Basar, P. F. Bedaque, G. W. Ridgway, and N. C. Warrington, Phys. Rev. D 93, 094514 (2016).
  28. A. Alexandru, P. F. Bedaque, H. Lamm, and S. Lawrence, Phys. Rev. D 96, 094505 (2017).
  29. J.-L. Wynen, E. Berkowitz, S. Krieg, T. Luu, and J. Ostmeyer, Phys. Rev. B 103, 125153 (2021).
  30. S. Lawrence, Proc. Sci. LATTICE2018 (2018) 149 [arXiv:1810.06529].
  31. S. Lawrence and Y. Yamauchi, Phys. Rev. D 110, 014508 (2024).
  32. S. Lawrence and Y. Yamauchi, Phys. Rev. D 103, 114509 (2021).
  33. W. Detmold, G. Kanwar, M. L. Wagman, and N. C. Warrington, Phys. Rev. D 102, 014514 (2020).
  34. W. Detmold, G. Kanwar, H. Lamm, M. L. Wagman, and N. C. Warrington, Phys. Rev. D 103, 094517 (2021).
  35. Y. Lin, W. Detmold, G. Kanwar, P. E. Shanahan, and M. L. Wagman, Proc. Sci. LATTICE2023 (2024) 043.
  36. Y. Mori, K. Kashiwa, and A. Ohnishi, Phys. Rev. D 96, 111501 (2017).
  37. F. Bursa and M. Kroyter, J. High Energy Phys. 12 (2018) 054.
  38. F. Bursa and M. Kroyter, J. High Energy Phys. 04 (2021) 181.
  39. K. Kashiwa, Y. Mori, and A. Ohnishi, Phys. Rev. D 99, 014033 (2019).
  40. Y. Mori, K. Kashiwa, and A. Ohnishi, Prog. Theor. Exp. Phys. 2019, 113B01 (2019).
  41. A. Alexandru, P. F. Bedaque, H. Lamm, and S. Lawrence, Phys. Rev. D 97, 094510 (2018).
  42. A. Alexandru, P. F. Bedaque, H. Lamm, S. Lawrence, and N. C. Warrington, Phys. Rev. Lett. 121, 191602 (2018).
  43. K. Kashiwa and Y. Mori, Phys. Rev. D 102, 054519 (2020).
  44. M. Giordano, A. Pasztor, D. Pesznyak, and Z. Tulipant, Phys. Rev. D 108, 094507 (2023).
  45. Z. Tulipant, M. Giordano, K. Kapas, S. D. Katz, and A. Pasztor, Phys. Rev. D 106, 054512 (2022).
  46. S. Lawrence, Proc. Sci. LATTICE2024 (2025) 010 [arXiv:2502.02670].
  47. J.-L. Wynen, E. Berkowitz, C. Körber, T. A. Lähde, and T. Luu, Phys. Rev. B 100, 075141 (2019).
  48. J. Ostmeyer, E. Berkowitz, S. Krieg, T. A. Lähde, T. Luu, and C. Urbach, Phys. Rev. B 102, 245105 (2020).
  49. M. Rodekamp, E. Berkowitz, C. Gäntgen, S. Krieg, T. Luu, and J. Ostmeyer, Phys. Rev. B 106, 125139 (2022).
  50. C. Gäntgen, E. Berkowitz, T. Luu, J. Ostmeyer, and M. Rodekamp, Phys. Rev. B 109, 195158 (2024).
  51. D. P. Kingma and J. Ba, arXiv:1412.6980.
  52. D. J. Gross and A. Neveu, Phys. Rev. D 10, 3235 (1974).
  53. G. V. Dunne, K.-M. Lee, and C.-h. Lu, Phys. Rev. Lett. 78, 3434 (1997).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation