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

Gravitational waves of GUT phase transition during inflation

Xi-He Hu1,2,3,* and Ye-Ling Zhou1,†

  • *Contact author: huxihe23@mails.ucas.ac.cn
  • †Contact author: zhouyeling@ucas.ac.cn

Phys. Rev. D 111, 115003 – Published 6 June, 2025

DOI: https://doi.org/10.1103/kbzd-kgdr

Abstract

Grand unified theory (GUT) phase transition is generally considered unobservable due to its ultrahigh energy scale, and the monopole problem associated with GUT phase transition is one motivation of inflation. We propose that if a first-order GUT phase transition happens during inflation, the induced gravitational waves (GWs) are redshifted and deformed, and might be observed today in GW observatories. We review the formalism of inflated GWs and derive the general deformation function between inflated and uninflated GW spectra in the instant-source or transitory-source application. It is valid for any e-folding number of instant or transitory source. Applying the formalism to GUT phase transition, we find that the e-folding number at 15 or 25 can shift the GWs to 10 Hz or mHz hands, respectively, which might be tested in the future ground-based or space-based interferometers. We further generalise the discussion to inflated GWs via phase transition below the GUT scale. It is worth mentioning that, due to the deformation of the spectrum, the peak of inflated GWs is not simply a redshift of the peak of uninflated GWs.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (62)

  1. A. M. Polyakov, JETP Lett. 20, 194 (1974).
  2. G. ’t Hooft, Nucl. Phys. B79, 276 (1974).
  3. T. W. B. Kibble, J. Phys. A 9, 1387 (1976).
  4. Y. B. Zeldovich and M. Y. Khlopov, Phys. Lett. 79B, 239 (1978).
  5. J. Preskill, Phys. Rev. Lett. 43, 1365 (1979).
  6. A. H. Guth, Phys. Rev. D 23, 347 (1981).
  7. A. D. Linde, Phys. Lett. 108B, 389 (1982).
  8. A. Albrecht and P. J. Steinhardt, Phys. Rev. Lett. 48, 1220 (1982).
  9. S. F. King, S. Pascoli, J. Turner, and Y.-L. Zhou, Phys. Rev. Lett. 126, 021802 (2021).
  10. J. A. Dror, T. Hiramatsu, K. Kohri, H. Murayama, and G. White, Phys. Rev. Lett. 124, 041804 (2020).
  11. S. F. King, S. Pascoli, J. Turner, and Y.-L. Zhou, J. High Energy Phys. 10 (2021) 225.
  12. S. Bertolini, L. Di Luzio, and M. Malinsky, Phys. Rev. D 80, 015013 (2009).
  13. J. Chakrabortty, R. Maji, and S. F. King, Phys. Rev. D 99, 095008 (2019).
  14. D. Meloni, T. Ohlsson, and M. Pernow, Eur. Phys. J. C 80, 840 (2020).
  15. S. Antusch, K. Hinze, S. Saad, and J. Steiner, Phys. Rev. D 108, 095053 (2023).
  16. W. Buchmuller, V. Domcke, H. Murayama, and K. Schmitz, Phys. Lett. B 809, 135764 (2020).
  17. W. Buchmuller, V. Domcke, and K. Schmitz, Phys. Lett. B 811, 135914 (2020).
  18. W. Buchmuller, V. Domcke, and K. Schmitz, J. Cosmol. Astropart. Phys. 12 (2021) 006.
  19. M. A. Masoud, M. U. Rehman, and Q. Shafi, J. Cosmol. Astropart. Phys. 11 (2021) 022.
  20. B. Fu, S. F. King, L. Marsili, S. Pascoli, J. Turner, and Y.-L. Zhou, Phys. Rev. D 109, 055025 (2024).
  21. G. Lazarides, R. Maji, A. Moursy, and Q. Shafi, J. Cosmol. Astropart. Phys. 03 (2024) 006.
  22. S. F. King, G. K. Leontaris, and Y.-L. Zhou, J. High Energy Phys. 03 (2024) 006.
  23. D. Croon, T. E. Gonzalo, and G. White, J. High Energy Phys. 02 (2019) 083.
  24. W.-C. Huang, F. Sannino, and Z.-W. Wang, Phys. Rev. D 102, 095025 (2020).
  25. P. Athron, C. Balázs, T. E. Gonzalo, and M. Pearce, Phys. Rev. D 109, L061303 (2024).
  26. V. Brdar, L. Graf, A. J. Helmboldt, and X.-J. Xu, J. Cosmol. Astropart. Phys. 12 (2019) 027.
  27. M. Li, Q.-S. Yan, Y. Zhang, and Z. Zhao, J. High Energy Phys. 03 (2021) 267.
  28. H. An, K.-F. Lyu, L.-T. Wang, and S. Zhou, Chin. Phys. C 46, 101001 (2022).
  29. H. An, K.-F. Lyu, L.-T. Wang, and S. Zhou, J. High Energy Phys. 06 (2022) 050.
  30. H. An, B. Su, H. Tai, L.-T. Wang, and C. Yang, Phys. Rev. D 109, L121304 (2024).
  31. H. Jiang, T. Liu, S. Sun, and Y. Wang, Phys. Lett. B 765, 339 (2017).
  32. Q. Shafi and A. Vilenkin, Phys. Rev. Lett. 52, 691 (1984).
  33. G. Lazarides and C. Panagiotakopoulos, Phys. Rev. D 52, R559 (1995).
  34. C. Caprini et al., J. Cosmol. Astropart. Phys. 04 (2016) 001.
  35. D. J. Weir, Phil. Trans. R. Soc. A 376, 20170126 (2018); 381, 20230212(E) (2023).
  36. L. Bian et al., Sci. China Phys. Mech. Astron. 64, 120401 (2021).
  37. P. Athron, C. Balázs, A. Fowlie, L. Morris, and L. Wu, Prog. Part. Nucl. Phys. 135, 104094 (2024).
  38. A. Kosowsky, M. S. Turner, and R. Watkins, Phys. Rev. D 45, 4514 (1992).
  39. A. Kosowsky, M. S. Turner, and R. Watkins, Phys. Rev. Lett. 69, 2026 (1992).
  40. A. Kosowsky and M. S. Turner, Phys. Rev. D 47, 4372 (1993).
  41. M. Kamionkowski, A. Kosowsky, and M. S. Turner, Phys. Rev. D 49, 2837 (1994).
  42. S. J. Huber and T. Konstandin, J. Cosmol. Astropart. Phys. 09 (2008) 022.
  43. C. Caprini, R. Durrer, T. Konstandin, and G. Servant, Phys. Rev. D 79, 083519 (2009).
  44. R.-G. Cai, S. Pi, and M. Sasaki, Phys. Rev. D 102, 083528 (2020).
  45. P. Amaro-Seoane et al. (LISA Collaboration), arXiv:1702.00786.
  46. W.-H. Ruan, Z.-K. Guo, R.-G. Cai, and Y.-Z. Zhang, Int. J. Mod. Phys. A 35, 2050075 (2020).
  47. J. Luo et al. (TianQin Collaboration), Classical Quantum Gravity 33, 035010 (2016).
  48. V. Corbin and N. J. Cornish, Classical Quantum Gravity 23, 2435 (2006).
  49. N. Seto, S. Kawamura, and T. Nakamura, Phys. Rev. Lett. 87, 221103 (2001).
  50. A. Sesana et al., Exp. Astron. 51, 1333 (2021).
  51. P. W. Graham, J. M. Hogan, M. A. Kasevich, S. Rajendran, and R. W. Romani (MAGIS Collaboration), arXiv:1711.02225.
  52. Y. A. El-Neaj et al. (AEDGE Collaboration), Eur. Phys. J. Quantum Technol. 7, 6 (2020).
  53. L. Badurina et al., J. Cosmol. Astropart. Phys. 05 (2020) 011.
  54. B. Sathyaprakash et al., Classical Quantum Gravity 29, 124013 (2012); 30, 079501(E) (2013).
  55. B. P. Abbott et al. (LIGO Scientific Collaboration), Classical Quantum Gravity 34, 044001 (2017).
  56. G. Janssen et al., Proc. Sci. AASKA14 (2015) 037 [arXiv:1501.00127].
  57. A. Afzal et al. (NANOGrav Collaboration), Astrophys. J. Lett. 951, L11 (2023); 971, L27(E) (2024).
  58. R. Abbott et al. (LIGO Scientific, Virgo, and KAGRA Collaborations), Phys. Rev. Lett. 126, 241102 (2021).
  59. R. Jeannerot, S. Khalil, G. Lazarides, and Q. Shafi, J. High Energy Phys. 10 (2000) 012.
  60. R. Jeannerot, J. Rocher, and M. Sakellariadou, Phys. Rev. D 68, 103514 (2003).
  61. J. Chakrabortty, G. Lazarides, R. Maji, and Q. Shafi, J. High Energy Phys. 02 (2021) 114.
  62. R. Maji and Q. Shafi, J. Cosmol. Astropart. Phys. 03 (2023) 007.

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation