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
  • Letter
  • Open Access

Discovery prospects for electron and neutron electric dipole moments in the general two Higgs doublet model

Wei-Shu Hou, Girish Kumar, and Sven Teunissen

  • Department of Physics, National Taiwan University, Taipei 10617, Taiwan

Phys. Rev. D 109, L011703 – Published 16 January, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.L011703

Abstract

Baryon asymmetry of the Universe offers one of the strongest hints for physics beyond the Standard Model (BSM). Remarkably, in the general two Higgs doublet model (g2HDM) that possesses a second set of Yukawa matrices, one can have electroweak baryogenesis (EWBG) while the electron electric dipole moment (eEDM) is evaded by a natural flavor tuning that echoes the Standard Model (SM). We show that eEDM may first emerge around 10−30  e cm or so, followed by neutron EDM (nEDM) down to 10−27  e cm. We illustrate a cancellation mechanism for nEDM itself, which in turn can be probed when a facility capable of pushing down to 10−28  e cm becomes available.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (43)

  1. R. L. Workman et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2022, 083C01 (2022).
  2. ACME Collaboration, Nature (London) 562, 355 (2018).
  3. T. S. Roussy et al., Science 381, 46 (2023).
  4. C. Abel et al. (nEDM Collaboration), Phys. Rev. Lett. 124, 081803 (2020).
  5. R. Alarcon et al., arXiv:2203.08103.
  6. See e.g. G. C. Branco, P. M. Ferreira, L. Lavoura, M. N. Rebelo, M. Sher, and J. P. Silva, Phys. Rep. 516, 1 (2012).
  7. S. L. Glashow and S. Weinberg, Phys. Rev. D 15, 1958 (1977).
  8. T. P. Cheng and M. Sher, Phys. Rev. D 35, 3484 (1987).
  9. W.-S. Hou, Phys. Lett. B 296, 179 (1992).
  10. A. Tumasyan et al. (CMS Collaboration), Phys. Rev. Lett. 129, 032001 (2022).
  11. K.-F. Chen, W.-S. Hou, C. Kao, and M. Kohda, Phys. Lett. B 725, 378 (2013).
  12. K. Fuyuto, W.-S. Hou, and E. Senaha, Phys. Lett. B 776, 402 (2018).
  13. V. A. Kuzmin, V. A. Rubakov, and M. E. Shaposhnikov, Phys. Lett. 155B, 36 (1985); for some reviews see, e.g., V. A. Rubakov and M. E. Shaposhnikov, Usp. Fiz. Nauk 166, 493 (1996); K. Funakubo, Prog. Theor. Phys. 96, 475 (1996); D. E. Morrissey and M. J. Ramsey-Musolf, New J. Phys. 14, 125003 (2012).
  14. S. Kanemura, Y. Okada, and E. Senaha, Phys. Lett. B 606, 361 (2005).
  15. W.-S. Hou and M. Kikuchi, Europhys. Lett. 123, 11001 (2018).
  16. M. Kohda, T. Modak, and W.-S. Hou, Phys. Lett. B 776, 379 (2018).
  17. D. K. Ghosh, W.-S. Hou, and T. Modak, Phys. Rev. Lett. 125, 221801 (2020).
  18. W.-S. Hou and T. Modak, Mod. Phys. Lett. A 36, 2130006 (2021).
  19. G. Aad et al. (ATLAS Collaboration), arXiv:2307.14759.
  20. A. Hayrapetyan et al. (CMS Collaboration), arXiv:2311.03261.
  21. S. M. Barr and A. Zee, Phys. Rev. Lett. 65, 21 (1990).
  22. K. Fuyuto, W.-S. Hou, and E. Senaha, Phys. Rev. D 101, 011901 (2020).
  23. W.-S. Hou, Chin. J. Phys. 77, 432 (2022).
  24. S. Davidson and H. E. Haber, Phys. Rev. D 72, 035004 (2005).
  25. W.-S. Hou and G. Kumar, Phys. Rev. D 102, 115017 (2020).
  26. M. Pospelov and A. Ritz, Ann. Phys. (Amsterdam) 318, 119 (2005).
  27. J. Hisano, D. Kobayashi, W. Kuramoto, and T. Kuwahara, J. High Energy Phys. 11 (2015) 085.
  28. K. Kaneta, N. Nagata, K. A. Olive, M. Pospelov, and L. Velasco-Sevilla, J. High Energy Phys. 03 (2023) 250.
  29. T. Abe, J. Hisano, T. Kitahara, and K. Tobioka, J. High Energy Phys. 01 (2014) 106.
  30. M. Jung and A. Pich, J. High Energy Phys. 04 (2014) 076.
  31. N. J. Ayres et al. (n2EDM Collaboration), Eur. Phys. J. C 81, 512 (2021).
  32. See the webpage https://nedm.ornl.gov/.
  33. D. Gonçalves, K. Kong, and J. H. Kim, J. High Energy Phys. 06 (2018) 079.
  34. K. Cheung, A. Jueid, Y. N. Mao, and S. Moretti, Phys. Rev. D 102, 075029 (2020).
  35. D. Gonçalves, J. H. Kim, K. Kong, and Y. Wu, J. High Energy Phys. 01 (2022) 158.
  36. K. Enomoto, S. Kanemura, and Y. Mura, J. High Energy Phys. 09 (2022) 121.
  37. W.-S. Hou, M. Kohda, and T. Modak, Phys. Rev. D 98, 075007 (2018).
  38. A. Tumasyan et al. (CMS Collaboration), J. High Energy Phys. 06 (2023) 081; 07 (2023) 023.
  39. J.-M. Gerard and M. Herquet, Phys. Rev. Lett. 98, 251802 (2007).
  40. W.-S. Hou, R. Jain, and C. Kao, Eur. Phys. J. C 83, 1112 (2023).
  41. W.-S. Hou, G. Kumar, and T. Modak, arXiv:2302.08847.
  42. H. Albrecht et al. (ARGUS Collaboration), Phys. Lett. B 192, 245 (1987).
  43. A. Bean et al. (CLEO Collaboration), Phys. Rev. Lett. 58, 183 (1987).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation