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

Matter-dark matter coincidence and the mirror world

Rabindra N. Mohapatra1 and Nobuchika Okada2

Phys. Rev. D 111, 123510 – Published 9 June, 2025

DOI: https://doi.org/10.1103/jwxp-dzlj

Abstract

Why matter and dark matter contents of the Universe are of the same order of magnitude, is one of the puzzles of modern cosmology. At the face of it, this would seem to point toward a basic similarity between matter and dark matter, suggesting perhaps the widely discussed mirror world picture as an ideal setting for a discussion of this issue. Here we outline a new and simple mirror world scenario to explain this puzzle. Our model uses the Affleck-Dine mechanism to generate baryon asymmetry and dark matter relic density leading to an asymmetric dark matter picture. We find that, for a certain parameter range of the model, the mirror electron is the unique possibility for dark matter whereas, in the complementary parameter range, the mirror baryons constitute the dark matter. In either case, the mirror photon must have mass in the MeV range for consistency with observations. For the case of mirror electron dark matter, the model predicts a lower bound on the amount of dark radiation, i.e., ΔNeff≥0.007.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (60)

  1. T. D. Lee and C. N. Yang, Phys. Rev. 104, 254 (1956).
  2. I. Yu. Kobzarev, L. B. Okun, and I. Ya. Pomeranchuk, Yad. Fiz. 3, 1154 (1966) [Sov. J. Nucl. Phys. 3, 837 (1966)].
  3. M. Pavsic, Int. J. Theor. Phys. 9, 229 (1974).
  4. L. B. Okun, JETP 79, 694 (1980).
  5. S. Blinnikov and M. Khlopov, Sov. Astron. 27, 371 (1983).
  6. R. Foot, H. Lew, and R. R. Volkas, Phys. Lett. B 272, 67 (1991); Mod. Phys. Lett. A 07, 2567 (1992).
  7. R. Foot and R. Volkas, Phys. Rev. D 52, 6595 (1995).
  8. Z. Berezhiani and R. N. Mohapatra, Phys. Rev. D 52, 6607 (1995).
  9. Z. Chacko, H.-S. Goh, and R. Harnik, Phys. Rev. Lett. 96, 231802 (2006).
  10. Z. Berezhiani, D. Comelli, and F. L. Villante, Phys. Lett. B 503, 362 (2001);
  11. Z. Berezhiani, Int. J. Mod. Phys. A 19, 3775 (2004).
  12. Z. Berezhiani, Int. J. Mod. Phys. A 33, 1844034 (2018).
  13. E. W. Kolb, D. Seckel, and M. S. Turner, Nature (London) 314, 415 (1985).
  14. H. M. Hodges, Phys. Rev. D 47, 456 (1993).
  15. Z. G. Berezhiani, A. D. Dolgov, and R. N. Mohapatra, Phys. Lett. B 375, 26 (1996).
  16. V. S. Berezinsky and A. Vilenkin, Phys. Rev. D 62, 083512 (2000).
  17. J. M. Cline and J. S. Roux, Phys. Rev. D 105, 043506 (2022).
  18. Z. Chacko, N. Craig, P. J. Fox, and R. Harnik, J. High Energy Phys. 07 (2017) 023.
  19. S. Nussinov, Phys. Lett. 165B, 55 (1985).
  20. S. M. Barr, R. S. Chivukula, and E. Farhi, Phys. Lett. B 241, 387 (1990).
  21. D. E. Kaplan, M. A. Luty, and K. M. Zurek, Phys. Rev. D 79, 115016 (2009).
  22. H. Davoudiasl and R. N. Mohapatra, New J. Phys. 14, 095011 (2012).
  23. K. Petraki and R. R. Volkas, Int. J. Mod. Phys. A 28, 1330028 (2013).
  24. K. M. Zurek, Phys. Rep. 537, 91 (2014).
  25. L. Bento and Z. Berezhiani, Phys. Rev. Lett. 87, 231304 (2001).
  26. H. An, S. L. Chen, R. N. Mohapatra, and Y. Zhang, J. High Energy Phys. 03 (2010) 124.
  27. Y. Cui and R. Sundrum, Phys. Rev. D 87, 116013 (2013).
  28. Tetsutaro Higaki, Kwang Sik Jeong, and Fuminobu Takahashi, J. Cosmol. Astropart. Phys. 08 (2013) 031.
  29. Shreyashi Chakdar, Kirtiman Ghosh, and S. Nandi, Phys. Lett. B 732, 343 (2014).
  30. W. Z. Feng and P. Nath, Phys. Lett. B 731, 43 (2014).
  31. M. Farina, J. Cosmol. Astropart. Phys. 11 (2015) 017.
  32. M. Farina, A. Monteux, and C. S. Shin, Phys. Rev. D 94, 035017 (2016).
  33. A. Bodas, M. A. Buen-Abad, A. Hook, and R. Sundrum, J. High Energy Phys. 06 (2024) 052.
  34. S. J. Lonsdale and R. R. Volkas, Phys. Rev. D 90, 083501 (2014); 91, 129906(E) (2015).
  35. M. Ibe, A. Kamada, S. Kobayashi, T. Kuwahara, and W. Nakano, Phys. Rev. D 100, 075022 (2019).
  36. G. Alonso-Alvarez, D. Curtin, A. Rasovic, and Z. Yuan, J. High Energy Phys. 05 (2024) 069.
  37. P. Bittar, G. Burdman, and L. Kiriliuk, J. High Energy Phys. 11 (2023) 043.
  38. C. Murgui and K. M. Zurek, Phys. Rev. D 105, 095002 (2022).
  39. Yi Chung, arXiv:2411.16860.
  40. D. Borah, S. J. Das, and N. Okada, J. High Energy Phys. 05 (2023) 004.
  41. D. Brzeminski and A. Hook, Phys. Rev. Lett. 132, 201001 (2024).
  42. A. Banerjee, D. Brzeminski, and A. Hook, arXiv:2410.22412.
  43. I. Affleck and M. Dine, Nucl. Phys. B249, 361 (1985).
  44. D. N. Spergel and P. J. Steinhardt, Phys. Rev. Lett. 84, 3760 (2000).
  45. S. Tulin and H. B. Yu, Phys. Rep. 730, 1 (2018).
  46. S. Tulin, H. B. Yu, and K. M. Zurek, Phys. Rev. D 87, 115007 (2013).
  47. A. Lloyd-Stubbs and J. McDonald, Phys. Rev. D 103, 123514 (2021).
  48. E. Babichev, D. Gorbunov, and S. Ramazanov, Phys. Lett. B 792, 228 (2019).
  49. J. M. Cline, M. Puel, and T. Toma, Phys. Rev. D 101, 043014 (2020).
  50. M. P. Hertzberg and J. Karouby, Phys. Lett. B 737, 34 (2014).
  51. R. N. Mohapatra and N. Okada, Phys. Rev. D 104, 055030 (2021).
  52. F. L. Bezrukov and M. Shaposhnikov, Phys. Lett. B 659, 703 (2008).
  53. Q. Bonnefoy, L. J. Hall, C. A. Manzari, A. McCune, and C. Scherb, Phys. Rev. D 109, 055045 (2024).
  54. D. I. Dunsky, L. J. Hall, and K. Harigaya, J. High Energy Phys. 02 (2024) 212.
  55. Michele Redi and Andrea Tesi, J. High Energy Phys. 11 (2023) 211.
  56. N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641, A6 (2020); 652, C4(E) (2021).
  57. Z. Chacko, Y. Cui, S. Hong, and T. Okui, Phys. Rev. D 92, 055033 (2015).
  58. K. N. Abazajian et al. (CMB-S4 Collaboration), arXiv:1610.02743.
  59. S. Aiola et al. (CMB-HD Collaboration), arXiv:2203.05728.
  60. M. Markevitch, A. H. Gonzalez, D. Clowe, A. Vikhlinin, L. David, W. Forman, C. Jones, S. Murray, and W. Tucker, Astrophys. J. 606, 819 (2004).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation