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Radiative corrections to neutrino mixing and CP violation in the minimal seesaw model with leptogenesis

Jian-wei Mei* and Zhi-zhong Xing†,‡

  • CCAST (World Laboratory), P. O. Box 8730, Beijing 100080, China
  • Institute of High Energy Physics, Chinese Academy of Sciences, P. O. Box 918 (4), Beijing 100039, China

  • *Electronic address: jwmei@mail.ihep.ac.cn
  • Electronic address: xingzz@mail.ihep.ac.cn
  • Mailing address.

Phys. Rev. D 69, 073003 – Published 9 April, 2004

DOI: https://doi.org/10.1103/PhysRevD.69.073003

Abstract

Radiative corrections to neutrino mixing and CP violation are analyzed in the minimal seesaw model with two heavy right-handed neutrinos. We find that the textures of the effective Majorana neutrino mass matrix are essentially stable against renormalization effects. Taking into account the Frampton-Glashow-Yanagida Ansatz for the Dirac neutrino Yukawa coupling matrix, we calculate the running effects of light neutrino masses, lepton flavor mixing angles, and CP-violating phases for both the m1=0 (normal mass hierarchy) and m3=0 (inverted mass hierarchy) cases in the standard model and in its minimal supersymmetric extension. Very instructive predictions for the cosmological baryon number asymmetry via thermal leptogenesis are also given with the help of low-energy neutrino mixing quantities.

References (31)

  1. For a review, see C.K. Jung, C. McGrew, T. Kajita, and T. Mann, Annu. Rev. Nucl. Part. Sci. 51, 451 (2001).
  2. SNO Collaboration, Q.R. Ahmad et al., Phys. Rev. Lett. 89, 011301 (2002); ibid.Q.R. Ahmad89, 011302 (2002).
  3. KamLAND Collaboration, K. Eguchi et al., Phys. Rev. Lett. 90, 021802 (2003).
  4. K2K Collaboration, M.H. Ahn et al., Phys. Rev. Lett. 90, 041801 (2003).
  5. M. Fukugita and T. Yanagida, Phys. Lett. B 174, 45 (1986).
  6. P.H. Frampton, S.L. Glashow, and T. Yanagida, Phys. Lett. B 548, 119 (2002).
  7. T. Endoh, S. Kaneko, S.K. Kang, T. Morozumi, and M. Tanimoto, Phys. Rev. Lett. 89, 231601 (2002); R. Kuchimanchi and R.N. Mohapatra, Phys. Rev. D 66, 051301 (2002); ibid.B. Datta and R.N. Mohapatra, 68, 056006 (2003); P. Chankowski and K. Turzynski, Phys. Lett. B 570, 198 (2003); H.K. Dreiner, H. Murayama, and M. Thormeier, hep-ph/0312012.
  8. W.L. Guo and Z.Z. Xing, hep-ph/0310326.
  9. M. Raidal and A. Strumia, Phys. Lett. B 553, 72 (2003); V. Barger, D.A. Dicus, H.J. He, and T. Li, hep-ph/0310278; R.G. Felipe, F.R. Joaquim, and B.M. Nobre, hep-ph/0311029; A. Ibarra and G.G. Ross, hep-ph/0312138.
  10. T. Yanagida, in Proceedings of the Workshop on Unified Theory and the Baryon Number of the Universe, edited by O. Sawada and A. Sugamoto (KEK, Tsukuba, 1979); M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, edited by F. van Nieuwenhuizen and D. Freedman (North-Holland, Amsterdam, 1979); R.N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
  11. Z.Z. Xing, Phys. Rev. D 69, 013006 (2004).
  12. For a review with extensive references, see P. Chankowski and S. Pokorski, Int. J. Mod. Phys. A 17, 575 (2002).
  13. S. Antusch, M. Drees, J. Kersten, M. Lindner, and M. Ratz, Phys. Lett. B 519, 238 (2001).
  14. P. Chankowski and Z. Pluciennik, Phys. Lett. B 316, 312 (1993); ibid.K.S. Babu, C.N. Leung, and J. Pantaleone, 319, 191 (1993); ibid.S. Antusch, M. Drees, J. Kersten, M. Lindner, and M. Ratz, 525, 130 (2002).
  15. R. Barbieri, P. Creminelli, A. Strumia, and N. Tetradis, Nucl. Phys. B575, 61 (2000); ibid.S. Antusch, J. Kersten, M. Lindner, and M. Ratz, B674, 401 (2003); G.F. Giudice, A. Notari, M. Raidal, A. Riotto, and A. Strumia, hep-ph/0310123.
  16. J.R. Ellis and S. Lola, Phys. Lett. B 458, 310 (1999); Z.Z. Xing, Phys. Rev. D 63, 057301 (2001).
  17. H. Fritzsch and Z.Z. Xing, Prog. Part. Nucl. Phys. 45, 1 (2000); H. Fusaoka and Y. Koide, Phys. Rev. D 57, 3986 (1998).
  18. H. Fritzsch and Z.Z. Xing, Phys. Lett. B 517, 363 (2001); ibid.Z.Z. Xing, 530, 159 (2002).
  19. Particle Data Group, K. Hagiwara et al., Phys. Rev. D 66, 010001 (2002).
  20. Z.Z. Xing, Int. J. Mod. Phys. A 19, 1 (2004).
  21. See, e.g., J.N. Bahcall and C. Peña-Garay, J. High Energy Phys. 11, 004 (2003); M. Maltoni et al., Phys. Rev. D 68, 113010 (2003); P.V. de Holanda and A.Yu. Smirnov, hep-ph/0309299; and references therein.
  22. CHOOZ Collaboration, M. Apollonio et al., Phys. Lett. B 420, 397 (1998); Palo Verde Collaboration, F. Boehm et al., Phys. Rev. Lett. 84, 3764 (2000).
  23. J.A. Casas, J.R. Espinosa, A. Ibarra, and I. Navarro, Nucl. Phys. B573, 652 (2000); and references therein.
  24. Antusch et al. [15].
  25. See, e.g., S. Antusch, hep-ph/0208179.
  26. For recent reviews of leptogenesis with extensive references, see W. Buchmüller and M. Plümacher, Int. J. Mod. Phys. A 15, 5047 (2000); A. Pilaftsis and T.E.J. Underwood, hep-ph/0309342; Giudice et al. [15].
  27. W. Buchmüller and M. Plümacher, Phys. Lett. B 431, 431 (1998); W. Buchmüller, P. Di Bari, and M. Plümacher, Nucl. Phys. B643, 367 (2002).
  28. E.W. Kolb and M.S. Turner, The Early Universe (Addison-Wesley, Reading, MA, 1990); H.B. Nielsen and Y. Takanishi, Phys. Lett. B 507, 241 (2001); E.Kh. Akhmedov, M. Frigerio, and A.Yu. Smirnov, J. High Energy Phys. 09, 021 (2003). A different analytical approximation for the dilution factor has been presented by Giudice et al. [26], but it has no significant numerical inconsistency with Eq. (17).
  29. V.A. Kuzmin, V.A. Rubakov, and M.E. Shaposhnikov, Phys. Lett. 155B, 36 (1985).
  30. D.N. Spergel et al., Astrophys. J., Suppl. Ser. 148, 175 (2003).
  31. See, e.g., J. Ellis and M. Raidal, Nucl. Phys. B643, 229 (2002); Raidal and Strumia [9], and references therein.

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