Vol. 24 No. 1 (2014)
Papers

Leptogenesis in \(A_4\) Flavor Symmetry Model by Renormalization Group Evolution

Nguyen Thanh Phong
Department of Physics, Cantho University

Published 12-03-2014

How to Cite

Phong, N. T. (2014). Leptogenesis in \(A_4\) Flavor Symmetry Model by Renormalization Group Evolution. Communications in Physics, 24(1), 9. https://doi.org/10.15625/0868-3166/24/1/3618

Abstract

We study how leptogenesis can be implemented in the seesaw models with \(A_4\) flavor symmetry, which lead to the tri-bimaximalneutrino mixing matrix. By considering renormalzation groupevolution from a high energy scale of flavor symmetry breaking(the GUT scale is assumed) to the low energy scale of relevantphenomena, the off-diagonal terms in a combination of DiracYukawa-coupling matrix can be generated. As aresult, the flavored leptogenesis is successfully realized. Wealso investigate how the effective light neutrino mass \(|\langle m_{ee}\rangle |\) associated with neutrinoless double beta decaycan be predicted byimposing the experimental data on the low energy observables. Wefind a link between the leptogenesis and the neutrinoless doublebeta decay characterized by \(|\langle m_{ee}\rangle|\) through ahigh energy CP phase $\phi$, which is correlated with the lowenergy Majorana CP phases. It is shown that the predictions of \(|\langle m_{ee}\rangle|\) for some fixed parameters of the highenergy physics can be constrained by the current observation ofbaryon asymmetry.

Downloads

Download data is not yet available.

Metrics

Metrics Loading ...

References

  1. P. F. Harrison, D. H. Perkins, W. G. Scott, Phys. Lett. B 530, (2002) 167 [arXiv:hep-ph/0202074].
  2. E. Ma and G. Rajasekaran, Phys. Rev. D 64 (2001) 113012 [arXiv:hep-ph/0106291]; K. S. Babu, E.
  3. Ma and J. W. F. Valle, Phys. Lett. B 552 (2003) 207 [arXiv:hepph/0206292]; G. Altarelli and F.
  4. Feruglio, Nucl. Phys. B 720 (2005) 64 [arXiv:hep-ph/0504165]; G. Altarelli and F. Feruglio, Nucl.
  5. Phys. B 741 (2006) 215 [arXiv:hep-ph/0512103]; G. Altarelli, F. Feruglio and Y. Lin, Nucl. Phys.
  6. B 775 (2007) 31 [arXiv:hepph/0610165]; F. Bazzocchi, S. Kaneko and S. Morisi, JHEP 0803 (2008)
  7. [arXiv:0707.3032 [hepph]]; G. Altarelli, F. Feruglio and C. Hagedorn, JHEP 0803 (2008) 052
  8. [arXiv:0802.0090[hep-ph]]; Y. Lin, Nucl. Phys. B 813, 91 (2009)[arXiv:0804.2867 [hep-ph]]; M. Hirsch,
  9. S. Morisi and J. W. F. Valle, Phys. Rev. D 78 (2008) 093007 [arXiv:0804.1521 [hep-ph]]; Y. H. Ahn
  10. and C. S. chen, arXiv:1001.2869 [hep-ph].
  11. G. Altarelli and F. Feruglio, Nucl. Phys. B 741 (2006) 215 [arXiv:hep-ph/0512103]; G. Altarelli,
  12. arXiv:hep-ph/0905.2350.
  13. F. Feruglio, C. Hagedorn, Y. Lin and L. Merlo, Nucl. Phys. B 775 (2007) 120 [arXiv:hep-ph/0702194];
  14. M. C. Chen and K. T. Mahanthappa, Phys. Lett. B 652 (2007) 34 [arXiv:0705.0714 [hep-ph]]; P.
  15. H. Frampton and T. W. Kephart, JHEP 0709 (2007) 110 [arXiv:0706.1186 [hep-ph]]; G. J. Ding,
  16. arXiv:0803.2278 [hep-ph]; P. H. Frampton and S. Matsuzaki, arXiv:0902.1140 [hep-ph].
  17. S. Pakvasa and H. Sugawara, Phys. Lett. B 82 (1979) 105; T. Brown, N. Deshpande, S. Pakvasa
  18. and H. Sugawara, Phys. Lett. B 141 (1984) 95; T. Brown, S. Pakvasa, H. Sugawara and Y. Ya-
  19. manaka, Phys. Rev. D 30 (1984) 255; D. G. Lee and R. N. Mohapatra, Phys. Lett. B 329 (1994) 463
  20. [arXiv:hep-ph/9403201]; E. Ma, Phys. Lett. B 632 (2006) 352 [arXiv:hep-ph/0508231]; C. Hagedorn,
  21. M. Lindner and R. N. Mohapatra, JHEP 0606 (2006) 042 [arXiv:hep-ph/0602244]; Y. Cai and H.
  22. B. Yu, Phys. Rev. D 74 (2006) 115005 [arXiv:hep-ph/0608022]; F. Caravaglios and S. Morisi, Int.
  23. J. Mod. Phys. A 22 (2007) 2469 [arXiv:hep-ph/0611078]; H. Zhang, Phys. Lett. B 655 (2007) 132
  24. [arXiv:hep-ph/0612214]; Y. Koide, JHEP 0708 (2007) 086 [arXiv:0705.2275 [hepph]]; H. Ishimori, Y.
  25. Shimizu and M. Tanimoto, arXiv:0812.5031 [hep-ph]; Federica Bazzocchi, Luca Merlo, Stefano Morisi,
  26. Nucl. Phys. B 816, (2009) 204; F. Bazzocchi and S. Morisi, arXiv:0811.0345 [hep-ph].
  27. T2K Collaboration, K. Abe et al., Phys. Rew. Lett. 107, 041801 (2011).
  28. MINOS Collaboration, P. Adamson et al., Phys. Rew. Lett. 107, 181802 (2011).
  29. RENO Collaboration, J. Ahn et al., Phys.Rev.Lett. 108 (2012) 191802 [arXiv:hep-ex/1204.0626].
  30. Double CHOOZE Collaboration, Y. Abe et al., Phys. Rew. Lett. 108, 231081 (2012).
  31. Daya Bay Collaboration, F. An et al., Phys. Rew. Lett. 108, 171803 (2012).
  32. D.V. Forero et al., Phys.Rev. D 86 (2012) 073012 [arXiv:hep-ph/1205.4018].
  33. P. Gell-Mann, R. Ramond, R. Slansky, Supergravity, Proceedings of the Supergravity Stony Brook
  34. Workshop, P. van Nieuwenhuizen and D. Freedmann, Eds., New York, NY, USA,1979.
  35. M. Fukugita and T. Yanagida, Phys. Lett. B 174 (1986) 45.
  36. S. M. Bilenky, S. Pascoli, and S. T. Petcov, Phys. Rev. D 64, 053010 (2001); S. Pascoli, S. T. Petcov,
  37. and L. Wolfenstein, Phys. Lett. B 524, 319 (2002); 549, 177 (2002); S. T. Petcov, New J. Phys. 6,
  38. (2004).
  39. C. D. Froggatt and H. B. Nielsen, Nucl. Phys. B 147 (1979) 277.
  40. R. Gonzalez Felipe, F. R. Joaquim and B. M. Nobre, Phys. Rev. D 70, 085009 (2004) [arXiv:hep-
  41. ph/0311029], K. Turzynski, Phys. Lett. B 589, 135 (2004) [arXiv:hep-ph/0401219], G. C. Branco,
  42. R. Gonzalez Felipe, F. R. Joaquim and B. M. Nobre, Phys. Lett. B 633, 336 (2006) [arXiv:hep-
  43. ph/0507092], J. A. Casas, J. R. Espinosa, A. Ibarra and I. Navarro, Nucl. Phys. B 573, (2000) 652
  44. [arXiv:hep-ph/9910420]; J. A. Casas, J. R. Espinosa, A. Ibarra and I. Navarro, Nucl. Phys. B 569,
  45. (2000) 82 [arXiv:hep-ph/9905381].
  46. T.Phong Nguyen, P.V. Dong, Adv.High Energy Phys. 2012 (2012) 254093.
  47. L. Covi, E. Roulet and F. Vissani, Phys. Lett. B384, (1996) 169; A. Pilaftsis, Int. J. Mod. Phys. A
  48. , (1999) 1811 [arXiv:hep-ph/9812256].
  49. A. Abada, S. Davidson, A. Ibarra, F. X. Josse-Michaux, M. Losada and A. Riotto, JHEP 0609, 010
  50. (2006) [arXiv:hep-ph/0605281].
  51. A. Abada, S. Davidson, F. X. Josse-Michaux, M. Losada and A. Riotto, JCAP 0604, (2006) 004
  52. [arXiv:hep-ph/0601083]; S. Antusch, S. F. King and A. Riotto, JCAP 0611, (2006) 011 [arXiv:hep-
  53. ph/0609038].
  54. H. V. Klapdor-Kleingrothaus et al., Eur. Phys. J. A 12, 147 (2001) [arXiv:hep-ph/0103062]; H. V.
  55. Klapdor-Kleingrothaus, I. V. Krivosheina, A. Dietz and O. Chkvorets, Phys. Lett. B 586, 198 (2004)
  56. [arXiv:hep-ph/0404088]; C. Arnaboldi et al. [CUORICINO Collaboration], Phys. Rev. C 78, 035502
  57. (2008) [arXiv:0802.3439 [hep-ex]]; J. Wolf [KATRIN Collaboration], arXiv:0810.3281 [physics.ins-det].
  58. C. Aalseth et al., arXiv:hep-ph/0412300; I. Abt et al., arXiv:hep-ex/0404039.
  59. WMAP Collaboration, D.N. Spergel et al., Astrophys. J. Suppl. 148, (2003) 175; M. Tegmark et al.,
  60. Phys. Rev. D 69, (2004) 103501; C. L. Bennett et al., Astrophys. J. Suppl. 148, (2003) 1 [arXiv:astro-
  61. ph/0302207].