- Access by Xinjiang University
Flavor violating transitions of charged leptons from a seesaw mechanism of dimension seven
Phys. Rev. D 82, 113003 – Published 1 December, 2010
DOI: https://doi.org/10.1103/PhysRevD.82.113003
Abstract
A mechanism has been suggested recently to generate the neutrino mass out of a dimension-seven operator. This is expected to relieve the tension between the occurrence of a tiny neutrino mass and the observability of other physics effects beyond it. Such a mechanism would inevitably entail lepton flavor violating effects. We study in this work the radiative and purely leptonic transitions of the light charged leptons. In so doing we make a systematic analysis of the flavor structure by providing a convenient parametrization of the mass matrices in terms of independent physical parameters and diagonalizing them explicitly. We illustrate our numerical results by sampling over two phases and one Yukawa coupling which are the essential parameters in addition to the heavy lepton mass. We find that with the stringent constraints coming from the muon decays and the muon-electron conversion in nuclei taken into account the decays of the tau lepton are severely suppressed in the majority of parameter space. There exist, however, small regions in which some tau decays can reach a level that is about 2 orders of magnitude below their current bounds.
Article Text
References (46)
- M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, edited by D. Freedman and P. van Nieuwenhuizen (North-Holland, Amsterdam, 1979), p. 315; T. Yanagida, in Proceedings of the Workshop on Unified Theory and Baryon Number in the Universe, edited by O. Sawada and A. Sugamoto (KEK, Japan, 1979); R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
- W. Konetschny and W. Kummer, Phys. Lett. 70B, 433 (1977); T. P. Cheng and L. F. Li, Phys. Rev. D 22, 2860 (1980); J. Schechter and J. W. F. Valle, 22, 2227 (1980).
- R. Foot, H. Lew, X. G. He, and G. C. Joshi, Z. Phys. C 44, 441 (1989).
- E. Ma, Phys. Rev. Lett. 81, 1171 (1998).
- S. Weinberg, Phys. Rev. Lett. 43, 1566 (1979).
- A. Zee, Phys. Lett. 93B, 389 (1980); 95B, 461(E) (1980).
- A. Zee, Nucl. Phys. B264, 99 (1986).
- K. S. Babu, Phys. Lett. B 203, 132 (1988).
- L. M. Krauss, S. Nasri, and M. Trodden, Phys. Rev. D 67, 085002 (2003); M. Aoki, S. Kanemura, and O. Seto, Phys. Rev. Lett. 102, 051805 (2009).
- K. S. Babu, S. Nandi, and Z. Tavartkiladze, Phys. Rev. D 80, 071702 (2009).
- I. Picek and B. Radovcic, Phys. Lett. B 687, 338 (2010).
- F. Bonnet, D. Hernandez, T. Ota, and W. Winter, J. High Energy Phys. 10 (2009) 076.
- M. L. Brooks et al. (MEGA Collaboration), Phys. Rev. Lett. 83, 1521 (1999).
- U. Bellgardt et al. (SINDRUM Collaboration), Nucl. Phys. B299, 1 (1988).
- E. Baracchini (MEG Collaboration), arXiv:1005.2569.
- B. Aubert et al. (BABAR Collaboration), Phys. Rev. Lett. 104, 021802 (2010).
- K. Hayasaka et al. (Belle Collaboration), Phys. Lett. B 666, 16 (2008).
- G. Marchiori (BABAR Collaboration), AIP Conf. Proc. 1200, 857 (2010).
- Y. Miyazaki et al. (Belle Collaboration), Phys. Lett. B 660, 154 (2008).
- B. C. Odom, D. Hanneke, B. D’Urso, and G. Gabrielse, Phys. Rev. Lett. 97, 030801 (2006); 99, 039902(E) (2007).
- G. W. Bennett et al. (Muon Collaboration), Phys. Rev. D 73, 072003 (2006).
- B. C. Regan, E. D. Commins, C. J. Schmidt, and D. DeMille, Phys. Rev. Lett. 88, 071805 (2002); G. W. Bennett et al. (Muon Collaboration), Phys. Rev. D 80, 052008 (2009).
- C. Dohmen et al. (SINDRUM II Collaboration), Phys. Lett. B 317, 631 (1993).
- W. H. Bertl et al. (SINDRUM II Collaboration), Eur. Phys. J. C 47, 337 (2006).
- Y. Kuno, Nucl. Phys. B, Proc. Suppl. 149, 376 (2005).
- J. Hisano, T. Moroi, K. Tobe, and M. Yamaguchi, Phys. Rev. D 53, 2442 (1996); J. Hisano, T. Moroi, K. Tobe, M. Yamaguchi, and T. Yanagida, Phys. Lett. B 357, 579 (1995).
- M. Kakizaki, Y. Ogura, and F. Shima, Phys. Lett. B 566, 210 (2003); E. J. Chun, K. Y. Lee, and S. C. Park, 566, 142 (2003).
- A. Abada, C. Biggio, F. Bonnet, M. B. Gavela, and T. Hambye, Phys. Rev. D 78, 033007 (2008).
- A. Abada, C. Biggio, F. Bonnet, M. B. Gavela, and T. Hambye, J. High Energy Phys. 12 (2007) 061.
- P. Q. Hung, Phys. Lett. B 649, 275 (2007); 659, 585 (2008); J. P. Bu, Y. Liao, and J. Y. Liu, 665, 39 (2008).
- S. R. Choudhury, A. S. Cornell, A. Deandrea, N. Gaur, and A. Goyal, Phys. Rev. D 75, 055011 (2007); M. Blanke, A. J. Buras, B. Duling, A. Poschenrieder, and C. Tarantino, J. High Energy Phys. 05 (2007) 013.
- P. Fileviez Perez and M. B. Wise, Phys. Rev. D 80, 053006 (2009); Y. Liao and J. Y. Liu, 81, 013004 (2010).
- Y. Kuno and Y. Okada, Rev. Mod. Phys. 73, 151 (2001).
- A. Masiero, S. K. Vempati, and O. Vives, New J. Phys. 6, 202 (2004); M. Raidal et al., Eur. Phys. J. C 57, 13 (2008).
- A. Brignole and A. Rossi, Nucl. Phys. B701, 3 (2004); E. Arganda and M. J. Herrero, Phys. Rev. D 73, 055003 (2006); J. R. Ellis, J. Hisano, M. Raidal, and Y. Shimizu, 66, 115013 (2002).
- T. P. Cheng and L. F. Li, Phys. Rev. Lett. 38, 381 (1977); A. Masiero, S. K. Vempati, and O. Vives, Nucl. Phys. B649, 189 (2003); J. Hisano, T. Moroi, K. Tobe, M. Yamaguchi, and T. Yanagida, Phys. Lett. B 357, 579 (1995).
- F. del Aguila, J. I. Illana, and M. D. Jenkins, J. High Energy Phys. 09 (2010) 40.
- J. Bernabeu, E. Nardi, and D. Tommasini, Nucl. Phys. B409, 69 (1993); B. Murakami, Phys. Rev. D 65, 055003 (2002).
- R. Kitano, M. Koike, and Y. Okada, Phys. Rev. D 66, 096002 (2002); 76, 059902(E) (2007).
- A. Czarnecki, W. J. Marciano, and K. Melnikov, AIP Conf. Proc. 435, 409 (1998).
- Y. Liao, Nucl. Phys. B749, 153 (2006).
- O. U. Shanker, Phys. Rev. D 20, 1608 (1979).
- H. C. Chiang, E. Oset, T. S. Kosmas, A. Faessler, and J. D. Vergados, Nucl. Phys. A559, 526 (1993).
- S. Weinberg and G. Feinberg, Phys. Rev. Lett. 3, 111 (1959); 3, 244(E) (1959); N. Cabibbo and R. Gatto, Phys. Rev. 116, 1334 (1959).
- W. J. Marciano and A. I. Sanda, Phys. Rev. Lett. 38, 1512 (1977).
- M. Maltoni, T. Schwetz, M. A. Tortola, and J. W. F. Valle, New J. Phys. 6, 122 (2004).