Lepton flavor violation in SUSY SO(10) with predictive Yukawa texture

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 53, Issue 9, 1996, Pages 5244-5252

  Gómez, Mario E ^a   Goldberg, Haim ^a  

^a NORTHEASTERN UNIVERSITY   (United States)

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Indexed keywords

EID: 0346497720     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.53.5244     Document Type: Article

References (28)

1. H. Georgi and C. Jarlskog, Phys. Lett. 86B, 297 (1979).
2. C. D. Froggatt and H. B. Nielsen, Nucl. Phys. B147, 277 (1979).
3. A recent discussion in the context of SO(10) has been given byG. Anderson, S. Raby, S. Dimopoulos, L. J. Hall and G. D. Starkman, Phys. Rev. D 49, 3660 (1994).
4. S. Chaudhuri, S. Chung, and J. Lykken, Report No. hep-ph/9405374, FERMILAB-PUB-94/137-T, 1994 (unpublished).
5. G. Cleaver, in PASCOS 94, Proceedings of the International Symposium on Particles, Strings and Cosmology, Syracuse, New York, edited by K. C. Wali (World Scientific, Singapore, 1995).
6. K. S. Babu and R. N. Mohapatra, Phys. Rev. Lett. 74, 2418 (1995).
7. L. Hall, V. A. Kostelecky, and S. Raby, Nucl. Phys. B267, 415 (1986).
8. F. Borzumati and A. Masiero, Phys. Rev. Lett. 57, 961 (1986).
9. F. Gabbiani and A. Masiero, Nucl. Phys. B322, 235 (1989).
10. R. Barbieri, L. Hall and A. Strumia, Nucl. Phys. B445, 219 (1995).
11. H. E. Haber and G. L. Kane, Phys. Rep. 117, 75 (1985);
12. H. P. Niles, Phys. Rep. 110, 1 (1984).
13. L. Hall, J. Lykken and S. Weinberg, Phys. Rev. D 27, 2359 (1983);
14. S. K. Soni and H. A. Weldon, Phys. Lett. 126B, 215 (1983).
15. As an example, Kahler terms of the form ∫(formula presented) in conjunction with gaugino exchange will generate a contribution δ(formula presented).
16. Particle Data Group, L. Montanet, et al., Phys. Rev. D 50, 1173 (1994).
17. R. Arnowitt and P. Nath, Phys. Rev. D 46, 3981 (1992).
18. M. E. Machacek and M. T. Vaughn, Nucl. Phys. B222, 831 (1983);
19. M. E. Machacek and M. T. Vaughn, Nucl. Phys. B236, 221 (1984);
20. M. E. Machacek and M. T. Vaughn, Nucl. Phys. B249, 70 (1985).
21. The importance of working to two loops has been pointed out in Ref. 15.
22. G. L. Kane, C. Kolda, L. Roszkowski and J. D. Wells, Phys. Rev. D 49, 6173 (1994).
23. S. Dimopoulos, L. Hall, and S. Raby, Phys. Rev. D 45, 4192 (1992);
24. G. W. Anderson, S. Raby, S. Dimopoulos and L. Hall, Phys. Rev. D 47, 3702 (1993).
25. V. Barger, M. S. Berger and P. Ohmann, Phys. Rev. D 47, 1092 (1993);
26. V. Barger, M. S. Berger, T. Han and M. Zralek, Phys. Rev. Lett. 68, 3394 (1992).
27. M. Neubert, Report No. CERN-TH/95-107, hep-ph/9505238 (unpublished).
28. S. G. Gorishny, A. L. Kataev, S. A. Larin and L. R. Surgaladze, Mod. Phys. Lett. A 5, 2703 (1990).