Can precision measurements of slepton masses probe right handed neutrinos?

Physical Review D

Volumn 63, Issue 5, 2001, Pages

  Baer, Howard ^a,b   Balazs, Csaba ^a   Kenichi Mizukoshi, J ^a   Tata, Xerxes ^a  

^a Florida State University   (United States)

^b UNIVERSITY OF HAWAII   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; CALCULATION; MASS; MODEL; MOLECULAR SIZE; PHYSICS; QUANTUM MECHANICS;

EID: 0034896101     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.63.055011     Document Type: Article

References (32)

1. For recent reviews, see, e.g., S. Martin, in Perspectives on Siipersymmetry, edited by G. Kane (World Scientific, Singapore, 1998), hep-ph/9709356; M. Drees, hep-ph/9611409; J. Bagger, hep-ph/9604232;
2. X. Tata, Proceedings of the IX J. Smeca Summer School, edited by J. Barata, A. Malbousson, and S. Novaes (World Scientific, Singapore, 1998), hep-ph/9706307;
3. S. Dawson, Proceedings TASI 97, edited by J. Bagger (World Scientific, Singapore, 1999), hep-ph/9712464.
4. K. Inoue, A. Kakuto, H. Komatsu, and H. Takeshita, Prog. Theor. Phys. 68, 927 (1982); 71, 413 (1984).
5. Y. Fukuda et al., Phys. Rev. Lett. 82, 2644 (1999);
6. S. Fukuda et al., Phys. Rev. Lett. ibid. 85, 3999 (2000).
7. M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity, Proceedings of the Workshop, New York, 1979, edited by D. Freedman and P. Van Nieuwenhuizen, Stony Brook, NY, 1979 (North-Holland, Amsterdam);
8. T. Yanagida, in Proceedings of the Workshop on Unified Theory and Baryon Number in the Universe, Tsukuba, Japan, 1979, edited by O. Sawuda and A. Sugamoto (KEK Report No. 79-18, Tsukuba, 1979);
9. R.N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
10. See, e.g., M.K. Parida and N. Nimai Singh, Phys. Rev. D 59, 032002 (1999).
11. For the impact of the RHN on other aspects of SUSY phenomenology, see J. Hisano, T. Moroi, K. Tobe, M. Yamaguchi, and T. Yanagida, Phys. Lett. B 357, 579 (1995);
12. J. Hisano, T. Moroi, K. Tobe, and M. Yamaguchi, Phys. Rev. D 53, 2442 (1996);
13. J. Hisano and D. Nomura, Phys. Rev. D ibid. 59, 116005 (1999);
14. T. Moroi, J. High Energy Phys. 03, 019 (2000);
15. K. Babu, B. Dutta, and R.N. Mohaptra, Phys. Rev. Lett. 85, 5064 (2000);
16. Phys. Lett. B 458, 93 (1999).
17. T. Moroi, Phys. Lett. B 321, 56 (1994).
18. V. Barger, T. Han, and J. Jiang, Phys. Rev. D (to be published), hep-ph/0006223.
19. We use the renormalization group equations as given in H. Baer, M. Dfaz, P. Quintana, and X. Tata, J. High Energy Phys. 04, 016 (2000); see also Hisano et al. [6].
20. S. Martin and M. Vaughn, Phys. Rev. D 50, 2282 (1994); explicit 2-loop renormalization group equations for the MSSM plus a RHN are given in H. Baer et al. (in preparation).
21. T. Tsukamoto et al, Phys. Rev. D 51, 3153 (1995).
22. H. Baer, R. Munroe, and X. Tata, Phys. Rev. D 54, 6735 (1996).
23. H. Baer, A. Bartl, D. Karatas, W. Majerotto, and X. Tata, Int. J. Mod. Phys. A4, 4111 (1989)
24. M. Danielson et al., in New Directions for High Energy Physics, Snowmass 96 Summer Study, edited by D. Cassel, L. Trindle Gennari, and R. H Siemann (SLAC, Stanford, 1997).
25. S. Kuhlman et al, NLC Zero Design Report, SLAC Report 485 (1996).
26. M. Nojiri, K. Fujii, and T. Tsukamoto, Phys. Rev. D 54, 6756 (1996).
27. F. Paige, S. Protopopescu, H. Baer, and X. Tata, hep-ph/0001086.
28. R.N. Mohaptra and J.W.F. Valle, Phys. Rev. D 34, 1642 (1986)
29. For a review, see R.N. Mohapatra, hep-ph/9910365.
30. This extreme case for the neutrino mass matrix is also realized in the flipped SU(5) model as discussed by M. Drees and X. Tata, Phys. Lett. B 206, 259 (1988)
31. Y. Grossman and M. Neubert, Phys. Lett. B 474, 361 (2000).
32. N. Arkani-Hamed, L. Hall, H. Murayama, D. Smith, and N. Weiner, hep-ph/0006312.