Realistic construction of split fermion models

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 67, Issue 1, 2003, Pages

  Perez, Gilad ^b  

^a TECHNION ISRAEL INSTITUTE OF TECHNOLOGY   (Israel)

^b WEIZMANN INSTITUTE OF SCIENCE   (Israel)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; MASS; MATHEMATICAL ANALYSIS; NORMAL DISTRIBUTION; PHYSICAL MODEL; PHYSICS; THEORY;

EID: 0037281444     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.015011     Document Type: Article

References (41)

1. N. Arkani-Hamed and M. Schmaltz, Phys. Rev. D 61, 033005 (2000).
2. E.A. Mirabelli and M. Schmaltz, Phys. Rev. D 61, 113011 (2000).
3. H. Georgi, A.K. Grant, and G. Hailu, Phys. Rev. D 63, 064027 (2001).
4. D.E. Kaplan and T.M. Tait, J. High Energy Phys. 11, 051 (2001).
5. H.V. Klapdor-Kleingrothaus and U. Sarkar, Phys. Lett. B 541, 332 (2002);
6. P.Q. Hung and M. Seco, hep-ph/0111013;
7. Y. Uehara, J. High Energy Phys. 12, 034 (2001);
8. G. Barenboim, G.C. Branco, A. de Gouvea, and M.N. Rebelo, Phys. Rev. D 64, 073005 (2001);
9. J.L. Crooks, J.O. Dunn, and P.H. Frampton, Astrophys. J. Lett. 546, L1 (2001).
10. T. Matsuda, Phys. Rev. D 66, 047301 (2002);
11. Phys. Rev. DT. Matsuda66, 023508 (2002);
12. Phys. Rev. DT. Matsuda65, 107302 (2002).
13. G. Perez, this issue, Phys. Rev. D 67, 013009 (2003).
14. N. Haba and N. Maru, Phys. Rev. D 66, 055005 (2002);
15. N. HabaN. Maruhep-ph/0202196;
16. N. HabaN. MaruPhys. Lett. B 532, 93 (2002);
17. N. Haba, N. Maru, and N. Nakamura, hep-ph/0209009;
18. N. Maru, Phys. Lett. B 522, 117 (2001);
19. M. Kakizaki and M. Yamaguchi, hep-ph/0110266;
20. M. Maru, N. Sakai, Y. Sakamura, and R. Sugisaka, Nucl. Phys. B616, 47 (2001);
21. M. Kakizaki and M. Yamaguchi, Prog. Theor. Phys. 107, 433 (2002).
22. D.E. Kaplan and T.M. Tait, J. High Energy Phys. 06, 020 (2000);
23. G.R. Dvali and M.A. Shifman, Phys. Lett. B 475, 295 (2000);
24. Phys. Lett. BA. Hebecker and J. March-Russell, 541, 338 (2002);
25. F. Del Aguila and J. Santiago, J. High Energy Phys. 03, 010 (2002).
26. G.C. Branco, A. de Gouvea, and M.N. Rebelo, Phys. Lett. B 506, 115 (2001).
27. N. Arkani-Hamed, Y. Grossman, and M. Schmaltz, Phys. Rev. D 61, 115004 (2000);
28. T. Han, G.D. Kribs, and B. McElrath, hep-ph/0207003;
29. W.F. Chang, I.L. Ho, and J.N. Ng, Phys. Rev. D 66, 076004 (2002);
30. S. Nussinov and R. Shrock, Phys. Lett. B 526, 137 (2002);
31. S. NussinovR. ShrockPhys. Rev. Lett. 88, 171601 (2002);
32. D.J. Chung and T. Dent, Phys. Rev. D 66, 023501 (2002);
33. Phys. Rev. DG. Barenboim, G.C. Branco, A. de Gouvea, and M.N. Rebelo, 64, 073005 (2001);
34. Phys. Rev. DT.G. Rizzo, 64, 015003 (2001);
35. Phys. Rev. DA. Masiero, M. Peloso, L. Sorbo, and R. Tabbash, 62, 063515 (2000);
36. A. Delgado, A. Pomarol, and M. Quiros, J. High Energy Phys. 01, 030 (2000).
37. Z. Chacko, M.A. Luty, and E. Ponton, J. High Energy Phys. 07, 036 (2000).
38. Particle Data Group, K. Hagiwara et al., Phys. Rev. D 66, 010001 (2002).
39. See, e.g., H. Fusaoka and Y. Koide, Phys. Rev. D 57, 3986 (1998);
40. M. Carena et al., hep-ph/0010338.
41. C. Jarlskog, Phys. Rev. Lett. 55, 1039 (1985).