Minimal four-family supergravity model

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 53, Issue 3, 1996, Pages 1616-1647

  Gunion, J F ^a   McKay, Douglas W ^b   Pois, H ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF KANSAS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000352498     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.53.1616     Document Type: Article

References (75)

1. J. F. Gunion, D. W. McKay and H. Pois, Phys. Lett. B 334, 339 (1994).
2. For a detailed discussion of the neutrino sector, seeS. King., Phys. Lett. B 281, 295 (1992).
3. OPAL Collaboration, M. Z. Akrawy, et al., Phys. Lett. B 236, 364 (1990);
4. ALEPH Collaboration, D. Decamp, et al., Phys. Lett. B 236, 511 (1990).
5. A recent survey of lower bounds on heavy and neutral charged leptons and on heavy quarks is given by the Particle Data Group, L. Montanet, et al., Phys. Rev. D 50, 1173 (1994).
6. M. Drees and S. P. Martin, Report of Subgroup 2 of the DPF Working Group on Electroweak Symmetry Breaking and Beyond the Standard Model (unpublished).
7. H. Baer, J. Gunion, C. Kao and H. Pois, Phys. Rev. D 51, 2159 (1995).
8. An exception is the early (formula presented) = 4, (formula presented) = 0 supergravity extension of the SM byM. Cvetic and C. Preitschopf, Nucl. Phys. B272, 490 (1986).
9. For more recent work, seeP. Agrawal and W. S. Hou, Phys. Rev. D 46, 1022 (1992);
10. P. Agrawal, S. Ellis and W. S. Hou, Phys. Lett. B 256, 289 (1991);
11. S. King, Phys. Lett. B 281, 295 (1992);
12. C. Hill and E. Paschos, Phys. Lett. B 241, 96 (1990);
13. W. S. Hou and R. G. Stuart, Nucl. Phys. B349, 91 (1991);
14. M. Sher and Y. Yuan, Phys. Lett. B 285, 336 (1992);
15. H. Fritzsch, Phys. Lett. B 289, 92 (1992);
16. B. Mukhopadhyaya and D. P. Roy, Phys. Rev. D 48, 2105 (1993);
17. J. L. Hewett, SLAC Report No. SLAC PUB 6521, 1994 (unpublished);
18. Z. Berezhiani and E. Nardi, Phys. Rev. D 52, 3087 (1995).
19. Mark II Collaboration, G. S. Abrams, et al., Phys. Rev. Lett. 63, 2173 (1989);
20. L3 Collaboration, B. Advera, et al., Phys. Lett. B 231, 509 (1989);
21. OPAL Collaboration, I. Decamp, et al., Phys. Lett. B 231, 519 (1989);
22. DELPHI Collaboration, M. Z. Akrawy, et al., Phys. Lett. B 231, 539 (1989).
23. For a recent example of theoretical motivation of (formula presented) = 4, see Berezhiani and Nardi Ref. 7.
24. P. Langacker, in Particles, Strings Cosmology, Proceedings of the International Symposium, Boston, Massachusetts, 1990, edited by P. Nath and S. Reucroft (World Scientific, Singapore, 1990);
25. P. Langacker and M. X. Luo, Phys. Rev. D 44, 817 (1991);
26. U. Amaldi, W. de Boer and H. Furstenau, Phys. Lett. B 260, 447 (1991);
27. J. Ellis, S. Kelley and D. V. Nanopoulos, Phys. Lett. B 260, 131 (1991).
28. P. Langacker and N. Polonsky, Phys. Rev. D 47, 4028 (1993);
29. P. Langacker and N. Polonsky, Phys. Rev. D 49, 1454 (1994);
30. V. Barger, M. Berger, P. Ohmann, and R.J. N. Phillips, Phys. Lett. B 314, 351 (1993);
31. G. Kane, C. Kolda, L. Roszkowski and J. Wells, Phys. Rev. D 49, 6173 (1994);
32. G. Ross and R. G. Roberts, Nucl. Phys. B377, 571 (1992);
33. B. D. Wright, Institution Report No. MAD/PH/812 (unpublished). For string Yukawa threshold effects, seeI. Antoniadis, E. Gava, K. S. Narain and T. R. Taylor, Nucl. Phys. B407, 706 (1993).
34. P. H. Frampton, S. Nandi and J. G. Scanio, Phys. Lett. 85B, 225 (1979).
35. S. Dimopoulos and A. Pomarol, Phys. Lett. B 353, 222 (1995).
36. H. E. Haber, CERN Report No. CERN TH/95 178, 1995 (unpublished).
37. D. V. Nanopoulos and D. Ross, Phys. Lett. 118B, 99 (1982);
38. J. Bjorkman and D. Jones, Nucl. Phys. B259, 533 (1985).
39. P. Langacker and N. Polonsky, Phys. Rev. D 52, 3081 (1995).
40. M. L. Swartz, SLAC Report No. PUB 6710 (unpublished).
41. J. Bagger, V. Matchev and D. Pierce, Phys. Lett. B 348, 443 (1995).
42. See, for example, V. Barger, M. S. Berger and P. Ohmann, Phys. Rev. D 47, 1093 (1993).
43. CDF Collaboration, F. Abe, et al., Phys. Rev. Lett. 74, 2626 (1995);
44. D0 Collaboration, S. Abachi, et al., Phys. Rev. Lett. 74, 2632 (1995).
45. B. Pendelton and G. Ross, Phys. Lett. 98B, 291 (1981);
46. C. Hill, Phys. Rev. D 24, 691 (1981);
47. W. Bardeen, M. Carena, S. Pokorski and C. Wagner, Phys. Lett. B 320, 110 (1994);
48. J. Bagger, S. Dimopoulos and E. Masso, Phys. Rev. Lett. 55, 920 (1985).
49. See, for example, G. Gamberini, G. Ridolfi and F. Zwirner, Nucl. Phys. B331, 331 (1990).
50. T. L. Barklow, et al., “Electroweak Symmetry Breaking and Beyond the Standard Model, " SLAC Report No. SLAC PUB 95 6893, 1995 (unpublished).
51. J. F. Gunion, A. Strange, and S. Willenbrock (in preparation).
52. S. Mrenna and G. Kane, Institution Report No. CALT 68 1938, 1994 (unpublished).
53. These effects were first explored byJ. F. Gunion and S. Geer, in Proceedings of the Workshop on Physics at Current Accelerators and the Supercollider, Argonne, Illinois, 1993, edited by J. Hewett, A. White, and D. Zeppenfeld (ANL HEP CP 93 92, Argonne, 1993), p. 335.
54. M. Drees and M. M. Nojiri, Phys. Rev. D 45, 2482 (1992).
55. S. Martin and P. Ramond, Phys. Rev. D 48, 5365 (1993), provide a convenient summary of squark and slepton mass relations in the (formula presented) = 3 case.
56. J. F. Gunion and H. E. Haber, Phys. Rev. D 37, 2515 (1988).
57. See H. Baer et al., “Low Energy Supersymmetry Phenomenology,” Institution Report No. FSU HEP 950401 (unpublished), and references therein.
58. V. Barger, M. Berger, J. Gunion and T. Han, Phys. Rev. Lett. 75, 1462 (1995).
59. F. Abe, et al., Phys. Rev. Lett. 64, 147 (1990);
60. F. Abe, et al., Phys. Rev. Lett. 68, 447 (1992);
61. Particle Data Group, T. Trippe (private communication).
62. J. Houston and R. Blair (private communication).
63. W. S. Hou and R. Stuart, Phys. Rev. D 43, 3669 (1991).
64. D. Schaile, in Proceedings of the 27th International Conference on High Energy Physics, Glasgow, Scotland, 1994, edited by P. J. Bussey and I. G. Knowles (IOP, London, 1995);
65. SLD Collaboration, F. Abe, et al., Phys. Rev. Lett. 73, 25 (1994).
66. M. Peskin and T. Takeuchi, Phys. Rev. D 46, 381 (1992).
67. C. P. Burgess, S. Godfrey, H. Konig, D. London and I. Maksymyk, Phys. Rev. D 49, 6115 (1994);
68. C. P. Burgess, S. Godfrey, H. Konig, D. London and I. Maksymyk, Phys. Lett. B 326, 276 (1994);
69. I. Maksymyk, C. P. Burgess and D. London, Phys. Rev. D 50, 529 (1994);
70. P. Bamert and C. P. Burgess, Z. Phys. C 66, 995 (1995).
71. A. Kundu and P. Roy, Institution Report No. SINP TNP/94 07, TIFR/TH/94 38 (unpublished).
72. H. Pois and T. C. Yuan (unpublished).
73. Figures available on the CDF WWW Home Page.
74. S. Martin and M. Vaughn, Phys. Rev. D 50, 2282 (1994).
75. We thank H. Murayama for several conversations on various aspects of the discussion in Appendix B. See also Ref. 30.