Low energy supersymmetry with a neutralino LSP and the CDF [Formula presented] event

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 55, Issue 3, 1997, Pages 1372-1398

  Ambrosanio, S ^a   Kane, G L ^a   Kribs, Graham D ^a   Martin, Stephen P ^a   Mrenna, S ^b  

^a UNIVERSITY OF MICHIGAN   (United States)

^b ARGONNE NATIONAL LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000460688     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.1372     Document Type: Article

References (54)

1. S. Ambrosanio, G. L. Kane, G. D. Kribs, S. P. Martin, and S. Mrenna, Phys. Rev. Lett.76, 3498 (1996).
2. S. Park, in 10th Topical Workshop on Proton-Anti-proton Collider Physics, edited by Rajendran Raja and John Yoh, AIP Conf. Proc. No. 357 (AIP, New York, 1996);
3. L. Nodulman, in Proceedings of the International Europhysics Conference on High Energy Physics, Brussels, 1995, edited by J. Lemonne (World Scientific, New Jersey, 1996).
4. We make no attempt to connect our results with unification scale physics using a RGE analysis such as in many studies, e.g., G. L. Kane, C. Kolda, L. Roszkowski, and J. D. Wells, Phys. Rev. D49, 6173 (1994); the primary issues one would have to address are obtaining low (Formula presented), small (Formula presented), (Formula presented) not necessarily equal to (Formula presented), and (Formula presented) not necessarily close to (perhaps a factor of (Formula presented)–(Formula presented) different from) (Formula presented).
5. S. Ambrosanio, G. L. Kane, G. D. Kribs, S. P. Martin, and S. Mrenna, Phys. Rev. D54, 5395 (1996).
6. S. Dimopoulos, M. Dine, S. Raby, and S. Thomas, Phys. Rev. Lett.76, 3494 (1996).
7. S. Dimopoulos, S. Thomas, and J. D. Wells, Phys. Rev. D54, 3283 (1996).
8. G. L. Kane and J. D. Wells, Phys. Rev. Lett.76, 4458 (1996).
9. H. Komatsu and J. Kubo, Phys. Lett.157B, 90 (1985);
10. Nucl. Phys.B263, 265 (1986);
11. H. E. Haber, G. L. Kane, and M. Quirós, Phys. Lett.160B, 297 (1985);
12. Nucl. Phys.B273, 333 (1986).
13. H. E. Haber and D. Wyler, Nucl. Phys.B323, 267 (1989).
14. S. Ambrosanio and B. Mele, Phys. Rev. D52, 3900 (1995);
15. 53, 2541 (1996).
16. S. Ambrosanio and B. Mele, following paper, Phys. Rev. D55, 1399 (1997).
17. H. E. Haber and G. L. Kane, Phys. Rep.117, 75 (1985).
18. M. M. El Kheishen, A. A. Shafik, and A. A. Aboshousha, Phys. Rev. D45, 4345 (1992).
19. V. Barger, M. S. Berger, and P. Ohmann, Phys. Rev. D49, 4908 (1994).
20. A. Bartl, H. Fraas, and W. Majerotto, Nucl. Phys.B278, 1 (1986);
21. A. Bartl, H. Fraas, W. Majerotto, and N. Oshimo, Phys. Rev. D40, 1594 (1989).
22. G. L. Kane and S. Mrenna, Phys. Rev. Lett.77, 3502 (1996).
23. S. Dawson, E. Eichten, and C. Quigg, Phys. Rev. D31, 1581 (1985).
24. H. Baer, C.-h. Chen, F. Paige, and X. Tata, Phys. Rev. D49, 3283 (1994).
25. See, e.g., Y. Okada, M. Yamaguchi, and T. Yanagida, Phys. Lett. B262, 54 (1991);
26. M. Drees and M. Nojiri, Phys. Rev. D45, 2482 (1992);
27. H. E. Haber and R. Hempfling, 48, 4280 (1993);
28. M. Carena, J. R. Espinosa, M. Quirós, and C. E. M. Wagner, Phys. Lett. B355, 209 (1995);
29. M. Carena, M. Quirós, and C. E. M. Wagner, Nucl. Phys.B461, 407 (1996).
30. J. Ellis, G. Ridolfi, and F. Zwirner, Phys. Lett. B262, 477 (1991).
31. L3 Collaboration, Phys. Lett. B377, 289 (1996).
32. See also OPAL Collaboration, 377, 181 (1996).
33. L3 Collaboration, Phys. Lett. B350, 109 (1995).
34. J. L. Feng, N. Polonsky, and S. Thomas, Phys. Lett. B370, 95 (1996).
35. H. L. Lai et al., Phys. Rev. D51, 4763 (1995).
36. See, e.g., S. Mrenna, G. L. Kane, G. D. Kribs, and J. D. Wells, Phys. Rev. D53, 1168 (1996), and references therein.
37. M. Drees and K. Hagiwara, Phys. Rev. D42, 1709 (1990).
38. M. Drees and K.-I. Hikasa, Phys. Lett. B252, 127 (1990).
39. A. Djouadi et al., Nucl. Phys.B349, 48 (1991);
40. M. Boulware and D. Finnell, Phys. Rev. D44, 2054 (1991);
41. J. D. Wells, C. Kolda, and G. L. Kane, Phys. Lett. B338, 219 (1994);
42. D. Garcia and J. Sola, 354, 335 (1995);
43. G. L. Kane, R. G. Stuart, and J. D. Wells, 354, 350 (1995);A. Dabelstein, W. Hollik, and W. Mösle, Report No. hep-ph/9506251 (unpublished);
44. M. Carena, H. E. Haber, and C. E. M. Wagner, Nucl. Phys.B472, 55 (1996);
45. P. H. Chankowski and S. Pokorski, Phys. Lett. B366, 188 (1996);
46. J. Ellis, J. Lopez, and D. Nanopoulos, 372, 95 (1996);
47. J. D. Wells and G. L. Kane, Phys. Rev. Lett.76, 869 (1996);
48. E. H. Simmons and Y. Su, Phys. Rev. D54, 3580 (1996);
49. P. H. Chankowski and S. Pokorski, Nucl. Phys.B475, 3 (1996).
50. M. Shifman, Mod. Phys. Lett. A10, 605 (1995);
51. J. Erler and P. Langacker, Phys. Rev. D52, 441 (1995); fifth reference of Ref. 29.
52. G. Bhattacharyya and R. N. Mohapatra, Phys. Rev. D54, 4204 (1996).
53. J. L. Lopez and D. V. Nanopoulos, Report No. hep-ph/9607220 (unpublished).
54. J. Hisano, K. Tobe, and T. Yanagida, Phys. Rev. D55, 411 (1997).