Possible signals of constrained minimal supersymmetry at a high luminosity Fermilab Tevatron collider

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 53, Issue 3, 1996, Pages 1168-1180

  Mrenna, Stephen ^a   Kane, G L ^b   Kribs, Graham D ^b   Wells, James D ^b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b UNIVERSITY OF MICHIGAN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001612198     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.53.1168     Document Type: Article

References (59)

1. T. Sjöstrand, Comput. Phys. Commun. 82, 74 (1994).
2. H. U. Bengtsson and T. Sjöstrand, Comput. Phys. Commun. 46, 43 (1987).
3. T. Sjöstrand and M. Bengtsson, Comput. Phys. Commun. 43, 367 (1987).
4. H. Baer, F. E. Paige, S. D. Protopopescu, and X. Tata, in Proceedings of the Workshop on Physics at Current Accelerators and the Supercolliders, Argonne, Illinois, 1993, edited by J. Hewett etal (ANL, Argonne, 1993), p. 703, Report No.
5. We note that a Monte Carlo “SUSYSM” was developed for hadron supercolliders using an interface to the scpythia scjetset system in Ref. [42].
6. F. E. Paige and S. D. Protopopescu, Report No. BNL 38774, 1986.
7. S. Mrenna, “Simulating Supersymmetry with scpythia and scjetset,” Report No. CIT 68 1987 (unpublished).
8. G. L. Kane, C. Kolda, L. Roszkowski and J. D. Wells, Phys. Rev. D 49, 6173 (1994).
9. H. E. Haber and G. L. Kane, Phys. Rep. 117, 75 (1985).
10. S. P. Martin, Phys. Rev. D 46, 2769 (1992).
11. E. Diehl, G. L. Kane, C. Kolda and J. D. Wells, Phys. Rev. D 52, 4223 (1993).
12. P. Sikivie, in Trends in Astroparticle Physics, Proceedings of the Workshop, Stockholm, Sweden, 1994, edited by L. Bergstrom et al. [Nucl. Phys. B (Proc. Suppl.) 43 (1995)], Report No. hep ph/9503292 (unpublished).
13. J. M. Frère and G. L. Kane, Nucl. Phys. B223, 331 (1983).
14. For a recent review, see H. Baer et al., Report No. FSU HEP 950401, hep ph/9503479 (unpublished), and references therein.
15. J. D. Wells, C. Kolda and G. L. Kane, Phys. Lett. B 338, 219 (1994).
16. M. Shifman, Mod. Phys. Lett. A 10, 605 (1995).
17. G. L. Kane, R. G. Stuart and J. D. Wells, Phys. Lett. B 354, 350 (1995).
18. S. Dawson, E. Eichten and C. Quigg, Phys. Rev. D 31, 1581 (1985).
19. A. Bartl, H. Fraas and W. Majerotto, Z. Phys. C 30, 441 (1986).
20. A. Bartl, H. Fraas and W. Majerotto, Nucl. Phys. B378, 1 (1986).
21. J. F. Gunion and H. E. Haber, Phys. Rev. D 37, 2515 (1988).
22. CDF Collaboration, F. Abe, et al., Phys. Rev. Lett. 74, 2626 (1995).
23. H. Baer, V. Barger, R. J. N. Phillips and X. Tata, Phys. Lett. B 220, 303 (1989).
24. H. Baer, C. Chen, F. Paige and X. Tata, Phys. Rev. D 49, 3283 (1994).
25. H. Baer, J. F. Gunion, C. Kao and H. Pois, Phys. Rev. D 51, 2159 (1995).
26. J. L. Lopez, D. V. Nanopoulos, X. Wang and A. Zichichi, Phys. Rev. D 52, 142 (1995).
27. H. Baer, C. Chen, C. Kao and X. Tata, Phys. Rev. D 52, 1565 (1995).
28. D. A. Dicus, S. Nandi and X. Tata, Phys. Lett. 129B, 451 (1983);
29. A. H. Chamseddine, P. Nath and R. Arnowitt, Phys. Lett. 129B, 445 (1983);
30. H. Baer, K. Hagiwara and X. Tata, Phys. Rev. D 35, 1598 (1987);
31. P. Nath and R. Arnowitt, Mod. Phys. Lett. A 2, 331 (1987);
32. H. Baer and X. Tata, Phys. Rev. D 47, 2739 (1993);
33. J. L. Lopez, D. V. Nanopoulos, X. Wang and A. Zichichi, Phys. Rev. D 48, 2062 (1993);
34. H. Baer, C. Kao and X. Tata, Phys. Rev. D 48, 5175 (1993);
35. H. Baer, C. Chen, F. Paige and X. Tata, Phys. Rev. D 50, 4508 (1994);
36. H. Baer, C. Chen, R. Munroe, F. E. Paige and X. Tata, Phys. Rev. D 51, 1046 (1995).
37. R. Barbieri, F. Caravaglios, M. Frigeni and M. L. Mangano, Nucl. Phys. B367, 28 (1991).
38. T. Kamon, J. L. Lopez, P. McIntyre and J. T. White, Phys. Rev. D 50, 5676 (1994).
39. E. Braaten and J. P. Leveille, Phys. Rev. D 22, 715 (1980).
40. G. L. Kane, C. Kolda and J. D. Wells, Phys. Rev. Lett. 70, 2686 (1993).
41. R. Barbieri and G. F. Giudice, Phys. Lett. B 309, 86 (1993).
42. J. Wu, R. Arnowitt and P. Nath, Phys. Rev. D 51, 1371 (1995).
43. V. Barger, M. S. Berger, P. Ohmann, and R.J. N. Phillips, Phys. Rev. D 51, 2438 (1995).
44. CLEO Collaboration, R. Ammar, et al., Phys. Rev. Lett. 71, 674 (1993).
45. CLEO Collaboration, M. S. Alam, et al., Phys. Rev. Lett. 74, 2885 (1995).
46. A. Buras, M. Misiak, M. Münz and S. Pokorski, Nucl. Phys. B424, 374 (1994).
47. M. Drees and M. Nojiri, Phys. Rev. D 47, 376 (1993).
48. L. Roszkowski, in SUSY '94, Proceedings of the International Workshop on Supersymmetry and Unification of Fundamental Interactions, Ann Arbor, Michigan 1994, edited by C. Kolda and J. D. Wells (University of Michigan, Ann Arbor, 1994), p. 480.
49. R. M. Barnett, J. F. Gunion and H. E. Haber, Phys. Rev. D 37, 1892 (1988);
50. H. Baer, X. Tata and J. Woodside, Phys. Rev. D 41, 906 (1990);
51. H. Baer, X. Tata and J. Woodside, Phys. Rev. D 42, 1450 (1990);
52. A. Bartl, W. Majerotto, B. Mösslacher and N. Oshimo, Z. Phys. C 52, 477 (1991);
53. H. Baer, C. Chen, F. Paige and X. Tata, Phys. Rev. D 52, 2746 (1995).
54. H. Baer, X. Tata and J. Woodside, Phys. Rev. D 45, 142 (1992).
55. J. Ellis and S. Rudaz, Phys. Lett. 128B, 248 (1983).
56. H. Baer, M. Drees, R. Godbole, J. F. Gunion and X. Tata, Phys. Rev. D 44, 725 (1991).
57. H. Baer, J. Sender and X. Tata, Phys. Rev. D 50, 4517 (1994).
58. J. L. Lopez, D. V. Nanopoulos, and A. Zichichi, Report No. CERN TH.7296/96, hep ph/9406254.
59. K. Hidaka, Y. Kizukuri and T. Kon, Phys. Lett. B 278, 155 (1992).