Probing gauge-mediated supersymmetry breaking through polarized electron beams in an [Formula presented] collider

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 56, Issue 1, 1997, Pages 504-507

  Ghosal, Ambar ^a   Kundu, Anirban ^a   Mukhopadhyaya, Biswarup ^a  

^a HARISH CHANDRA RESEARCH INSTITUTE   (India)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001441528     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.56.504     Document Type: Article

References (25)

1. E. Cremmer et al., Nucl. Phys. B212, 43 (1983);
2. For general reviews, see, e.g., H. P. Nilles, Phys. Rep. 110, 1 (1984);
3. H. Haber and G. Kane, 117, 75 (1985);
4. A. Chamseddine, R. Arnowitt, and P. Nath, Applied(Formula presented)Supergravity (World Scientific, Singapore, 1984).
5. For experimental results, see, e.g., A. Acciari et al., Phys. Lett. B 350, 109 (1995).
6. M. Dine, A. E. Nelson, and Y. Shirman, Phys. Rev. D 51, 1362 (1995);
7. M. Dine et al., 53, 2658 (1996);
8. T. Hotta, K.-I. Izawa, and T. Yanagida, 55, 415 (1997);
9. M. Dine, Y. Nir, and Y. Shirman, 55, 1501 (1997);
10. S. P. Martin, 55, 3177 (1997);
11. S. Dimopoulos, S. Thomas, and J. D. Wells, Report No. (unpublished) and references therein.
12. S. Ambrosanio et al., Phys. Rev. Lett. 76, 3498 (1996);
13. S. Dimopoulos et al., 76, 3494 (1996);
14. Nevertheless, other explanations based on conventional SUSY models are suggested in S. Ambrosanio et al., Phys. Rev. D 55, 1372 (1997).
15. S. Dimopoulos, S. Thomas, and J. D. Wells, Phys. Rev. D 54, 3283 (1996);
16. S. Ambrosanio et al., 54, 5395 (1996);
17. H. Baer et al., 55, 4463 (1997).
18. J. Bagger et al., Phys. Rev. D 55, 3188 (1997).
19. K. S. Babu, C. Kolda, and F. Wilczek, Phys. Rev. Lett. 77, 3070 (1996).
20. L. Alvarez-Gaume, M. Claudson, and M. Wise, Nucl. Phys. B207, 96 (1982).
21. D. Stump, M. Wiest, and C. P. Yuan, Phys. Rev. D 54, 1936 (1996).
22. The mass spectrum depends crucially on the messenger scale dynamics. Also, for a strongly interacting messenger sector, right sleptons can naturally become the NLSP; see the first reference in 5.
23. See, e.g., the third reference in 1.
24. A. Czarnecki and W. J. Marciano, Phys. Rev. D 53, 1066 (1996).
25. For SUSY models embedded in GUT theories, the (Formula presented)-term correction is in general small; see, e.g., N. Polonsky and A. Pomarol, Phys. Rev. D 51, 6532 (1995).