Constraints from electric dipole moments on chargino baryogenesis in the minimal supersymmetric standard model

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 66, Issue 11, 2002, Pages

  Keung, Wai Yee ^a  

^a NATIONAL TSING HUA UNIVERSITY   (Taiwan)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; BARYON; DIPOLE; ELECTRICITY; ELECTRON; ELEMENTARY PARTICLE; MATHEMATICAL ANALYSIS; MODEL; NEUTRON; PHYSICS;

EID: 0036990002     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.66.116008     Document Type: Article

References (54)

1. H.P. Nilles, Phys. Rep. 110, 1 (1984);
2. Phys. Rep.H. Haber and G. Kane, 117, 75 (1985);
3. S. Dawson, hep-ph/9612229;
4. M. Drees, hep-ph/9611409;
5. M. Peskin, hep-ph/9705479;
6. S. Martin, hep-ph/9709356; among others.
7. G.R. Farrar and M.E. Shaposhnikov, Phys. Rev. D 50, 774 (1994).
8. M. Carena, M. Quiros, and C.E. Wagner, Phys. Lett. B 380, 81 (1996);
9. M. Carena, J.M. Moreno, M. Quiros, M. Seco, and C.E. Wagner, Nucl. Phys. B599, 158 (2001);
10. Nucl. Phys.M. Carena, M. Quiros, A. Riotto, I. Vilja, and C.E. Wagner, B503, 387 (1997);
11. J.M. Cline, M. Joyce, and K. Kainulainen, Phys. Lett. B 417, 79 (1998);
12. Phys. Lett. BJ.M. ClineM. JoyceK. Kainulainen448, 321(E) (1998);
13. J.M. ClineM. JoyceK. KainulainenJ. High Energy Phys. 07, 018 (2000);
14. J.M. ClineM. JoyceK. Kainulainenhep-ph/0110031(erratum);
15. S.J. Huber, P. John, and M.G. Schmidt, Eur. Phys. J. C 20, 695 (2001);
16. P. Huet and A.E. Nelson, Phys. Rev. D 53, 4578 (1996);
17. M. Quiros, Nucl. Phys. B (Proc. Suppl.) 101, 401 (2001);
18. M. Aoki, N. Oshimo, and A. Sugamoto, Prog. Theor. Phys. 98, 1179 (1997);
19. Prog. Theor. Phys.M. AokiN. OshimoA. Sugamoto98, 1325 (1997).
20. Y. Kizukuri and N. Oshimo, Phys. Rev. D 46, 3025 (1992);
21. J. Ellis, S. Ferrara, and D.V. Nanopoulos, Phys. Lett. 114B, 231 (1982);
22. Phys. Lett.W. Buchmüller and D. Wyler, 121B, 321 (1983);
23. Phys. Lett.J. Polchinski and M. Wise, 125B, 393 (1983);
24. Phys. Lett.F. del Aguila, M. Gavela, J. Grifols, and A. Mendez, 126B, 71 (1983);
25. Phys. Lett.D.V. Nanopoulos and M. Srednicki, 128B, 61 (1983);
26. M. Dugan, B. Grinstein, and L. Hall, Nucl. Phys. B255, 413 (1985).
27. T. Ibrahim and P. Nath, Phys. Rev. D 57, 478 (1998);
28. Phys. Rev. DT. IbrahimP. Nath58, 019901(E) (1998).
29. S. Abel, S. Khalil, and O. Lebedev, Nucl. Phys. B606, 151 (2001).
30. A.G. Cohen, D.B. Kaplan, and A.E. Nelson, Phys. Lett. B 388, 588 (1996).
31. D. Chang, W.-Y. Keung, and A. Pilaftsis, Phys. Rev. Lett. 82, 900 (1999);
32. Phys. Rev. Lett.D. ChangW.-Y. KeungA. Pilaftsis83, 3972 (1999).
33. The contribution of the chargino loop was pointed out in this paper, but detailed analysis was only given to the top-squark loop contribution. See also D. Chang, W.-F. Chang, and W.-Y. Keung, Phys. Lett. B 478, 239 (2000);
34. Phys. Lett. BA. Pilaftsis, 471, 174 (1999).
35. S.M. Barr and A. Zee, Phys. Rev. Lett. 65, 21 (1990).
36. D. Chang, W.Y. Keung, and T.C. Yuan, Phys. Rev. D 43, 14 (1991);
37. R.G. Leigh, S. Paban, and R.M. Xu, Nucl. Phys. B352, 45 (1991);
38. C. Kao and R.-M. Xu, Phys. Lett. B 296, 435 (1992);
39. D. Chang, W.-S Hou, and W.-Y. Keung, Phys. Rev. D 48, 217 (1993);
40. Phys. Rev. DD. Chang, W.-F. Chang, C.-H. Chou, and W.-Y. Keung, 63, 091301(R) (2001).
41. D. Chang, W.-Y. Keung, and T.C. Yuan, Phys. Lett. B 251, 608 (1990);
42. Phys. Lett. BJ.F. Gunion and D. Wyler, 248, 170 (1990);
43. D. Chang, W.-F. Chang, M. Frank, and W.-Y. Keung, Phys. Rev. D 62, 095002 (2000).
44. T. Kadoyoshi and N. Oshimo, Phys. Rev. D 55, 1481 (1997). This paper also used the same CP violating source from the chargino mixing; however, their two-loop amplitudes are not the dominant ones.
45. H.E. Haber, R. Hempfling, and A.H. Hoang, Z. Phys. C 75, 539 (1997).
46. B.C. Regan, Phys. Rev. Lett. 88, 071805 (2002).
47. For a review, see J.M. Cline, Pramana 54, 1 (2000);
48. PramanaJ.M. Cline55, 33 (2000); and Ref. 16.
49. H. Murayama and A. Pierce, hep-ph/0201261.
50. J.M. Cline, hep-ph/0201286.
51. P.G. Harris, Phys. Rev. Lett. 82, 904 (1999).
52. K.F. Smith, Phys. Lett. B 234, 191 (1990).
53. S.K. Lamoreaux and R. Golub, Phys. Rev. D 61, 051301(R) (2000).
54. M. Carena, M. Quiros, M. Seco, and C.E.M. Wagner, hep-ph/0208043.