QCD corrections to spin correlations in top quark production at lepton colliders

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 59, Issue 1, 1999, Pages

  Parke, Stephen ^b   Nasuno, Takashi ^a  

^a HIROSHIMA UNIVERSITY   (Japan)

^b FERMI NATIONAL ACCELERATOR LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 17144398061     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.59.014023     Document Type: Article

References (40)

1. CDF Collaboration, F. Abe, Phys. Rev. Lett. 74, 2626 (1995).
2. D0 Collaboration, S. AbachiPhys. Rev. Lett. 74, 2632 (1995).
3. J. H. Kühn, Nucl. Phys. B237, 77 (1984).
4. I. Bigi, Y. Dokshizer, V. Khoze, J. Kühn, and P. Zerwas, Phys. Lett. B 181, 157 (1986).
5. M. Jezabek and J. H. Kühn, Phys. Lett. B 329, 317 (1994).
6. V. Barger, J. Ohnemus, and R. J. N. Phillips, Int. J. Mod. Phys. A 4, 617 (1989).
7. G. L. Kane, J. Pumplin, and W. Repko, Phys. Rev. Lett. 41, 1689 (1978);
8. G. L. Kane, G. A. Ladinsky, and C.-P. Yuan, Phys. Rev. D 45, 124 (1992).
9. M. Anselmino, P. Kroll, and B. Pire, Phys. Lett. 167B, 113 (1986);
10. D. Atwood and A. Soni, Phys. Rev. D 45, 2405 (1992);
11. Phys. Rev. DC.-P. Yuan, 45, 782 (1992);
12. Phys. Rev. DG. A. Ladinsky, 46, 3789 (1992);
13. W. Bernreuther, O. Nachtmann, P. Overmann, and T. Schröder, Nucl. Phys. B388, 53 (1992);
14. Nucl. Phys.W. BernreutherO. NachtmannP. OvermannT. SchröderB406, 516(E) (1993);
15. M. E. Peskin, in Physics and Experiments at Linear Colliders, edited by R. Orava, P. Eeorla, and M. Nordberg (World Scientific, Singapore, 1992);
16. T. Arens and L. M. Seghal, Nucl. Phys. B393, 46 (1993);
17. F. Cuypers and S. D. Rindani, Phys. Lett. B 343, 333 (1995);
18. Phys. Lett. BP. Poulose and S. D. Rindani, 349, 379 (1995).
19. C. R. Schmidt and M. E. Peskin, Phys. Rev. Lett. 69, 410 (1992);
20. Phys. Rev. Lett.D. Atwood, A. Aeppli, and A. Soni, 69, 2754 (1992);
21. Y. Hara, Prog. Theor. Phys. 86, 779 (1991);
22. W. Bernreuther and A. Brandenburg, Phys. Rev. D 49, 4481 (1994);
23. Phys. Rev. DP. Haberl, O. Nachtmann, and A. Wilch, 53, 4875 (1996);
24. T. Stelzer and S. Willenbrock, Phys. Lett. B 374, 169 (1996);
25. D. Chang, S.-C. Lee, and A. Sumarokov, Phys. Rev. Lett. 77, 1218 (1996);
26. K. Cheung, Phys. Rev. D 55, 4430 (1997).
27. G. Mahlon and S. Parke, Phys. Rev. D 53, 4886 (1996);
28. G. MahlonS. ParkePhys. Lett. B 411, 173 (1997).
29. S. Parke and Y. Shadmi, Phys. Lett. B 387, 199 (1996).
30. G. Grunberg, Y. J. Ng, and S.-H. H. Tye, Phys. Rev. D 21, 62 (1980);
31. Phys. Rev. DJ. Jersák, E. Laermann, and P. Zerwas, 25, 1218 (1982).
32. S. Groote, J. G. Körner, and J. A. Leyva, Nucl. Phys. B527, 3 (1998).
33. C. R. Schmidt, Phys. Rev. D 54, 3250 (1996);
34. S. D. Rindani and M. M. Tung, Phys. Lett. B 424, 125 (1998);
35. S. Groote, J. G. Körner, and M. M. Tung, Z. Phys. C 70, 281 (1996);
36. M. M. Tung, Phys. Rev. D 52, 1353 (1995);
37. J. G. Körner, A. Pilaftsis, and M. M. Tung, Z. Phys. C 63, 575 (1994).
38. M. M. Tung, J. Bernabeu, and J. Penarrocha, Nucl. Phys. B470, 41 (1996);
39. M. M. Tung, J. Bernabeu, and J. Penarrocha, Phys. Lett. B 418, 181 (1998).
40. R. Harlander and M. Steinhauser, Eur. Phys. J. C 2, 151 (1998).