Subleading form factors at order 1/mQ in terms of leading quantities using the nonforward amplitude in heavy quark effective theory

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 71, Issue 5, 2005, Pages 1-17

  Jugeau, F ^a   Le Yaouanc, A ^a   Oliver, L ^a   Raynal, J C ^a  

^a UNIVERSITÉ PARIS SUD   (France)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; MATHEMATICAL COMPUTING; MODEL; PHENOMENOLOGY; QUARK; THEORY;

EID: 18444410570     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.71.054031     Document Type: Article

References (44)

1. J. D. Bjorken, Report No. SLAC-PUB-5278, 1990 (unpublished).
2. N. Isgur and M. B. Wise, Phys. Rev. D 43, 819 (1991).
3. N. Uraltsev, Phys. Lett. B 501, 86 (2001); N. Uraltsev, J. Phys. G 27, 1081 (2001).
4. N. Uraltsev, Phys. Lett. B 501, 86 (2001); N. Uraltsev, J. Phys. G 27, 1081 (2001).
5. A. Le Yaouanc, L. Oliver, and J.-C. Raynal, Phys. Rev. D 67, 114009 (2003).
6. A. Le Yaouanc, L. Oliver, and J.-C. Raynal, Phys. Lett. B 557, 207 (2003).
7. A. Le Yaouanc, L. Oliver, and J.-C. Raynal, Phys. Rev. D 69, 094022 (2004).
8. A. Falk, Nucl. Phys. B 378, 79 (1992).
9. A. F. Falk et al., Nucl. Phys. B 343, 1 (1990); J. D. Bjorken, in Proceedings of the 18th SLAC Summer Institute on Particle Physics, Stanford, 1990, edited by J. H. F. Hawthorne (SLAC, Stanford, 1991), p. 167.
10. A. F. Falk et al., Nucl. Phys. B 343, 1 (1990); J. D. Bjorken, in Proceedings of the 18th SLAC Summer Institute on Particle Physics, Stanford, 1990, edited by J. H. F. Hawthorne (SLAC, Stanford, 1991), p. 167.
11. A. Falk and M. Neubert, Phys. Rev. D 47, 2965 (1993).
12. A. Leibovich, Z. Ligeti, I. Steward, and M. Wise, Phys. Rev. D 57, 308 (1998).
13. A. Le Yaouanc, D. Melikhov, V. Morénas, L. Oliver, O. Pène, and J.-C. Raynal, Phys. Lett. B 480, 119 (2000).
14. G. Boyd, Z. Ligeti, I. Rothstein, and M. Wise, Phys. Rev. D 55, 3027 (1997).
15. M. P. Dorsten, Phys. Rev. D 70, 096013 (2004).
16. B. Blok, L. Koryakh, M. Shifman, and A. Vainshtein, Phys. Rev. D 49, 3356 (1994).
17. A. Grozin and G. Korchemsky, Phys. Rev. D 53, 1378 (1996).
18. See, for example M. Neubert, hep-ph/0001334.
19. I. Bigi, M. Shifman, N. Uraltsev, and A. Vainshtein, Phys. Rev. D 52, 196 (1995).
20. M. Shifman and M. B. Voloshin, Sov. J. Nucl. Phys. 47, 511 (1988).
21. M. Luke, Phys. Lett. B 252, 447 (1990).
22. M. Voloshin, Phys. Rev. D 46, 3062 (1992).
23. B. Bakamjian and L. H. Thomas, Phys. Rev. 92, 1300 (1953); A. Le Yaouanc, L. Oliver, O. Pène. and J.-C. Raynal, Phys. Lett. B 365, 319 (1996); A. Le Yaouanc, L. Oliver, O. Pène, and J.-C. Raynal, Phys. Lett. B 386, 304 (1996); A. Le Yaouanc, L. Oliver, O. Pène, J.-C. Raynal, and V. Morénas, Phys. Lett. B 520, 25 (2001).
24. B. Bakamjian and L. H. Thomas, Phys. Rev. 92, 1300 (1953); A. Le Yaouanc, L. Oliver, O. Pène. and J.-C. Raynal, Phys. Lett. B 365, 319 (1996); A. Le Yaouanc, L. Oliver, O. Pène, and J.-C. Raynal, Phys. Lett. B 386, 304 (1996); A. Le Yaouanc, L. Oliver, O. Pène, J.-C. Raynal, and V. Morénas, Phys. Lett. B 520, 25 (2001).
25. B. Bakamjian and L. H. Thomas, Phys. Rev. 92, 1300 (1953); A. Le Yaouanc, L. Oliver, O. Pène. and J.-C. Raynal, Phys. Lett. B 365, 319 (1996); A. Le Yaouanc, L. Oliver, O. Pène, and J.-C. Raynal, Phys. Lett. B 386, 304 (1996); A. Le Yaouanc, L. Oliver, O. Pène, J.-C. Raynal, and V. Morénas, Phys. Lett. B 520, 25 (2001).
26. B. Bakamjian and L. H. Thomas, Phys. Rev. 92, 1300 (1953); A. Le Yaouanc, L. Oliver, O. Pène. and J.-C. Raynal, Phys. Lett. B 365, 319 (1996); A. Le Yaouanc, L. Oliver, O. Pène, and J.-C. Raynal, Phys. Lett. B 386, 304 (1996); A. Le Yaouanc, L. Oliver, O. Pène, J.-C. Raynal, and V. Morénas, Phys. Lett. B 520, 25 (2001).
27. S. Godfrey and N. Isgur, Phys. Rev. D 32, 189 (1985).
28. V. Morénas, A. Le Yaouanc, L. Oliver, O. Pène, and J.-C. Raynal, Phys. Rev. D 56, 5668 (1997).
29. V. Morénas et al., Phys. Rev. D 58, 114019 (1998); Vincent Morénas (private communication).
30. V. Morénas et al., Phys. Rev. D 58, 114019 (1998); Vincent Morénas (private communication).
31. I. Bigi, M. Shifman, and N. Uraltsev, Annu. Rev. Nucl. Part. Sci. 47, 591 (1997); N. Uraltsev, J. Phys. G 27, 1081 (2001).
32. I. Bigi, M. Shifman, and N. Uraltsev, Annu. Rev. Nucl. Part. Sci. 47, 591 (1997); N. Uraltsev, J. Phys. G 27, 1081 (2001).
33. M. Neubert, Phys. Rev. D 46, 3914 (1992); M. Neubert, Z. Ligeti, and Y. Nir, Phys. Lett. B 301, 101 (1993); Phys. Rev. D 47, 5060 (1993); Z. Ligeti, Y. Nir, and M. Neubert, Phys. Rev. D 49, 1302 (1994).
34. M. Neubert, Phys. Rev. D 46, 3914 (1992); M. Neubert, Z. Ligeti, and Y. Nir, Phys. Lett. B 301, 101 (1993); Phys. Rev. D 47, 5060 (1993); Z. Ligeti, Y. Nir, and M. Neubert, Phys. Rev. D 49, 1302 (1994).
35. M. Neubert, Phys. Rev. D 46, 3914 (1992); M. Neubert, Z. Ligeti, and Y. Nir, Phys. Lett. B 301, 101 (1993); Phys. Rev. D 47, 5060 (1993); Z. Ligeti, Y. Nir, and M. Neubert, Phys. Rev. D 49, 1302 (1994).
36. M. Neubert, Phys. Rev. D 46, 3914 (1992); M. Neubert, Z. Ligeti, and Y. Nir, Phys. Lett. B 301, 101 (1993); Phys. Rev. D 47, 5060 (1993); Z. Ligeti, Y. Nir, and M. Neubert, Phys. Rev. D 49, 1302 (1994).
37. M. Neubert, Phys. Rep. 245, 259 (1994).
38. B. Grinstein and Z. Ligeti, Phys. Lett. B 526, 345 (2002).
39. BPS = 0 that would give, without including radiative corrections, η(1) = 1/2, another algebraic value for η(1) different from the QCDSR result.
40. We do not enter in the discussion and comparison with the value Λ̄ = 0.40 ± 0.10 found by fitting the data in inclusive B decays, see for example D. Abbaneo et al., CKM Workshop, CERN-2003-002-corr (Chap. 3).
41. Abe et al., Phys. Rev. D 69, 112002 (2004).
42. M. Bataglia, Nucl. Phys. B, Proc. Suppl. 96, 443 (2001); S. Anderson et al., Nucl. Phys. A 663, 545c (2000).
43. M. Bataglia, Nucl. Phys. B, Proc. Suppl. 96, 443 (2001); S. Anderson et al., Nucl. Phys. A 663, 545c (2000).
44. M. Beneke, G. Buchalla, M. Neubert, and G. Sachrajda, Nucl. Phys. B 591, 313 (2000).