Academia.eduAcademia.edu

Outline

Model Independent Results for Heavy Quarkonium

2004, Modern Physics Letters A

https://doi.org/10.1142/S0217732304014690

Abstract

We review a number of results for the spectrum and inclusive decays of heavy quarkonium systems which can be derived from QCD under well controlled approximations. They essentially follow from the hierarchy of scales in these systems, which can be efficiently exploited using non-relativistic effective field theories. In particular, we discuss under which conditions non-relativistic potential models emerge as effective theories of QCD.

References (81)

  1. J. J. Aubert et al., Phys. Rev. Lett. 33 (1974) 1404;
  2. J. E. Augustin et al., Phys. Rev. Lett. 33 (1974) 1406.
  3. S. W. Herb et al., Phys. Rev. Lett. 39 (1977) 252.
  4. T. Appelquist and H. D. Politzer, Phys. Rev. Lett. 34 (1975) 43.
  5. K. G. Wilson, Phys. Rev. D 10 (1974) 2445.
  6. M. B. Voloshin, Nucl. Phys. B 154 (1979) 365; Sov. J. Nucl. Phys. 36 (1982) 143 [Yad. Fiz. 36 (1982) 247];
  7. H. Leutwyler, Phys. Lett. B 98 (1981) 447.
  8. W. Lucha, F. F. Schoberl and D. Gromes, Phys. Rept. 200 (1991) 127.
  9. L. Susskind, in Les Houches, Session XXIX, ed. R. Balian and C. H. Llewellyn Smith (North-Holland Publishing Company, Amsterdam, 1977);
  10. W. Fischler, Nucl. Phys. B 129, 157 (1977);
  11. L. S. Brown and W.I. Weisberger, Phys. Rev. D 20, 3239 (1979);
  12. E. Eichten and F. L. Feinberg, Phys. Rev. D 23, 2724 (1981);
  13. M. E. Peskin, in Proceeding of the 11th SLAC Institute, SLAC Report No. 207, 151, edited by P. Mc Donough (1983);
  14. D. Gromes, Z. Phys. C 26, 401 (1984);
  15. A. Barchielli, E. Montaldi and G. M. Prosperi, Nucl. Phys. B 296, 625 (1988); (E) ibid. 303, 752 (1988);
  16. A. Barchielli, N. Brambilla and G. Prosperi, Nuovo Cimento 103 A, 59 (1990).
  17. S.N. Gupta, S.F. Radford and W.W. Repko, Phys. Rev. D26 3305 (1982).
  18. R. Barbieri, R. Gatto and R. Kogerler, Phys. Lett. B 60 (1976) 183;
  19. R. Barbieri, R. Gatto and E. Remiddi, Phys. Lett. B 61 (1976) 465; Nucl. Phys. B 162 (1980) 220;
  20. R. Barbieri, M. Caffo, R. Gatto and E. Remiddi, Phys. Lett. B 95 (1980) 93. Nucl. Phys. B 192 (1981) 61.
  21. W. E. Caswell and G. P. Lepage, Phys. Lett. B 167 (1986) 437; B. A. Thacker and G. P. Lepage, Phys. Rev. D 43 (1991) 196; G. T. Bodwin, E. Braaten and G. P. Lepage, Phys. Rev. D 51 (1995) 1125 [Erratum-ibid. D 55 (1997) 5853] [arXiv:hep-ph/9407339].
  22. G. T. Bodwin, E. Braaten and G. P. Lepage, Phys. Rev. D 46 (1992) 1914 [arXiv:hep-lat/9205006].
  23. Y. Q. Chen, Y. P. Kuang and R. J. Oakes, Phys. Rev. D 52 (1995) 264 [arXiv:hep-ph/9406287].
  24. G. Bonvicini [CLEO Collaboration], arXiv:hep-ex/0404021;
  25. S. E. Csorna et al. [CLEO Collaboration], arXiv:hep-ex/0207060; J. Z. Bai et al. [BES Collaboration], Phys. Lett. B 550 (2002) 24 [arXiv:hep-ph/0209354].
  26. S. K. Choi et al. [Belle Collaboration], Phys. Rev. Lett. 91 (2003) 262001 [arXiv:hep-ex/0309032];
  27. K. Abe et al. [Belle Collaboration], Phys. Rev. Lett. 89 (2002) 142001 [arXiv:hep-ex/0205104].
  28. G. S. Bali, Phys. Rept. 343 (2001) 1 [arXiv:hep-ph/0001312].
  29. T. Skwarnicki, Int. J. Mod. Phys. A 19 (2004) 1030 [arXiv:hep-ph/0311243].
  30. A. V. Manohar, Phys. Rev. B 56, 230 (1997) [arXiv:hep-ph/9701294].
  31. A. Pineda and J. Soto, Phys. Rev. D 58, 114011 (1998) [arXiv:hep-ph/9802365].
  32. M. E. Luke and A. V. Manohar, Phys. Lett. B 286 (1992) 348 [arXiv:hep-ph/9205228].
  33. N. Brambilla, D. Gromes and A. Vairo, Phys. Lett. B 576 (2003) 314 [arXiv:hep-ph/0306107].
  34. A. Vairo, Mod. Phys. Lett. A 19 (2004) 253 [arXiv:hep-ph/0311303].
  35. A. Petrelli, M. Cacciari, M. Greco, F. Maltoni and M. L. Mangano, Nucl. Phys. B 514 (1998) 245 [arXiv:hep-ph/9707223].
  36. S. Fleming and A. K. Leibovich, Phys. Rev. D 67 (2003) 074035 [arXiv:hep-ph/0212094].
  37. G. T. Bodwin, arXiv:hep-ph/0312173.
  38. A. Pineda and J. Soto, Nucl. Phys. Proc. Suppl. 64 (1998) 428 [arXiv:hep-ph/9707481].
  39. N. Brambilla, A. Pineda, J. Soto and A. Vairo, Nucl. Phys. B 566 (2000) 275 [arXiv:hep-ph/9907240].
  40. N. Brambilla, D. Eiras, A. Pineda, J. Soto and A. Vairo, Phys. Rev. D 67 (2003) 034018 [arXiv:hep-ph/0208019].
  41. A. Pineda and J. Soto, Phys. Lett. B 420 (1998) 391 [arXiv:hep-ph/9711292];
  42. Phys. Rev. D 59 (1999) 016005 [arXiv:hep-ph/9805424].
  43. A. Czarnecki, K. Melnikov and A. Yelkhovsky, Phys. Rev. A 59 (1999) 4316 [arXiv:hep-ph/9901394].
  44. A. Pineda and F. J. Yndurain, Phys. Rev. D 58 (1998) 094022 [arXiv:hep-ph/9711287];
  45. Phys. Rev. D 61 (2000) 077505 [arXiv:hep-ph/9812371].
  46. K. Melnikov and A. Yelkhovsky, Nucl. Phys. B 528 (1998) 59 [arXiv:hep-ph/9802379];
  47. A. A. Penin and A. A. Pivovarov, Phys. Atom. Nucl. 64 (2001) 275 [Yad. Fiz. 64 (2001) 323] [arXiv:hep-ph/9904278].
  48. A. H. Hoang et al., Eur. Phys. J. directC 2 (2000) 3 [arXiv:hep-ph/0001286].
  49. Y. Schroder, Phys. Lett. B 447 (1999) 321 [arXiv:hep-ph/9812205];
  50. M. Peter, Nucl. Phys. B 501 (1997) 471 [arXiv:hep-ph/9702245].
  51. A. Pineda, Nucl. Phys. B 494 (1997) 213 [arXiv:hep-ph/9611388].
  52. N. Brambilla, A. Pineda, J. Soto and A. Vairo, Phys. Lett. B 470 (1999) 215 [arXiv:hep-ph/9910238].
  53. B. A. Kniehl, A. A. Penin, M. Steinhauser and V. A. Smirnov, Phys. Rev. D 65 (2002) 091503 [arXiv:hep-ph/0106135];
  54. Nucl. Phys. B 635 (2002) 357 [arXiv:hep-ph/0203166];
  55. A. A. Penin and M. Steinhauser, Phys. Lett. B 538 (2002) 335 [arXiv:hep-ph/0204290].
  56. M. E. Luke, A. V. Manohar and I. Z. Rothstein, Phys. Rev. D 61 (2000) 074025 [arXiv:hep-ph/9910209];
  57. A. V. Manohar and I. W. Stewart, Phys. Rev. D 62 (2000) 014033 [arXiv:hep-ph/9912226].
  58. A. Pineda, Phys. Rev. D 65 (2002) 074007 [arXiv:hep-ph/0109117];
  59. Phys. Rev. A 66 (2002) 062108 [arXiv:hep-ph/0204213].
  60. A. Pineda, Phys. Rev. D 66 (2002) 054022 [arXiv:hep-ph/0110216].
  61. A. H. Hoang and I. W. Stewart, Phys. Rev. D 67 (2003) 114020 [arXiv:hep-ph/0209340].
  62. B. A. Kniehl, A. A. Penin, A. Pineda, V. A. Smirnov and M. Steinhauser, arXiv:hep-ph/0312086; A. A. Penin, A. Pineda, V. A. Smirnov and M. Steinhauser, arXiv:hep-ph/0403080.
  63. B. A. Kniehl and A. A. Penin, Nucl. Phys. B 577 (2000) 197 [arXiv:hep-ph/9911414].
  64. B. A. Kniehl, A. A. Penin, M. Steinhauser and V. A. Smirnov, Phys. Rev. Lett. 90 (2003) 212001 [arXiv:hep-ph/0210161].
  65. A. Pineda, Acta Phys. Polon. B 34 (2003) 5295.
  66. X. Garcia i Tormo and J. Soto, arXiv:hep-ph/0401233.
  67. N. Brambilla, D. Gromes and A. Vairo, Phys. Rev. D 64 (2001) 076010 [arXiv:hep-ph/0104068].
  68. N. Brambilla, A. Pineda, J. Soto and A. Vairo, Phys. Rev. D 63 (2001) 014023 [arXiv:hep-ph/0002250];
  69. A. Pineda and A. Vairo, Phys. Rev. D 63 (2001) 054007 [Erratum-ibid. D 64 (2001) 039902] [arXiv:hep-ph/0009145].
  70. N. Brambilla, A. Pineda, J. Soto and A. Vairo, Phys. Lett. B 580 (2004) 60 [arXiv:hep-ph/0307159].
  71. G. S. Bali, K. Schilling and A. Wachter, Phys. Rev. D 56 (1997) 2566 [arXiv:hep-lat/9703019].
  72. N. Brambilla and A. Vairo, arXiv:hep-ph/9904330.
  73. F. Jugeau and H. Sazdjian, Nucl. Phys. B 670 (2003) 221 [arXiv:hep-ph/0305021].
  74. N. Brambilla, D. Eiras, A. Pineda, J. Soto and A. Vairo, Phys. Rev. Lett. 88 (2002) 012003 [arXiv:hep-ph/0109130].
  75. D. Cinabro et al. [CLEO Collaboration], arXiv:hep-ex/0207062.
  76. A. Pineda, JHEP 0106 (2001) 022 [arXiv:hep-ph/0105008].
  77. N. Brambilla, Y. Sumino and A. Vairo, Phys. Lett. B 513 (2001) 381 [arXiv:hep-ph/0101305];
  78. Phys. Rev. D 65 (2002) 034001 [arXiv:hep-ph/0108084];
  79. S. Recksiegel and Y. Sumino, Phys. Lett. B 578 (2004) 369 [arXiv:hep-ph/0305178].
  80. N. Brambilla and A. Vairo, Phys. Rev. D 62 (2000) 094019 [arXiv:hep-ph/0002075].
  81. M. Neubert, Phys. Rept. 245 (1994) 259 [arXiv:hep-ph/9306320].