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Volumn 19, Issue 7, 2004, Pages 1030-1045

Heavy quarkonium

Author keywords

[No Author keywords available]

Indexed keywords

HADRON; MOLECULAR DYNAMICS; MOLECULAR INTERACTION; MOLECULAR PHYSICS; PHASE TRANSITION; PHOTON; QUANTUM MECHANICS; QUARK; REVIEW;

EID: 3142703503     PISSN: 0217751X     EISSN: None     Source Type: Journal    
DOI: 10.1142/S0217751X04018956     Document Type: Review
Times cited : (30)

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    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
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    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
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    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
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    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
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    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
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    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
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    • 0.80
    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
    • (1982) Z. Phys. , vol.C13 , pp. 131
    • Baacke, J.1    Igarashi, Y.2    Kasperidus, G.3
  • 63
    • 0003169269 scopus 로고
    • 0.83
    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
    • (1986) Phys. Rev. , vol.D34 , pp. 201
    • Gupta, S.N.1    Radford, S.F.2    Repko, W.W.3
  • 64
    • 0037286711 scopus 로고    scopus 로고
    • 0.84
    • HF given in square brackets. H. Ito, Prog. of Theor. Phys. 84, 94 (1990) [0.29]; T. A. Lahde, Nucl. Phys. A714, 183 (2003) [0.37]; S. Godfrey, N.Isgur, Phys. Rev. D32, 189 (1985) [0.46]; S. N. Jena, Phys. Lett. B123, 445 (1983) [0.48]; J. Carlson, J. B. Kogut, V.R.Pandharipande, Phys. Rev. D28, 2807 (1983) [0.55]; T. A. Lahde, C. J. Nyfalt, D. O. Riska Nucl. Phys. A645, 587 (1999) [0.56]; S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989) [0.61]; D. Beavis, S.-Y. Chu, B. R. Desai, P. Kaus, Phys. Rev. D20, 2345 (1979) [0.62]; N. Barik, S. N. Jena, Phys. Rev. D24, 680 (1981) [0.70]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984) [0.73]; L. P. Fulcher, Phys. Rev. D44, 2079 (1991) [0.74]; J. S. Kang, Phys. Rev. D20, 2978 (1979) [0.76]; J. Baacke, Y. Igarashi, G. Kasperidus Z. Phys. C13, 131 (1982) [0.80]; S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986) [0.83]; D. Ebert, R. N. Faustov, and V. O. Galkin Phys. Rev. D67, 014027 (2003) [0.84].
    • (2003) Phys. Rev. , vol.D67 , pp. 014027
    • Ebert, D.1    Faustov, R.N.2    Galkin, V.O.3
  • 66
    • 84888917616 scopus 로고    scopus 로고
    • S. Recksiegel, Y. Sumino, TU-691, TUM-HEP-508-03, hep-ph/0305178
    • S. Recksiegel, Y. Sumino, TU-691, TUM-HEP-508-03, hep-ph/0305178.
  • 67
    • 3843122952 scopus 로고    scopus 로고
    • M. Okamoto et al. (CP-PACS Collaboration) Phys. Rev. D65, 094508 (2002).
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    • Okamoto, M.1
  • 68
    • 0037187762 scopus 로고    scopus 로고
    • b in two-photon collisions with the DELPHI detector", #62.
    • (2002) Phys. Lett. , vol.B530 , pp. 56
    • Heister, A.1
  • 70
    • 0003467992 scopus 로고
    • The following sample of potential model predictions for the M1 matrix elements (ordered according to the publication date) is displayed in Fig. 8: V. Zambetakis, N.Byers, Phys. Rev. D28, 2908 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev., D30, 1924 (1984) (2 entries: scalar and vector confinement potential); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985) (2 entries: based on quoted transition moments and wave functions respectively); X. Zhang, K. J. Sebastian, H. Grotch, Phys. Rev. D44, 1606 (1991) (2 entries: scalar-vector and pure scalar confinement potential); D. Ebert, R. N. Faustov, V. O. Galkin Phys. Rev. D67, 014027 (2003); T. A. Lahde, Nucl. Phys. A714, 183(2003) (2 entries: without and with exchange currents). Values of the M1 matrix elements in the bb̄ system are displayed for the photon energies and b quark mass assumed in S. Godfrey, J. L. Rosner, Phys. Rev. D64, 074011 (2001), Erratum-ibid. D65, 039901 (2002).
    • (1983) Phys. Rev. , vol.D28 , pp. 2908
    • Zambetakis, V.1    Byers, N.2
  • 71
    • 0000389717 scopus 로고
    • 2 entries: scalar and vector confinement potential
    • The following sample of potential model predictions for the M1 matrix elements (ordered according to the publication date) is displayed in Fig. 8: V. Zambetakis, N.Byers, Phys. Rev. D28, 2908 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev., D30, 1924 (1984) (2 entries: scalar and vector confinement potential); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985) (2 entries: based on quoted transition moments and wave functions respectively); X. Zhang, K. J. Sebastian, H. Grotch, Phys. Rev. D44, 1606 (1991) (2 entries: scalar-vector and pure scalar confinement potential); D. Ebert, R. N. Faustov, V. O. Galkin Phys. Rev. D67, 014027 (2003); T. A. Lahde, Nucl. Phys. A714, 183(2003) (2 entries: without and with exchange currents). Values of the M1 matrix elements in the bb̄ system are displayed for the photon energies and b quark mass assumed in S. Godfrey, J. L. Rosner, Phys. Rev. D64, 074011 (2001), Erratum-ibid. D65, 039901 (2002).
    • (1984) Phys. Rev. , vol.D30 , pp. 1924
    • Grotch, H.1    Owen, D.A.2    Sebastian, K.J.3
  • 72
    • 4243827703 scopus 로고
    • 2 entries: based on quoted transition moments and wave functions respectively
    • The following sample of potential model predictions for the M1 matrix elements (ordered according to the publication date) is displayed in Fig. 8: V. Zambetakis, N.Byers, Phys. Rev. D28, 2908 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev., D30, 1924 (1984) (2 entries: scalar and vector confinement potential); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985) (2 entries: based on quoted transition moments and wave functions respectively); X. Zhang, K. J. Sebastian, H. Grotch, Phys. Rev. D44, 1606 (1991) (2 entries: scalar-vector and pure scalar confinement potential); D. Ebert, R. N. Faustov, V. O. Galkin Phys. Rev. D67, 014027 (2003); T. A. Lahde, Nucl. Phys. A714, 183(2003) (2 entries: without and with exchange currents). Values of the M1 matrix elements in the bb̄ system are displayed for the photon energies and b quark mass assumed in S. Godfrey, J. L. Rosner, Phys. Rev. D64, 074011 (2001), Erratum-ibid. D65, 039901 (2002).
    • (1985) Phys. Rev. , vol.D32 , pp. 189
    • Godfrey, S.1    Isgur, N.2
  • 73
    • 0000823821 scopus 로고
    • 2 entries: scalar-vector and pure scalar confinement potential
    • The following sample of potential model predictions for the M1 matrix elements (ordered according to the publication date) is displayed in Fig. 8: V. Zambetakis, N.Byers, Phys. Rev. D28, 2908 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev., D30, 1924 (1984) (2 entries: scalar and vector confinement potential); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985) (2 entries: based on quoted transition moments and wave functions respectively); X. Zhang, K. J. Sebastian, H. Grotch, Phys. Rev. D44, 1606 (1991) (2 entries: scalar-vector and pure scalar confinement potential); D. Ebert, R. N. Faustov, V. O. Galkin Phys. Rev. D67, 014027 (2003); T. A. Lahde, Nucl. Phys. A714, 183(2003) (2 entries: without and with exchange currents). Values of the M1 matrix elements in the bb̄ system are displayed for the photon energies and b quark mass assumed in S. Godfrey, J. L. Rosner, Phys. Rev. D64, 074011 (2001), Erratum-ibid. D65, 039901 (2002).
    • (1991) Phys. Rev. , vol.D44 , pp. 1606
    • Zhang, X.1    Sebastian, K.J.2    Grotch, H.3
  • 74
    • 0037286711 scopus 로고    scopus 로고
    • The following sample of potential model predictions for the M1 matrix elements (ordered according to the publication date) is displayed in Fig. 8: V. Zambetakis, N.Byers, Phys. Rev. D28, 2908 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev., D30, 1924 (1984) (2 entries: scalar and vector confinement potential); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985) (2 entries: based on quoted transition moments and wave functions respectively); X. Zhang, K. J. Sebastian, H. Grotch, Phys. Rev. D44, 1606 (1991) (2 entries: scalar-vector and pure scalar confinement potential); D. Ebert, R. N. Faustov, V. O. Galkin Phys. Rev. D67, 014027 (2003); T. A. Lahde, Nucl. Phys. A714, 183(2003) (2 entries: without and with exchange currents). Values of the M1 matrix elements in the bb̄ system are displayed for the photon energies and b quark mass assumed in S. Godfrey, J. L. Rosner, Phys. Rev. D64, 074011 (2001), Erratum-ibid. D65, 039901 (2002).
    • (2003) Phys. Rev. , vol.D67 , pp. 014027
    • Ebert, D.1    Faustov, R.N.2    Galkin, V.O.3
  • 75
    • 0037428956 scopus 로고    scopus 로고
    • 2 entries: without and with exchange currents
    • The following sample of potential model predictions for the M1 matrix elements (ordered according to the publication date) is displayed in Fig. 8: V. Zambetakis, N.Byers, Phys. Rev. D28, 2908 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev., D30, 1924 (1984) (2 entries: scalar and vector confinement potential); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985) (2 entries: based on quoted transition moments and wave functions respectively); X. Zhang, K. J. Sebastian, H. Grotch, Phys. Rev. D44, 1606 (1991) (2 entries: scalar-vector and pure scalar confinement potential); D. Ebert, R. N. Faustov, V. O. Galkin Phys. Rev. D67, 014027 (2003); T. A. Lahde, Nucl. Phys. A714, 183(2003) (2 entries: without and with exchange currents). Values of the M1 matrix elements in the bb̄ system are displayed for the photon energies and b quark mass assumed in S. Godfrey, J. L. Rosner, Phys. Rev. D64, 074011 (2001), Erratum-ibid. D65, 039901 (2002).
    • (2003) Nucl. Phys. , vol.A714 , pp. 183
    • Lahde, T.A.1
  • 76
    • 0035478226 scopus 로고    scopus 로고
    • Erratum-ibid. D65, 039901 (2002)
    • The following sample of potential model predictions for the M1 matrix elements (ordered according to the publication date) is displayed in Fig. 8: V. Zambetakis, N.Byers, Phys. Rev. D28, 2908 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev., D30, 1924 (1984) (2 entries: scalar and vector confinement potential); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985) (2 entries: based on quoted transition moments and wave functions respectively); X. Zhang, K. J. Sebastian, H. Grotch, Phys. Rev. D44, 1606 (1991) (2 entries: scalar-vector and pure scalar confinement potential); D. Ebert, R. N. Faustov, V. O. Galkin Phys. Rev. D67, 014027 (2003); T. A. Lahde, Nucl. Phys. A714, 183(2003) (2 entries: without and with exchange currents). Values of the M1 matrix elements in the bb̄ system are displayed for the photon energies and b quark mass assumed in S. Godfrey, J. L. Rosner, Phys. Rev. D64, 074011 (2001), Erratum-ibid. D65, 039901 (2002).
    • (2001) Phys. Rev. , vol.D64 , pp. 074011
    • Godfrey, S.1    Rosner, J.L.2
  • 77
    • 14244265433 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1978) Phys. Lett. , vol.74 B , pp. 108
    • Pignon, D.1    Piketty, C.A.2
  • 78
    • 4243346296 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1980) Phys. Rev. , vol.D21 , pp. 203
    • Eichten, E.1    Gottfried, K.2    Kinoshita, T.3    Lane, K.D.4    Yan, T.M.5
  • 79
    • 4243432310 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1980) Phys. Rev. Lett. , vol.45 , pp. 103
    • Buchmuller, W.1    Grunberg, G.2    Tye, S.-H.3
  • 80
    • 14244250431 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1981) Phys. Rev. , vol.D24 , pp. 132
  • 81
    • 0000447929 scopus 로고
    • 2 entries: cc̄, bb̄ potential respectively
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1981) Phys. Rev. , vol.D23 , pp. 2625
    • Quigg, C.1    Rosner, J.L.2
  • 82
    • 0039996723 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1982) Z. Phys. , vol.C13 , pp. 131
    • Baacke, J.1    Igarashi, Y.2    Kasperidus, G.3
  • 83
    • 0001195170 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1983) Phys. Rev. , vol.D28 , pp. 1692
    • McClary, R.1    Byers, N.2
  • 84
    • 0000623937 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1983) Phys. Rev. , vol.D28 , pp. 1132
    • Moxhay, P.1    Rosner, J.L.2
  • 85
    • 0000389717 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1984) Phys. Rev. , vol.D30 , pp. 1924
    • Grotch, H.1    Owen, D.A.2    Sebastian, K.J.3
  • 86
    • 33744680044 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1982) Phys. Rev. , vol.D26 , pp. 3305
    • Gupta, S.N.1    Radford, S.F.2    Repko, W.W.3
  • 87
    • 22444432441 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1984) Phys. Rev. , vol.D30 , pp. 2424
  • 88
    • 0003169269 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1986) Phys. Rev. , vol.D34 , pp. 201
    • Gupta, S.N.1    Radford, S.F.2    Repko, W.W.3
  • 89
    • 11144350646 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1984) Phys. Lett. , vol.B134 , pp. 258
    • Bander, M.1    Silverman, D.2    Klima, B.3    Maor, U.4
  • 90
    • 11144261171 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D.
    • (1984) Phys. Rev. , vol.D29 , pp. 2038
  • 91
    • 22444450844 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1987) Phys. Rev. , vol.D36 , pp. 3401
  • 92
    • 0001635964 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1988) Phys. Rev. , vol.D38 , pp. 279
    • Kwong, W.1    Rosner, J.L.2
  • 93
    • 14244265433 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1988) Phys. Rev. , vol.D37 , pp. 1259
    • Fulcher, L.P.1
  • 94
    • 25044440928 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
    • (1989) Phys. Rev. , vol.D39 , pp. 974
    • Gupta, S.N.1    Repko, W.W.2    Suchyta III, C.J.3
  • 95
    • 26744435216 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
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    • Fulcher, L.P.1
  • 96
    • 0001573955 scopus 로고
    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
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    • Grant, A.K.1    Rosener, J.L.2    Rynes, E.3
  • 97
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    • The following sample of potential model predictions for the E1 matrix elements (ordered according to the publication date) is displayed in Fig. 9: D. Pignon, C. A. Piketty, Phys. Lett. 74B, 108 (1978); E. Eichten, K. Gottfried, T. Kinoshita, K. D. Lane, T. M. Yan, Phys. Rev. D21, 203 (1980); W. Buchmuller, G. Grunberg, S.-H. Tye Phys. Rev. Lett. 45, 103 (1980), Phys. Rev. D24, 132 (1981); C. Quigg, J. L. Rosner, Phys. Rev. D23, 2625 (1981) (2 entries: cc̄, bb̄ potential respectively); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982); R. McClary, N. Byers, Phys. Rev. D28, 1692 (1983); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); H. Grotch, D. A. Owen, K. J. Sebastian, Phys. Rev. D30, 1924 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D26, 3305 (1982), Phys. Rev. D30, 2424 (1984); S. N. Gupta, S. F. Radford, W. W. Repko, Phys. Rev. D34, 201 (1986); M. Bander, D. Silverman, B. Klima, U. Maor, Phys. Lett. B134, 258 (1984), Phys. Rev. D29, 2038 (1984), Phys. Rev. D36, 3401 (1987); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P. Fulcher, Phys. Rev. D37, 1259 (1988); S. N. Gupta, W. W. Repko, C. J. Suchyta III, Phys. Rev. D39, 974 (1989); L. P. Fulcher, Phys. Rev. D42, 2337 (1990); A. K. Grant, J. L. Rosener, E. Rynes, Phys. Rev. D47, 1981 (1993); T. A. Lahde, Nucl. Phys. A714, 183(2003).
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    • Lahde, T.A.1
  • 99
  • 101
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    • H. Severini et al. (CLEO), CLEO-CONF-03-06, contributed to Lepton Photon 2003, hep-ex/0307034
    • H. Severini et al. (CLEO), CLEO-CONF-03-06, contributed to Lepton Photon 2003, hep-ex/0307034
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    • M. B. Voloshin Nucl. Phys. B154, 365 (1979); M. B. Voloshin, V. Zakharov Phys. Rev. Lett. 45, 688 (1980); V. A. Novikov, M. A. Shifman, Z. Phys. 8, 43 (1981); M. B. Voloshin Pisma Zh. Eksp. Teor. Fiz. 37, 58 (1983) [JETP Lett. 37, 69 (1983)].
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    • 84888909751 scopus 로고    scopus 로고
    • private communication
    • CLEO collaboration, private communication.
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    • 17044413663 scopus 로고    scopus 로고
    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
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    • Ebert, D.1    Faustov, R.N.2    Galkin, V.O.3
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    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
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    • Kwong, W.1    Rosner, J.L.2
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    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
    • (1990) Phys. Rev. , vol.D42 , pp. 2337
    • Fulcher, L.P.1
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    • 0000623937 scopus 로고
    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
    • (1983) Phys. Rev. , vol.D28 , pp. 1132
    • Moxhay, P.1    Rosner, J.L.2
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    • 18044374246 scopus 로고
    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
    • (1991) Phys. Rev. , vol.D44 , pp. 2079
    • Fulcher, L.P.1
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    • 4243827703 scopus 로고
    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
    • (1985) Phys. Rev. , vol.D32 , pp. 189
    • Godfrey, S.1    Isgur, N.2
  • 117
    • 30244486708 scopus 로고
    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
    • (1981) Phys. Rev. , vol.D23 , pp. 2724
    • Eichten, E.1    Feinberg, F.2
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    • 0037428956 scopus 로고    scopus 로고
    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
    • (2003) Nucl. Phys. , vol.A714 , pp. 183
    • Lahde, T.A.1
  • 119
    • 17044364884 scopus 로고
    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
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    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
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    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
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    • Lahde, T.A.1    Nyfalt, C.J.2    Riska, D.O.3
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    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
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    • Kang, J.S.1
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    • cog)) is displayed in Fig. 11: D. Ebert, R. N. Faustov, V. O. Galkin, Phys. Rev. D62, 034014 (2000); W. Kwong, J. L. Rosner, Phys. Rev. D38, 279 (1988); L. P.Fulcher, Phys. Rev. D42, 2337 (1990); P. Moxhay, J. L. Rosner, Phys. Rev. D28, 1132 (1983); L. P. Fulcher, Phys. Rev. D44, 2079 (1991); S. Godfrey, N. Isgur, Phys. Rev. D32, 189 (1985); E. Eichten, F. Feinberg, Phys. Rev. D23, 2724 (1981); T. A. Lahde, Nucl. Phys. A714, 183 (2003); J. R. Hiller, Phys. Rev. D30, 1520 (1984); W. Buchmuller, Phys. Lett. B112, 479 (1982); T. A. Lahde, C. J. Nyfalt, D. O. Riska, Nucl. Phys. A645, 587 (1999); J. S. Kang, Phys. Rev. D20, 2978 (1979); M. Hirano, Prog. of Theor. Phys. 83, 575 (1990); J. Baacke, Y. Igarashi, G. Kasperidus, Z. Phys. C13, 131 (1982).
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