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2024年10月30日

Meson decays in an extended Nambu—Jona-Lasinio model with heavy quark flavors

  • In a previous work, we proposed an extended Nambu-Jona-Lasinio (NJL) model including heavy quark flavors. In this work, we will calculate strong and radiative decays of vector mesons in this extended NJL model, including light ρ, ω, K*, φ and heavy D*, D*s, B*, B*s.
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  • [1] Nambu Y, Jona-Lasinio G. Phys. Rev., 1961, 122: 345-358[2] Nambu Y, Jona-Lasinio G. Phys. Rev., 1961, 124: 246-254[3] Eguchi T. Phys. Rev. D, 1976, 14: 2755[4] Kikkawa K. Prog. Theor. Phys., 1976, 56: 947[5] Klimt S, Lutz M F, Vogl U, Weise W. Nucl. Phys. A, 1990, 516: 429-468[6] Vogl U, Lutz M F, Klimt S, Weise W. Nucl. Phys. A, 1990, 516: 469-495[7] Vogl U, Weise W. Prog. Part. Nucl. Phys., 1991, 27: 195-272[8] Klevansky S. Rev. Mod. Phys., 1992, 64: 649-708[9] Ebert D, Reinhardt H, Volkov M. Prog. Part. Nucl. Phys., 1994, 33: 1-120[10] Isgur N, Wise M B. Phys. Lett. B, 1989, 232: 113[11] Caswell W, Lepage G. Phys. Lett. B, 1986, 167: 437[12] Ebert D, Feldmann T, Friedrich R, Reinhardt H. Nucl. Phys. B, 1995, 434: 619-646; arXiv:hep-ph/9406220 [hep-ph][13] GUO X Y, CHEN X L, DENG W Z. Chin. Phys. C (HEP NP), 2013, 37: 033102; arXiv:1205.0355 [hep-ph][14] Akhmetshin R et al. (CMD-2 collaboration). Phys. Lett. B, 2004, 578: 285-289; arXiv:hep-ex/0308008 [hep-ex][15] Akhmetshin R et al. (CMD-2 collaboration). Phys. Lett. B, 2007, 648: 28-38; arXiv:hep-ex/0610021 [hep-ex][16] Akhmetshin R, Aulchenko V, Banzarov V S, Barkov L, Bashtovoy N et al. Phys. Lett. B, 2006, 642: 203-209[17] Fujikawa M et al. (Belle collaboration). Phys. Rev. D, 2008, 78: 072006; arXiv:0805.3773 [hep-ex][18] Baubillier M et al. (Birmingham-CERN-Glasgow-Michigan State-Paris collaboration). Z. Phys. C, 1984, 26: 37[19] Chandlee C, Berg D, Cihangir S, Collick B, Ferbel T et al. Phys. Rev. Lett., 1983, 51: 168[20] Abachi S, Akerlof C, Baringer P S, Blockus D, Brabson B et al. Phys. Lett. B, 1988, 212: 533[21] Gronberg J et al. (CLEO collaboration). Phys. Rev. Lett., 1995, 75: 3232-3236; arXiv:hep-ex/9508001 [hep-ex][22] Abreu P et al. (DELPHI collaboration). Z. Phys. C, 1995, 68: 353-362[23] Le Yaouanc A, Oliver L, Pene O, Raynal J C. Phys. Rev. D, 1973, 8: 2223-2234[24] Micu L. Nucl. Phys. B, 1969, 10: 521-526[25] Blundell H G, Godfrey S. Phys. Rev. D, 1996, 53: 3700-3711; arXiv:hep-ph/9508264[26] Barnes T, Close F E, Page P R, Swanson E S. Phys. Rev. D, 1997, 55: 4157-4188; arXiv:hep-ph/9609339[27] Capstick S, Isgur N. Phys. Rev. D, 1986, 34: 2809-2835[28] Capstick S, Roberts W. Phys. Rev. D, 1994, 49: 4570-4586[29] Jena S, Muni M, Pattnaik H, Sahu K. Int. J. Mod. Phys. A, 2010, 25: 2063-2086[30] Goity J, Roberts W. Phys. Rev. D, 2001, 64: 094007; arXiv:hep-ph/0012314 [hep-ph][31] Sucipto E, Thews R. Phys. Rev. D, 1987, 36: 2074[32] Deandrea A. arXiv:hep-ph/9809393 [hep-ph][33] Ebert D, Faustov R, Galkin V. Phys. Lett. B, 2002, 537: 241-248; arXiv:hep-ph/0204089 [hep-ph][34] Colangelo P, De Fazio F, Nardulli G. Phys. Lett. B, 1994, 334: 175-179; arXiv:hep-ph/9406320 [hep-ph][35] Orsland A H, Hogaasen H. Eur. Phys. J. C, 1999, 9: 503-510; arXiv:hep-ph/9812347 [hep-ph][36] Amundson J F, Boyd C G, Jenkins E E, Luke M E, Manohar A V et al. Phys. Lett. B, 1992, 296: 415-419; arXiv:hep-ph/9209241 [hep-ph][37] Aliev T, Demir D A, Iltan E, Pak N. Phys. Rev. D, 1996, 54: 857-862; arXiv:hep-ph/9511362 [hep-ph][38] Dosch H G, Narison S. Phys. Lett. B, 1996, 368: 163-170; arXiv:hep-ph/9510212 [hep-ph][39] Bernard V, Blin A, Hiller B, Meissner U, Ruivo M. Phys. Lett. B, 1993, 305: 163-167; arXiv:hep-ph/9302245 [hep-ph][40] Polleri A, Broglia R, Pizzochero P, Scoccola N. Z. Phys. A, 1997, 357: 325-331; arXiv: hep-ph/9611300 [hep-ph][41] Frison J et al. (Budapest-Marseille-Wuppertal collaboration). PoS, 2010, LATTICE2010: 139; arXiv:1011.3413 [hep-lat][42] Fu Z, Fu K. Phys. Rev. D, 2012, 86: 094507; arXiv:1209.0350 [hep-lat][43] Becirevic D, Haas B. Eur. Phys. J. C, 2011, 71: 1734; arXiv:0903.2407 [hep-lat][44] Nakamura K et al. (Particle Data Group). J. Phys. G, 2010, 37: 075021[45] Godfrey S, Isgur N. Phys. Rev. D, 1985, 32: 189-231[46] Kamal A, Xu Q. Phys. Lett. B, 1992, 284: 421-426[47] Anastassov A et al. (CLEO collaboration). Phys. Rev. D, 2002, 65: 032003; arXiv:hep-ex/0108043 [hep-ex]
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DENG Hong-Bo, CHEN Xiao-Lin and DENG Wei-Zhen. Meson decays in an extended Nambu—Jona-Lasinio model with heavy quark flavors[J]. Chinese Physics C, 2014, 38(1): 013103. doi: 10.1088/1674-1137/38/1/013103
DENG Hong-Bo, CHEN Xiao-Lin and DENG Wei-Zhen. Meson decays in an extended Nambu—Jona-Lasinio model with heavy quark flavors[J]. Chinese Physics C, 2014, 38(1): 013103.  doi: 10.1088/1674-1137/38/1/013103 shu
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Received: 2013-04-19
Revised: 2013-09-10
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Meson decays in an extended Nambu—Jona-Lasinio model with heavy quark flavors

    Corresponding author: DENG Wei-Zhen,
  • 1. School of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871, China

Abstract: In a previous work, we proposed an extended Nambu-Jona-Lasinio (NJL) model including heavy quark flavors. In this work, we will calculate strong and radiative decays of vector mesons in this extended NJL model, including light ρ, ω, K*, φ and heavy D*, D*s, B*, B*s.

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