Systematic analysis of DJ(2580), DJ*(2650), DJ(2740), DJ*(2760), DJ(3000) and DJ*(3000) in the D meson family

  • In this work, we tentatively assign the charmed mesons DJ(2580), DJ*(2650), DJ(2740), DJ*(2760), DJ(3000) and DJ*(3000) observed by the LHCb collaboration according to their spin, parity and masses, then systematically study their strong decays to ground state charmed mesons plus pseudoscalar mesons with the 3P0 decay model. Based on these studies, we assign the DJ*(2760) as the 1D(5/2)3- state, the DJ*(3000) as the 1F(5/2)2+ or 1F(7/2)4+ state, the DJ(3000) as the 1F(7/2)3+ or 2P(1/2)1+ state in the D meson family. As a byproduct, we also study the strong decays of the states 2P(1/2)0+, 2P(3/2)2+, 3S(1/2)1-, 3S(1/2)0- etc, which will be valuable in searching for the partners of these D mesons.
  • [1] Aaij R et al. (LHCb collaboration). JHEP, 2013, 1309: 145[2] del Amo Sanchez P et al. Phys. Rev. D, 2010, 82: 111101[3] WANG Z G. Phys. Rev. D, 2011, 83: 014009[4] ZHONG X H. Phys. Rev. D, 2010, 82: 114014[5] CHEN B, YUAN L, ZHANG A L. Phys. Rev. D, 2011, 83: 114025[6] Colangelo P, De Fazio F, Giannuzzi F, Nicotri S. Phys. Rev. D, 2012, 86: 054024[7] WANG Z G. Phys. Rev. D, 2013, 88: 114003[8] Micu L. Nucl. Phys. B, 1969, 10: 521[9] Le Yaouanc A, Oliver L, Pene O, Raynal J-C. Phys. Rev. D, 1973, 8: 2223; Phys. Rev. D, 1974, 9: 1415; Phys. Rev. D, 1975, 11: 1272; Phys. Lett. B, 1977, 71: 397[10] Le Yaouanc A, Oliver L, Pene O, Raynal J C. Phys. Lett. B, 1977, 72: 57[11] Le Yaouanc A, Oliver L, Pene O, Raynal J C. Hadron Transitons in the Quark Model, New York: Gordon and Breach Science Publishers, 1988[12] Roberts W, Brac B S. Few-Body Syst., 1992, 11: 171[13] Capstick S, Isgur N. Phys. Rev. D, 1986, 34: 2809; Capstick S, Roberts W. Phys. Rev. D, 1994, 49: 4570[14] Blundell H G. hep-ph/9608473; Blundell H G, Godfrey S. Phys. Rev. D, 1996, 53: 3700; Blundell H G, Godfrey S, Phelps B. Phys. Rev. D, 1996, 53: 3712[15] Ackleh E S, Barnes T, Swanson E S. Phys. Rev. D, 1996, 54: 6811; Barnes T, Black N, Page P R. Phys. Rev. D, 2003, 68: 054014; Close F E, Swanson E S. Phys. Rev. D, 2005, 72: 094004; Close F E, Thomas C E, Lakhina O, Swanson E S. Phys. Lett. B, 2007, 647: 159[16] ZHOU H Q, PING R G, ZOU B S. Phys. Lett. B, 2005, 611: 123; DING G J, YAN M L. Phys. Lett. B, 2007, 657: 49[17] CHEN B, WANG D X, ZHANG A L. Phys. Rev. D, 2009, 80: 071502[18] LI D M, ZHOU S. Phys.Rev. D, 2008, 78: 054013; LI D M, JI P F, MA B. Eur. Phys. J. C, 2011, 71: 1582[19] LI D M, MA B. Phys. Rev. D, 2010, 81: 014021[20] ZHANG B, LIU X, DENG W Z, ZHU S L. Eur. Phys. J. C, 2007, 50: 617; SUN Y, SONG Q T, CHEN D Y, LIU X, ZHU S L. arXiv:1401.1595 [hep-ph][21] YANG Y C, XIA Z R, PING J L. Phys. Rev. D, 2010, 81: 094003[22] SUN Y, LIU X, Matsuki T. Phys. Rev. D, 2013, 88: 094020[23] Manohar A V, Wise M B. Camb. Monogr. Part. Phys. Nucl. Phys. Cosmol, 2000, 10: 1; Neubert M. Phys. Rept., 1994, 245: 259[24] Beringer J et al. Phys. Rev. D, 2012, 86: 010001[25] Godfrey S, Isgur N. Phys. Rev. D, 1985, 32: 189[26] Pierro M D, Eichten E. Phys. Rev. D, 2001, 64: 114004[27] Ebert D, Faustov R N, Galkin V O. Eur. Phys. J. C, 2010, 66: 197[28] Hayne C, Isgur N. Phys. Rev. D, 1982, 25: 1944[29] Jacob M, Wick G C. Ann. Phys., 1959, 7: 404[30] Matsuki T, Morii T, Seo K. Prog. Theor. Phys., 2010, 124: 285[31] Avery P et al. Phys. Lett. B, 1994, 331: 236[32] Avery P et al. Phys. Rev. D, 1990, 41: 774[33] Albrecht H et al. Phys. Lett. B, 1989, 232: 398[34] Chekanov S et al. Eur. Phys. J. C, 2009, 60: 25
  • [1] Aaij R et al. (LHCb collaboration). JHEP, 2013, 1309: 145[2] del Amo Sanchez P et al. Phys. Rev. D, 2010, 82: 111101[3] WANG Z G. Phys. Rev. D, 2011, 83: 014009[4] ZHONG X H. Phys. Rev. D, 2010, 82: 114014[5] CHEN B, YUAN L, ZHANG A L. Phys. Rev. D, 2011, 83: 114025[6] Colangelo P, De Fazio F, Giannuzzi F, Nicotri S. Phys. Rev. D, 2012, 86: 054024[7] WANG Z G. Phys. Rev. D, 2013, 88: 114003[8] Micu L. Nucl. Phys. B, 1969, 10: 521[9] Le Yaouanc A, Oliver L, Pene O, Raynal J-C. Phys. Rev. D, 1973, 8: 2223; Phys. Rev. D, 1974, 9: 1415; Phys. Rev. D, 1975, 11: 1272; Phys. Lett. B, 1977, 71: 397[10] Le Yaouanc A, Oliver L, Pene O, Raynal J C. Phys. Lett. B, 1977, 72: 57[11] Le Yaouanc A, Oliver L, Pene O, Raynal J C. Hadron Transitons in the Quark Model, New York: Gordon and Breach Science Publishers, 1988[12] Roberts W, Brac B S. Few-Body Syst., 1992, 11: 171[13] Capstick S, Isgur N. Phys. Rev. D, 1986, 34: 2809; Capstick S, Roberts W. Phys. Rev. D, 1994, 49: 4570[14] Blundell H G. hep-ph/9608473; Blundell H G, Godfrey S. Phys. Rev. D, 1996, 53: 3700; Blundell H G, Godfrey S, Phelps B. Phys. Rev. D, 1996, 53: 3712[15] Ackleh E S, Barnes T, Swanson E S. Phys. Rev. D, 1996, 54: 6811; Barnes T, Black N, Page P R. Phys. Rev. D, 2003, 68: 054014; Close F E, Swanson E S. Phys. Rev. D, 2005, 72: 094004; Close F E, Thomas C E, Lakhina O, Swanson E S. Phys. Lett. B, 2007, 647: 159[16] ZHOU H Q, PING R G, ZOU B S. Phys. Lett. B, 2005, 611: 123; DING G J, YAN M L. Phys. Lett. B, 2007, 657: 49[17] CHEN B, WANG D X, ZHANG A L. Phys. Rev. D, 2009, 80: 071502[18] LI D M, ZHOU S. Phys.Rev. D, 2008, 78: 054013; LI D M, JI P F, MA B. Eur. Phys. J. C, 2011, 71: 1582[19] LI D M, MA B. Phys. Rev. D, 2010, 81: 014021[20] ZHANG B, LIU X, DENG W Z, ZHU S L. Eur. Phys. J. C, 2007, 50: 617; SUN Y, SONG Q T, CHEN D Y, LIU X, ZHU S L. arXiv:1401.1595 [hep-ph][21] YANG Y C, XIA Z R, PING J L. Phys. Rev. D, 2010, 81: 094003[22] SUN Y, LIU X, Matsuki T. Phys. Rev. D, 2013, 88: 094020[23] Manohar A V, Wise M B. Camb. Monogr. Part. Phys. Nucl. Phys. Cosmol, 2000, 10: 1; Neubert M. Phys. Rept., 1994, 245: 259[24] Beringer J et al. Phys. Rev. D, 2012, 86: 010001[25] Godfrey S, Isgur N. Phys. Rev. D, 1985, 32: 189[26] Pierro M D, Eichten E. Phys. Rev. D, 2001, 64: 114004[27] Ebert D, Faustov R N, Galkin V O. Eur. Phys. J. C, 2010, 66: 197[28] Hayne C, Isgur N. Phys. Rev. D, 1982, 25: 1944[29] Jacob M, Wick G C. Ann. Phys., 1959, 7: 404[30] Matsuki T, Morii T, Seo K. Prog. Theor. Phys., 2010, 124: 285[31] Avery P et al. Phys. Lett. B, 1994, 331: 236[32] Avery P et al. Phys. Rev. D, 1990, 41: 774[33] Albrecht H et al. Phys. Lett. B, 1989, 232: 398[34] Chekanov S et al. Eur. Phys. J. C, 2009, 60: 25
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12. Tan, X.-Z., Jiang, Y., Wang, T. et al. Rates of D0∗(2400) , DJ∗(3000) as the D0∗(2P) and D0∗(3P) in B decays[J]. European Physical Journal C, 2019, 79(9): 805. doi: 10.1140/epjc/s10052-019-7305-3
13. Kato, Y., Iijima, T. Open charm hadron spectroscopy at B-factories[J]. Progress in Particle and Nuclear Physics, 2019. doi: 10.1016/j.ppnp.2019.01.001
14. Gupta, P., Upadhyay, A. Masses and strong decay properties of radially excited bottom states B(2S) and B(2P) with their strange partners Bs(2S) and Bs(2P)[J]. European Physical Journal A, 2018, 54(9): 160. doi: 10.1140/epja/i2018-12590-6
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YU Guo-Liang, WANG Zhi-Gang, LI Zhen-Yu and MENG Gao-Qing. Systematic analysis of DJ(2580), DJ*(2650), DJ(2740), DJ*(2760), DJ(3000) and DJ*(3000) in the D meson family[J]. Chinese Physics C, 2015, 39(6): 063101. doi: 10.1088/1674-1137/39/6/063101
YU Guo-Liang, WANG Zhi-Gang, LI Zhen-Yu and MENG Gao-Qing. Systematic analysis of DJ(2580), DJ*(2650), DJ(2740), DJ*(2760), DJ(3000) and DJ*(3000) in the D meson family[J]. Chinese Physics C, 2015, 39(6): 063101.  doi: 10.1088/1674-1137/39/6/063101 shu
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Received: 2014-09-28
Revised: 2015-01-13
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Systematic analysis of DJ(2580), DJ*(2650), DJ(2740), DJ*(2760), DJ(3000) and DJ*(3000) in the D meson family

    Corresponding author: YU Guo-Liang,
    Corresponding author: WANG Zhi-Gang,

Abstract: In this work, we tentatively assign the charmed mesons DJ(2580), DJ*(2650), DJ(2740), DJ*(2760), DJ(3000) and DJ*(3000) observed by the LHCb collaboration according to their spin, parity and masses, then systematically study their strong decays to ground state charmed mesons plus pseudoscalar mesons with the 3P0 decay model. Based on these studies, we assign the DJ*(2760) as the 1D(5/2)3- state, the DJ*(3000) as the 1F(5/2)2+ or 1F(7/2)4+ state, the DJ(3000) as the 1F(7/2)3+ or 2P(1/2)1+ state in the D meson family. As a byproduct, we also study the strong decays of the states 2P(1/2)0+, 2P(3/2)2+, 3S(1/2)1-, 3S(1/2)0- etc, which will be valuable in searching for the partners of these D mesons.

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