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《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2015, Vol. 39> Issue(6) : 063102 DOI: 10.1088/1674-1137/39/6/063102

Investigations on the charmless decays of Y(4260)

  • Apart from the charmful decay channels of Y(4260), the charmless decay channels of Y(4260) also provide us a good platform to study the nature and the decay mechanism of Y(4260). In this paper, we propose to probe the structure of Y(4260) through the charmless decays Y(4260)→VP via intermediate D1D+c.c. meson loops, where V and P stand for light vector and pseudoscalar mesons, respectively. Under the molecule ansatz of Y(4260), the predicted total branching ratio BRVP for all Y(4260)→VP processes are about (0.34-0.23+0.23)% to (0.75-0.52+0.72)% with the cutoff parameter α=2-3. Numerical results show that the intermediate m D1D+c.c. meson loops may be a possible transition mechanism in the Y(4260)→VP decays. These predicted branching ratios are the same order to that of Y(4260)→Zc+(3900)π-, which may be an evidence of D1D molecule and can be examined by the forthcoming BESⅢ data in the near future.
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    [1] Brambilla B, Eidelman S, Heltsley B K, Vogt R, Bodwin G T, Eichten E, Frawley A D, Meyer A B et al. Eur. Phys. J. C, 2011, 71: 1534[2] Swanson E S. Phys. Rept., 2006, 429: 243[3] Eichten E, Godfrey S, Mahlke H, Rosner J H. Rev. Mod. Phys., 2008, 80: 1161[4] Voloshin M B. Prog. Part. Nucl. Phys., 2008, 61: 455[5] Godfrey S, Olsen S L. Ann. Rev. Nucl. Part. Sci., 2008, 58: 51[6] Drenska N, Faccini R, Piccinini F, Polosa F A, Renga F, Sabelli C, Riv. Nuovo Cim., 2010, 033: 633[7] Aubert B et al. (BABAR collaboration). Phys. Rev. Lett., 2005, 95: 142001[8] HE Q et al. (CLEO collaboration). Phys. Rev. D, 2006, 74: 091104[9] YUAN C Z et al. (Belle collaboration). Phys. Rev. Lett., 2007, 99: 182004[10] Olive K A et al. (Particle Data Group collaboration). Chin. Phys. C, 2014, 38: 1[11] Ablikim M et al. (BESⅢ collaboration). Phys. Rev. Lett., 2013, 110: 252001[12] Llanes-Estrada F J. Phys. Rev. D, 2005, 72: 031503[13] Maiani L, Riquer V, Piccinini F, Polosa A D. Phys. Rev. D, 2005, 72: 031502[14] ZHU S L. Phys. Lett. B, 2005, 625: 212[15] Kou E, Pene O. Phys. Lett. B, 2005, 631: 164[16] Close F E, Page P R. Phys. Lett. B, 2005, 628: 215[17] DING G J, ZHU J J, YAN M L. Phys. Rev. D, 2008, 77: 014033[18] DING G J. Phys. Rev. D, 2009, 79: 014001[19] WANG Q, Hanhart C, ZHAO Q. Phys. Rev. Lett., 2013, 111: 132003[20] GUO F K, Hanhart C, Meiner U G, WANG Q, ZHAO Q. Phys. Lett. B, 2013, 725: 127[21] Filin A A, Romanov A, Baru V, Hanhart C, Kalashnikova Y X, Kudryavtsev A E, Meiner U G, Nefediev A V. Phys. Rev. Lett., 2010, 105: 019101[22] GUO F K, Meiner U G. Phys. Rev. D, 2011, 84: 014013[23] YUAN C Z, WANG P, MO X H. Phys. Lett. B, 2006, 634: 399[24] LIU X, ZENG X Q, LI X Q. Phys. Rev. D, 2005, 72: 054023[25] Dubynskiy S, Voloshin M B. Phys. Lett. B, 2008, 666: 344[26] LI X, Voloshin M B. Phys. Rev. D, 2013, 588: 034012[27] QIAO C F. Phys. Lett. B, 2006, 639: 263[28] QIAO C F. J. Phys. G, 2008, 35: 075008[29] CHEN Y D, QIAO C F. Phys. Rev. D, 2012, 85: 034034[30] CHEN Y D, QIAO C F, SHEN P N, ZENG Z Q. Phys. Rev. D, 2013, 88: 114007[31] van Beveren E, Rupp G. arXiv:0904.4351 [hep-ph][32] van Beveren E, Rupp G. Phys. Rev. D, 2009, 79: 111501[33] van Beveren E, Rupp G, Segovia J. Phys. Rev. Lett., 2010, 105 102001[34] CHEN D Y, HE J, LIU X. Phys. Rev. D, 2011, 83 054021[35] LIU X H, LI G. Phys. Rev. D, 2013, 88: 014013[36] WANG Q, Cleven M, GUO F K, Hanhart C, Meiner U G, WU X G, ZHAO Q. Phys. Rev. D, 2014, 89: 034001[37] LI X Q, Bugg D V, ZOU B S. Phys. Rev. D, 1997, 55: 1421[38] ZHAO Q, ZOU B S. Phys. Rev. D, 2006, 74: 114025[39] ZHAO Q. Phys. Lett. B, 2006, 636: 197[40] LI G, ZHAO Q. Phys. Rev. D, 2011, 84: 074005[41] LI G, LIU X H, ZHAO Q. Eur. Phys. J. C, 2013, 73: 2576[42] LI G, ZHAO Q, CHANG C H. J. Phys. G, 2008, 35: 055002[43] WANG Q, LI G, ZHAO Q. Phys. Rev. D, 2012, 85: 074015[44] LI G, SHAO F L, ZHAO C W, ZHAO Q. Phys. Rev. D, 2013, 87: 034020[45] LI G, ZHAO Q. Phys. Lett. B, 2008, 670: 55[46] Achasov N N, Kozhevnikov A A. Phys. Lett. B, 1991, 260: 425[47] Achasov N N, Kozhevnikov A A. JETP Lett., 1991, 54: 193; Pisma Zh. Eksp. Teor. Fiz., 1991, 54: 197[48] Achasov N N, Kozhevnikov A A. Phys. Rev. D, 1994, 49: 275[49] Achasov N N, Kozhevnikov A A. Phys. Atom. Nucl., 2006, 69: 988[50] ZHANG Y J, LI G, ZHAO Q. Phys. Rev. Lett., 2009, 102: 172001[51] LIU X, ZHANG BO, LI X Q. Phys. Lett. B, 2009, 675: 441[52] LI G, LIU X H, WANG Q, ZHAO Q. Phys. Rev. D, 2013, 88: 014010[53] WU J J, ZHAO Q, ZOU B S. Phys. Rev. D, 2007, 75: 114012[54] LIU X, ZENG X Q, LI X Q. Phys. Rev. D, 2006, 74: 074003[55] CHENG H Y, CHUA C K, Soni A. Phys. Rev. D, 2005, 71: 014030[56] Anisovich V V, Bugg D V, Sarantsev A V, ZOU B S. Phys. Rev. D, 1995, 51: 4619[57] ZHAO Q, ZOU B S, MA Z B. Phys. Lett. B, 2005, 631: 22[58] LI G, ZHAO Q, ZOU B S. Phys. Rev. D, 2008, 77: 014010[59] LIU X H, ZHAO Q. Phys. Rev. D, 2010, 81: 014017[60] WANG Q, LIU X H, ZHAO Q. Phys. Lett. B, 2012, 711: 364[61] LIU X H, ZHAO Q. J. Phys. G, 2011, 38: 035007[62] GUO F K, Hanhart C, Meiner U G. Phys. Rev. Lett., 2009, 103: 082003; 2010, 104: 109901[63] GUO F K, Hanhart C, LI G, U. G. Meiner, ZHAO Q. Phys. Rev. D, 2010, 82: 034025[64] GUO F K, Hanhart C, LI G, U. G. Meiner, ZHAO Q. Phys. Rev. D, 2011, 83: 034013[65] LI G. Eur. Phys. J. C, 2013, 73: 2621[66] Brambilla N et al. (Quarkonium Working Group collaboration). hep-ph/0412158[67] Brambilla N, Pineda A, Soto J, Vairo A. Rev. Mod. Phys., 2005, 77: 1423[68] WANG Q, Hanhart C, ZHAO Q. Phys. Lett. B, 2013, 725: 106[69] Cleven M, WANG Q, GUO F K, Hanhart C, Meiner U G, ZHAO Q. arXiv:1310.2190 [hep-ph][70] WU X G, Hanhart C, WANG Q, ZHAO Q. Phys. Rev. D, 2014, 89: 054038[71] LI G, LIU X H. Phys. Rev. D, 2013, 88: 094008[72] LI G, WANG W. Phys. Lett. B, 2014, 733: 100[73] LI G, LIU X H, ZHOU Z. Phys. Rev. D, 2014, 90: 054006[74] Lipkin H J. Nucl. Phys. B, 1987, 291: 720[75] Lipkin H J. Phys. Lett. B, 1986, 179: 278[76] Weinberg S. Phys. Rev., 1965, 137 B672[77] Baru V et al. Phys. Lett. B, 2004, 586: 53[78] Casalbuoni R, Deandrea A, Bartolomeo N Di, Gatto R, Feruglio F, Nardulli G. Phys. Lett. B, 1992, 292: 371[79] Casalbuoni R, Deandrea A, Bartolomeo N Di, Gatto R, Feruglio F, Nardulli G. Phys. Lett. B, 1993, 299: 139[80] Burdman G, Donoghue J F. Phys. Lett. B, 1992, 280: 287[81] YAN T M, CHENG H Y, CHEUNG C Y, LIN G L, LIN C Y, YU H L. Phys. Rev. D, 1992, 46: 1148; 1997, 55: 5851[82] Falk A F, Luke M E. Phys. Lett. B, 1992, 292: 119[83] Casalbuoni R, Deandrea A, Bartolomeo N Di, Gatto R, Feruglio F, Nardulli G. Phys. Rept., 1997, 281: 145[84] Isola C, Ladisa M, Nardulli G, Santorelli P. Phys. Rev. D, 2003, 68: 114001[85] Deandrea A, Gatto R, Nardulli G, Polosa A D. JHEP, 1999, 9902: 021[86] Locher M P, LU Y, ZOU B S. Z. Phys. A, 1994, 347: 281[87] LI X Q, ZOU B S. Phys. Lett. B, 1997, 399: 297[88] Cleven M, GUO F K, Hanhart C, Meiner U G. Eur. Phys. J. A, 2011, 47: 120

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LI Gang, AN Chun-Sheng, LI Peng-Yu, LIU Di, ZHANG Xiao and ZHOU Zhu. Investigations on the charmless decays of Y(4260)[J]. Chinese Physics C, 2015, 39(6): 063102. doi: 10.1088/1674-1137/39/6/063102
LI Gang, AN Chun-Sheng, LI Peng-Yu, LIU Di, ZHANG Xiao and ZHOU Zhu. Investigations on the charmless decays of Y(4260)[J]. Chinese Physics C, 2015, 39(6): 063102.  doi: 10.1088/1674-1137/39/6/063102 shu
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Received: 2014-10-11
Revised: 2014-11-17
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Investigations on the charmless decays of Y(4260)

    Corresponding author: LI Gang,
    Corresponding author: AN Chun-Sheng,
  • Received Date: 2014-10-11
  • Accepted Date: 2014-11-17
  • Available Online: 2015-06-05

Abstract: Apart from the charmful decay channels of Y(4260), the charmless decay channels of Y(4260) also provide us a good platform to study the nature and the decay mechanism of Y(4260). In this paper, we propose to probe the structure of Y(4260) through the charmless decays Y(4260)→VP via intermediate D1D+c.c. meson loops, where V and P stand for light vector and pseudoscalar mesons, respectively. Under the molecule ansatz of Y(4260), the predicted total branching ratio BRVP for all Y(4260)→VP processes are about (0.34-0.23+0.23)% to (0.75-0.52+0.72)% with the cutoff parameter α=2-3. Numerical results show that the intermediate m D1D+c.c. meson loops may be a possible transition mechanism in the Y(4260)→VP decays. These predicted branching ratios are the same order to that of Y(4260)→Zc+(3900)π-, which may be an evidence of D1D molecule and can be examined by the forthcoming BESⅢ data in the near future.

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