Possible dibaryon production at ${{\overline {\bf P} }}$ anda with a Lagrangian approach

  • In order to confirm the existence of the dibaryon state $ d^*(2380) $ observed at WASA@COSY, we estimate the cross section for production of the possible dibaryon and anti-dibaryon pair $ {d^*}{\bar{d}^*} $ in the energy region of the upcoming experiments at $ {\bar{{\rm{P}}}} $ anda. Based on some qualitative properties of $ {d^*} $ extracted from the analyses in the non-relativistic quark model, the production cross section for this spin-3 particle pair are calculated with the help of a phenomenological effective relativistic and covariant Lagrangian approach.
      PCAS:
  • 加载中
  • [1] H. Clement, Prog. Part. Nucl. Phys.93, 195 (2017), arXiv:1610.05591[nucl-ex doi:10.1016/j.ppnp.2016.12.004
    [2] H. Clement and T. Skorodko, Chin. Phys. C45, 022001 (2021), arXiv:2008.07200[nucl-th doi:10.1088/1674-1137/abcd8e
    [3] M. Bashkanovet al., Phys. Rev. Lett.102, 052301 (2009) doi:10.1103/PhysRevLett.102.052301
    [4] P. Adlarsonet al. (WASA-at-COSY Collaboration), Phys. Rev. Lett.106, 242302 (2011)
    [5] P. Adlarsonet al. (WASA-at-COSY Collaboration), Phys. Lett. B721, 229 (2013)
    [6] P. Adlarsonet al. (WASA-at-COSY Collaboration), Phys. Rev. Lett.112(20), 202301 (2014)
    [7] H. X. Chen, W. Chen, X. Liuet al., Phys. Rept.639, 1 (2016), arXiv:1601.02092[hep-ph doi:10.1016/j.physrep.2016.05.004
    [8] F. K. Guo, C. Hanhart, U. G. Meissneret al., Rev. Mod. Phys.90, 015004 (2018), arXiv:1705.00141[hep-ph doi:10.1103/RevModPhys.90.015004
    [9] Y. Dong, A. Faessler, and V. E. Lyubovitskij, Prog. Part. Nucl. Phys.94, 282 (2017)
    [10] R. F. Lebed, R. E. Mitchell, and E. S. Swanson,, Prog. Part. Nucl. Phys.93, 143 (2017), arXiv:1610.04528[hep-ph doi:10.1016/j.ppnp.2016.11.003
    [11] X. Q. Yuanet al., Phys. Rev. C60, 045203 (1999) doi:10.1103/PhysRevC.60.045203
    [12] M. Bashkanov, Stanley J. Brodskyet al., Phys. Lett. B727, 438 (2013) doi:10.1016/j.physletb.2013.10.059
    [13] F. Huang, Z. Y. Zhang, P. N. Shenet al., Heavy-Quark QCD Exotica39(7), 071001 (2015)
    [14] F. Huang, P. N. Shen, Y. B. Donget al., Sci. China Phys. Mech. Astron.59(2), 622002 (2016) doi:10.1007/s11433-015-5767-3
    [15] Yubing Dong, Pengnian Shen, Fei Huanget al., Phys. Rev. C91, 064002 (2015) doi:10.1103/PhysRevC.91.064002
    [16] Yubing Dong, Fei Huang, Pengnian Shenet al., Phys. Rev. C94, 014003 (2016) doi:10.1103/PhysRevC.94.014003
    [17] Yubing Dong, Fei Huang, Pengian Shenet al., Chinese PhysicsC41, 101001 (2017)
    [18] H. Huang, J. Ping, and F. Wang, Phys. Rev. C89(3), 034001 (2014), arXiv:1312.7756[hep-ph doi:10.1103/PhysRevC.89.034001
    [19] F. Huang and W. L. Wang, Phys. Rev. D98(7), 074018 (2018) doi:10.1103/PhysRevD.98.074018
    [20] A. Gal and H. Garcilazo, Phys. Rev. Lett.111, 172301 (2013) doi:10.1103/PhysRevLett.111.172301
    [21] A. Gal and H. Garcilazo, Nucl. Phys. A928, 73 (2014) doi:10.1016/j.nuclphysa.2014.02.019
    [22] M. N. Platonova and V. I. Kukulin, Nucl. Phys. A946, 117 (2016), arXiv:1412.4574[nucl-th doi:10.1016/j.nuclphysa.2015.11.009
    [23] M. N. Platonova and V. I. Kukulin, Phys. Rev. C87(2), 025202 (2013), arXiv:1211.0444[nucl-th doi:10.1103/PhysRevC.87.025202
    [24] Pan-Pan Shi, Fei Huang, and Wen-Ling Wang, Eur. Phys. J. C79(4), 314 (2019) doi:10.1140/epjc/s10052-019-6809-1
    [25] Natsumi Ikeno, Raquel Molina, and Eulogio Oset, Phys. Rev. C104(1), 014614 (2021) doi:10.1103/PhysRevC.104.014614
    [26] Yubing Dong, Fei Huang, Pennian Shenet al., Phys. Rev. D96, 094001 (2017) doi:10.1103/PhysRevD.96.094001
    [27] Yubing Dong, Pennian Shen, and Zongye Zhang, Phys. Rev. D97, 11-114002 (2018)
    [28] Yubing Dong, Fei Huang, Pennian Shenet al., Int. J. Mod. Phys. A34(18), 1950100 (2019) doi:10.1142/S0217751X19501008
    [29] T. Ishikawaet al., Phys. Lett. B772, 398-402 (2017), arXiv:1610.05532[nucl-ex doi:10.1016/j.physletb.2017.04.010
    [30] T. Ishikawaet al., Phys. Lett. B789, 413-318 (2019) doi:10.1016/j.physletb.2018.12.050
    [31] T. Ishikawaet al., Springer Proc. Phys.238, 609-613 (2020)
    [32] Elisa Fioravanti, J. Phys. Conf. Ser.503, 012030 (2014) doi:10.1088/1742-6596/503/1/012030
    [33] P. Hawranek, Int. J. Mod. Phys. A22, 574-577 (2007) doi:10.1142/S0217751X07035860
    [34] Diego Bettoni, Prof. Part. Nucl. Phys.67, 502-510 (2012) doi:10.1016/j.ppnp.2012.01.018
    [35] Y. B. Dong, A. Faessler, T. Gutscheet al., Phys. Rev. D77, 094013 (2008) doi:10.1103/PhysRevD.77.094013
    [36] Y. B. Dong, A. Faessler, T. Gutscheet al., Phys. Rev. D79, 094013 (2009) doi:10.1103/PhysRevD.79.094013
    [37] Yubing Dong, Amand Faessler, Thomas Gutscheet al., J. Phys. G.38, 015001 (2011), arXiv:0909.0380[hep-ph doi:10.1088/0954-3899/38/1/015001
    [38] Yubing Dong, Amand Faessler, Thomas Gutscheet al., Phys. Rev. D88, 014030 (2013), arXiv:1306.0824[hep-ph doi:10.1103/PhysRevD.88.014030
    [39] Y. Dong, A. Faessler, T. Gutscheet al., Phys. Rev. D81, 014006 (2010), arXiv:0910.1204[hep-ph doi:10.1103/PhysRevD.81.014006
    [40] Y. Dong, A. Faessler, T. Gutscheet al., Phys. Rev. D82, 034035 (2010) doi:10.1103/PhysRevD.82.034035
    [41] Y. Dong, A. Faessler, T. Gutscheet al., Phys. Rev. C78, 035205 (2008), arXiv:0806.3679[hep-ph
    [42] Amand Faessler, Thomas Gutsche, M. A. Ivanovet al., Phys. Rev. D68, 014011 (2003), arXiv:0304031[hep-ph doi:10.1103/PhysRevD.68.014011
    [43] Cheng-Jian Xiao, Yubing Dong, Thomas Gutscheet al., Phys. Rev. D, 101101, 114032 (2020), arXiv:2004.12415[hep-ph doi:10.1103/PhysRevD.101.114032
    [44] Q. B. Li and P.N.Shen, Euro. Phys. J. A8, 417 (2000)
    [45] T. Iritaniet al. (HAL QCD Collaboration), Phys. Lett. B 792, 284 (2019)
    [46] D. Michael Scadron, Phys. Rev.165, 1640-1647 (1968) doi:10.1103/PhysRev.165.1640
    [47] A. Salam, Nuovo Cim.25, 224 (1962) doi:10.1007/BF02733330
    [48] S. Weinberg, Phys. Rev.130, 776 (1963) doi:10.1103/PhysRev.130.776
    [49] K. Hayashi, M. Hirayama, T. Mutaet al., Fortsch. Phys.15, 625 (1967)
    [50] G. V. Efimov and M. A. Ivanov,The Quark Confinement Model of Hadrons, (IOP Publishing, Bristol & Philadelphia, 1993)
    [51] Kenji Hayashi, Minoru Hirayama, Taizo Mutaet al., Fortsch. Phys.15(10), 625-660 (1967) doi:10.1002/prop.19670151002
    [52] G. V. Efimov, M. A. Ivanov, and V. E. Lyubovitskij, Few Body Syst.6, 17-43 (1989) doi:10.1007/BF01076281
    [53] G. W. Van Apeldoorn, R. L. F. Gruendeman, D. Hartinget al., Nucl. Phys. B.133, 245-265 (1978) doi:10.1016/0550-3213(78)90301-2
    [54] D. R. Ward, R. E. Ansorge, C. P. Bustet al., Nucl. Phys. B. 141, 203-219 (2978)
    [55] P. Johnsonet al., Nucl. Phys. B173, 77-92 (1980) doi:10.1016/0550-3213(80)90444-7
    [56] G. W. Van Apeldoornet al., Z. Phys. C12, 95-98 (1985)
    [57] Mohammad Saleem and Fazal-e-Aleem, Prog. Theor. Phys., 70(1983), (1156)
    [58] E. Guenter Wolf, Phys. Rev.182, 1538-1560 (1969) doi:10.1103/PhysRev.182.1538
    [59] Xu Cao, Bing-Song Zou, Bing-Songet al., Nucl. Phys. A861, 23-36 (2011), arXiv:1009.1060[nucl-th doi:10.1016/j.nuclphysa.2011.05.094
    [60] D. O. Riska and G. E. Brown, Nucl. Phys. A679, 577-596 (2011), arXiv:0005049[nucl-th
    [61] Chao-Yi Lgu, Ping Wang, Yubing Donget al., Phys. Rev. D99, 036015 (2019), arXiv:1810.02138[hep-ph doi:10.1103/PhysRevD.99.036015
    [62] Chao-Yi Lü, Ping Wang, Yubing Donget al., Chinese Phys. C42, 064102 (2018), arXiv:1803.07795[hep-ph doi:10.1088/1674-1137/42/6/064102
  • 加载中

Figures(5)

Get Citation
Yubing Dong and Pengnian Shen. Possible dibaryon production at Panda with a Lagrangian approach[J]. Chinese Physics C. doi: 10.1088/1674-1137/ac3567
Yubing Dong and Pengnian Shen. Possible dibaryon production at Panda with a Lagrangian approach[J]. Chinese Physics C. doi:10.1088/1674-1137/ac3567 shu
Milestone
Received: 2021-09-06
Baidu
map