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Charmonium-like exotic hadron productions in e+e− collisions at the BESIII energy with the PACIAE model

Jian Cao1, Wen-Chao Zhang1,*, Zhi-Lei She2, An-Ke Lei3, Jin-Peng Zhang1, Hua Zheng1, Dai-Mei Zhou3,†, Yu-Liang Yan4, Zhong-Qi Wang5 et al.

Ben-Hao Sa4,3,‡

  • *Contact author: wenchao.zhang@snnu.edu.cn
  • †Contact author: zhoudm@mail.ccnu.edu.cn
  • ‡Contact author: sabhliuym35@qq.com

Phys. Rev. D 112, 014033 – Published 21 July, 2025

DOI: https://doi.org/10.1103/1gtz-xkgh

Abstract

Inspired by the BESIII observation of exotic hadron G(3900) in the e+e−→DD¯ process [M. Ablikim et al. (BESIII Collaboration), Phys. Rev. Lett. 133, 081901 (2024)], we use the parton and hadron cascade model PACIAE to simulate the productions of charmonium-like exotic hadrons, including X(3872), Zc(3900)0, and G(3900) in the e+e− annihilations at s=4.95  GeV. The charmonium-like candidates are recombined by the dynamically constrained phase-space coalescence model using component mesons DD¯ [for G(3900)] or DD¯*/D¯D* [for X(3872), Zc(3900)0, and G(3900)] in the PACIAE simulated final hadronic state. We then calculate, for the first time, the charmonium-like candidate’s orbital angular momentum quantum number in its rest frame and perform the spectral classification for each of the above candidates. For G(3900), as its JPC is 1−−, it is identified as the P-wave DD¯ or DD¯*/D¯D* state. Meanwhile, for X(3872) and Zc(3900)0, as their JPCs are, respectively, 1++ and 1+−, they are identified as the S-wave DD¯*/D¯D* candidates. It is observed that the yield of the P-wave G(3900) composed of DD¯*/D¯D* is significantly larger than that composed of DD¯. Moreover, in the DD¯*/D¯D* channel, the yield of the P-wave G(3900) is around three times as large as the yield of the S-wave Zc(3900)0, and it is around two orders of magnitude as large as the yield of the S-wave X(3872). Finally, significant discrepancies are observed in the transverse momentum spectra and the rapidity distributions among the X(3872), Zc(3900)0, and G(3900) states. These discrepancies are proposed as valuable criteria for identifying the different charmonium-like exotic hadrons from each other.

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