English

Deciphering the nature of $X(2300)$ with the PACIAE model

High Energy Physics - Phenomenology 2026-02-13 v2 High Energy Physics - Theory

Abstract

Inspired by the BESIII newest observation of an axial-vector particle X(2300)X(2300) in the ψ(3686)ϕηη\psi(3686)\rightarrow \phi\eta \eta' process, we simulate its production in e+ee^+e^- collisions at s=4.95\sqrt{s}=4.95 GeV using the parton and hadron cascade model PACIAE 4.0. In this model, the final partonic state (FPS) and hadronic state (FHS) are simulated and recorded sequentially. We propose, for the first time, that X(2300)X(2300) could be a qqˉssˉq\bar{q}s\bar{s} (q=u/dq=u/d) state or a hadro-strangeonium state, i.e., a bound system of a strangeonium and a light hadron. The excited strangeonium candidate is formed by coalescing an ssˉs\bar{s} quark pair in the FPS with the quantum statistical mechanics inspired dynamically constrained phase-space coalescence model. The tetraquark candidates of qqˉssˉq\bar{q}s\bar{s} and sssˉsˉss\bar{s}\bar{s} are similarly produced by coalescing four constituent quarks in the FPS. In contrast, a hadro-strangeonium candidate emerges from the recombination of the constituent ϕ\phi and η/η\eta/\eta in the FHS. We then calculate the X(2300)X(2300)'s orbital angular momentum quantum number in its rest frame and perform the spectral classification for each of the above candidates. Given its quantum numbers JPC=1+J^{PC}=1^{+-}, X(2300)X(2300) is identified as a PP-wave ssˉs\bar{s}, an SS-wave qqˉssˉ/sssˉsˉq\bar{q}s\bar{s}/ss\bar{s}\bar{s} or SS-wave ϕη/ϕη\phi\eta'/\phi \eta candidate. For the first time, we estimate the production rates for these configurations. The PP-wave ssˉs\bar{s} and SS-wave qqˉssˉq\bar{q}s\bar{s} states are produced at rates on the order of 10510^{-5}, whereas the SS-wave sssˉsˉss\bar{s}\bar{s} and ϕη/ϕη\phi\eta'/\phi \eta states appear at rates on the order of 10610^{-6}. Moreover, significant discrepancies are observed in the rapidity and transverse momentum distributions among different candidates. These discrepancies could be served as valuable criteria for deciphering the nature of X(2300)X(2300).

Keywords

Cite

@article{arxiv.2509.11746,
  title  = {Deciphering the nature of $X(2300)$ with the PACIAE model},
  author = {Jian Cao and Wen-Chao Zhang and Jin-Peng Zhang and Bo Feng and An-Ke Lei and Zhi-Lei She and Hua Zheng and Dai-Mei Zhou and Yu-Liang Yan and Ben-Hao Sa},
  journal= {arXiv preprint arXiv:2509.11746},
  year   = {2026}
}

Comments

6 pages, 3 tables, 2 figures, updated according to the referee's comments