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Medium modifications of $1P$-wave charmonia $χ_{cJ}(1P)$ in cold nuclear matter

Ze-Hua Zhang, Xiang Liu

TL;DR

This work investigates how the masses of the $χ_{cJ}(1P)$ ($J=0,1,2$) charmonia shift in cold symmetric nuclear matter using the quark-meson coupling framework combined with unquenched hadron-loop dynamics. The authors model in-medium effects by incorporating density-dependent $D^{(*)}$ masses from the QMC approach and compute the self-energies of $χ_{cJ}(1P)$ via loops involving $D\bar{D}$, $D^{*}\bar{D}$, $D\bar{D}^{*}$, and $D^{*}\bar{D}^{*}$ with dipole form factors and a cutoff $\\Lambda = m_E + \alpha \\Lambda_{QCD}$. They find sizable negative mass shifts at $ρ_0$, with the vector-vector channel playing a crucial role, especially for $χ_{c2}(1P)$, where the total shift can reach nearly $-100$ MeV; notably, no level crossing with the $D\bar{D}$ threshold occurs up to $ρ_B = 3ρ_0$. These results refine our understanding of cold nuclear matter effects on charmonia and provide input for CNM phenomenology and future experimental probes at facilities like FAIR-CBM and RHIC.

Abstract

In this work, we employ the quark-meson coupling model to investigate the mass shifts of $1P$-wave charmonia $χ_{cJ}(1P)$ ($J=0,1,2$) in cold symmetric nuclear matter by incorporating in-medium loop contributions to the $χ_{cJ}(1P)$ self-energy within the unquenched picture. At normal nuclear matter density, we obtain significant mass reductions of about 60 MeV for the $χ_{cJ}(1P)$ states, with the $χ_{c2}(1P)$ mass shift primarily arising from the vector-vector loop. Our results also indicate the absence of level crossing between the in-medium $χ_{cJ}(1P)$ mass and the $D\bar{D}$ mass threshold up to $ρ_B < 3ρ_0$-a feature that could be probed in the Compressed Baryonic Matter experiment at FAIR and the Beam Energy Scan program at RHIC.

Medium modifications of $1P$-wave charmonia $χ_{cJ}(1P)$ in cold nuclear matter

TL;DR

This work investigates how the masses of the () charmonia shift in cold symmetric nuclear matter using the quark-meson coupling framework combined with unquenched hadron-loop dynamics. The authors model in-medium effects by incorporating density-dependent masses from the QMC approach and compute the self-energies of via loops involving , , , and with dipole form factors and a cutoff . They find sizable negative mass shifts at , with the vector-vector channel playing a crucial role, especially for , where the total shift can reach nearly MeV; notably, no level crossing with the threshold occurs up to . These results refine our understanding of cold nuclear matter effects on charmonia and provide input for CNM phenomenology and future experimental probes at facilities like FAIR-CBM and RHIC.

Abstract

In this work, we employ the quark-meson coupling model to investigate the mass shifts of -wave charmonia () in cold symmetric nuclear matter by incorporating in-medium loop contributions to the self-energy within the unquenched picture. At normal nuclear matter density, we obtain significant mass reductions of about 60 MeV for the states, with the mass shift primarily arising from the vector-vector loop. Our results also indicate the absence of level crossing between the in-medium mass and the mass threshold up to -a feature that could be probed in the Compressed Baryonic Matter experiment at FAIR and the Beam Energy Scan program at RHIC.

Paper Structure

This paper contains 4 sections, 23 equations, 7 figures, 2 tables.

Figures (7)

  • Figure 1: Schematic diagram of the charmed-meson loop contributions to the $\chi_{c0}(1P)$ self-energy, where (1) and (2) represent the $D\bar{D}$ and $D^{*}\bar{D}^{*}$ loop contributions, respectively.
  • Figure 2: Schematic diagram of the charmed-meson loop contributions to the $\chi_{c1}(1P)$ self-energy, where (1) and (2) represent the $D^{*}\bar{D}$ and $D\bar{D}^{*}$ loop contributions, respectively.
  • Figure 3: Schematic diagram showing the charmed-meson loop contributions to the $\chi_{c2}(1P)$ self-energy: (1) $D\bar{D}$, (2) $D\bar{D}^{*}$, (3) $D^{*}\bar{D}$, and (4) $D^{*}\bar{D}^{*}$.
  • Figure 4: Mass shift of the $\chi_{c0}(1P)$ meson as a function of baryon density $\rho_{B}$ (in units of the normal nuclear matter density, $\rho_{0} = 0.15\,\mathrm{fm}^{-3}$) arising from the $D\bar{D}$ loop (a), the $D^{*}\bar{D}^{*}$ loop (b), and their combined effect (c); the solid, dotted, and dashed lines represent cutoff values $\alpha = 2$, $3$, and $4$, respectively.
  • Figure 5: Mass shift of the $\chi_{c1}(1P)$ meson as a function of baryon density $\rho_{B}$ (in units of $\rho_{0}$) arising from the $D\bar{D}^{*}$ or the $D^{*}\bar{D}$ loop (a), and their combined effect (b); the solid, dotted, and dashed lines represent cutoff values $\alpha = 2$, $3$, and $4$, respectively.
  • ...and 2 more figures