Convergence in charmonium structure: light-front wave functions from basis light-front quantization and Dyson-Schwinger equations
Xianghui Cao, Yang Li, Chao Shi, James P. Vary, Qun Wang
TL;DR
This work benchmarks two non-perturbative QCD approaches—Basis Light-Front Quantization (BLFQ) and Dyson-Schwinger Equations (DSE)—by comparing their charmonium light-front wave functions across multiple observables: charge and gravitational form factors, light-cone distribution amplitudes, decay constants, and two-photon transition form factors. Despite their different foundations and parameters, BLFQ and DSE show remarkable agreement, validating both methods for heavy quarkonia and highlighting the universality of charmonium structure. The results reinforce the reliability of the BSA projection method and establish a solid baseline for extending these Hamiltonian- and Lagrangian-based techniques to more complex hadronic systems. The cross-method convergence strengthens confidence for interpreting experimental data at facilities like Jefferson Lab and future electron-ion colliders.
Abstract
We present a systematic comparison of charmonium light-front wave functions obtained through two complementary non-perturbative approaches: Basis Light-Front Quantization (BLFQ) and Dyson-Schwinger Equations (DSE). Key observables include the charge form factor, gravitational form factors, light-cone distribution amplitudes, decay constants, and two-photon transition form factors. Despite their distinct theoretical foundations and model parameters, the predictions from BLFQ and DSE exhibit remarkable agreement across all observables. This convergence validates both frameworks for studying charmonium structure and highlights the complementary strengths of Hamiltonian-based -- BLFQ -- and Lagrangian-based -- DSE -- methods in addressing non-perturbative QCD.
