An improved light-cone harmonic oscillator model for the pionic leading-twist distribution amplitude
Tao Zhong, Zhi-Hao Zhu, Hai-Bing Fu, Xing-Gang Wu, Tao Huang

TL;DR
This paper refines the light-cone harmonic oscillator model for the pion's leading-twist distribution amplitude, using QCD sum rules to determine moments and parameters, and compares the results with other theoretical approaches and experimental data.
Contribution
It introduces an improved model for the pion distribution amplitude by constraining parameters with higher-order moments from QCD sum rules and fitting the model to match various theoretical and experimental results.
Findings
The model's pion DA aligns closely with AdS/QCD and lattice results.
Calculated transition form factors agree with experimental data.
The improved model narrows the pion DA compared to Dyson-Schwinger predictions.
Abstract
In this paper, we study the pion leading-twist distribution amplitude by improving the traditional light-cone harmonic oscillator model within the reconstruction of the function . In order to constraining the model parameters, we calculate its moments in the framework of QCD background field theory sum rule (BFTSR) up to order. Considering the fact that the sum rule of the moment cannot be normalized, we suggest a more reasonable sum rule formula for . Then, we obtain the values of with at the initial scale . The first two moments are: , $\langle\xi^4\rangle_{2;\pi}|_{\mu_0} = 0.138…
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