An improved light-cone harmonic oscillator model for the pionic leading-twist distribution amplitude
arXiv:2102.03989 · doi:10.1103/PhysRevD.104.016021
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: , ; and the corresponding Gegenbauer moments are , , respectively. After fitting the moments , we obtained the appropriate model parameters by using the least square method. The resultant behavior for twist-2 pion DA is more closely to the AdS/QCD and lattice result, but is narrower than that by Dyson-Schwinger equation. Furthermore, we calculate the pion-photon transition form factors (TFF) and TFF within light-cone sum rule approach, which are conform with experimental and theoretical results.
arXiv comment15 pages, 6 figures, matches the version to appear in PRD
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