transition form factors from QCD light-cone sum rules
arXiv:0907.4008 · doi:10.1103/PhysRevD.80.074012
Abstract
Light-cone sum rules for the transition form factors are derived from the correlation functions expanded by the twist of the distribution amplitudes of baryon. In terms of the three-quark distribution amplitudes models constrained by the QCD theory, we calculate the form factors at small momentum transfers and compare the results with that estimated in the conventional light-cone sum rules (LCSR) and perturbative QCD approaches. Our results indicate that the two different version of sum rules can lead to the consistent numbers of form factors responsible for transition. The transition form factors from LCSR with the asymptotic baryon distribution amplitudes are found to be almost one order larger than that obtained in the -baryon LCSR, implying that the pre-asymptotic corrections to the baryonic distribution amplitudes are of great importance. Moreover, SU(3) symmetry breaking effect between the form factors and are computed as in the framework of -baryon LCSR.
18 pages, 5 figures
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