transition form factors within the QCD light-cone sum rules and the -meson leading-twist distribution amplitude
arXiv:1406.3892 · doi:10.1088/0954-3899/42/5/055002
Abstract
The QCD light-cone sum rules (LCSR) provides an effective way for dealing with the heavy-to-light transition form factors (TFFs), whose non-perturbative dynamics are parameterized into the light-meson's light-cone distribution amplitudes (LCDAs) with various twist structures. By taking the chiral correlator as the starting point, we calculate the LCSRs for the TFFs up to twist-4 accuracy. As for the TFFs at the large recoil region, we observe that the twist-2 transverse DA provides the dominant contribution, while the contributions from the remaining twist-3 and twist-4 terms are -suppressed. Thus, our present improved LCSRs provides a good platform for testing the behavior. For the purpose, we suggest a convenient WH-model for the -meson leading-twist wavefunction, in which the parameter dominantly controls its longitudinal distribution. Typically, its DA is CZ-like as , which changes to be asymptotic-like as . By varying , we present a detailed comparison of the LCSR estimation for the TFFs with those of pQCD and Lattice QCD predictions. Furthermore, by using the extrapolated TFFs, we estimate the CKM-matrix element with the help of two semi-leptonic decays. The predicted value for increases with the increment of , i.e. we have $\Vub=(2.91\pm0.19)\times 10^{-3}$ for and $\Vub=(3.11\pm0.19)\times 10^{-3}$ for . If using the BABAR prediction as a criteria, we observe that , which indicates that the -meson DA prefers a single-peak behavior rather than a double-humped behavior.
14 pages, 3 figures and 12 tables. References updated and discussions improved. To be published in J. Phys. G
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