Perturbative QCD factorization of ργρ

Ya-lan Zhang, Shan Cheng, Jun Hua, and Zhen-Jun Xiao
Phys. Rev. D 93, 036002 – Published 5 February 2016

Abstract

In this paper we first demonstrate step by step that the factorization hypothesis is valid at the next-to-leading order (NLO) for the exclusive process ργρ by employing the collinear factorization approach, and then extend this proof to the case of the kT factorization by taking into account the transversal momentum of the light external quark (antiquark) lines in the ρ meson. At the NLO level, we then show that the soft divergences from different subdiagrams will cancel each other in the quark level, while the remaining collinear divergences can be absorbed into the NLO meson wave functions. The full NLO amplitudes can therefore be factorized as the convolution of the NLO wave functions Φρ(1) and the infrared-finite leading order (LO) hard kernels GX,IJ,kl0 in the kT factorization. We also write down the polarized NLO ρ meson wave functions in the form of nonlocal hadron matrix elements with the gauge factor integral path deviating from the light cone. These NLO ρ meson wave functions can be used to calculate the NLO hard corrections to some relevant exclusive processes, such as Bρ transition.

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  • Received 4 December 2015

DOI:https://doi.org/10.1103/PhysRevD.93.036002

© 2016 American Physical Society

Physics Subject Headings (PhySH)

  1. Physical Systems
Particles & Fields

Authors & Affiliations

Ya-lan Zhang1, Shan Cheng2,*, Jun Hua1, and Zhen-Jun Xiao1,3,†

  • 1Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing, Jiangsu 210023, People’s Republic of China
  • 2Theoretische Elementarteilchenphysik, Naturwissenschaftlich Technische Fakultät, Universiät Siegen, 57068 Siegen, Germany
  • 3Jiangsu Key Laboratory for Numerical Simulation of Large Scale Complex Systems, Nanjing Normal University, Nanjing 210023, People’s Republic of China

  • *cheng@physik.uni-siegen.de
  • xiaozhenjun@njnu.edu.cn

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Issue

Vol. 93, Iss. 3 — 1 February 2016

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