• Open Access

Global analysis of hadronic two-body B decays in the perturbative QCD approach

Jun Hua, Hsiang-nan Li, Cai-Dian Lü, Wei Wang, and Zhi-Peng Xing
Phys. Rev. D 104, 016025 – Published 28 July 2021

Abstract

Based on the flavor structure of four-quark effective operators, we develop an automatic computation program to calculate hadronic two-body B meson decay amplitudes, and apply it to their global analysis in the perturbative QCD (PQCD) approach. Fitting the PQCD factorization formulas for BPP,VP decays at leading order in the strong coupling αs to measured branching ratios and direct CP asymmetries, we determine the Gegenbauer moments in light meson light cone distribution amplitudes (LCDAs). It is found that most of the fitted Gegenbauer moments of the twist-2 and twist-3 LCDAs for the pseudoscalar meson P (P=π, K) and vector meson V (V=ρ, K*) agree with those derived in QCD sum rules. The shape parameter for the Bs meson distribution amplitude and the weak phase ϕ3(γ)=(75.2±2.9)° consistent with the value in Particle Data Group are also obtained. It is straightforward to extend our analysis to higher orders and higher powers, when the corresponding subleading contributions are available in the PQCD approach, and to the global determination of LCDAs for other hadrons.

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  • Received 7 January 2021
  • Accepted 8 July 2021

DOI:https://doi.org/10.1103/PhysRevD.104.016025

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Jun Hua1,†, Hsiang-nan Li2,‡, Cai-Dian Lü3,4,§, Wei Wang1,*, and Zhi-Peng Xing1,∥

  • 1INPAC, Key Laboratory for Particle Astrophysics and Cosmology (MOE), Shanghai Key Laboratory for Particle Physics and Cosmology, School of Physics and Astronomy, Shanghai Jiao-Tong University, Shanghai 200240, China
  • 2Institute of Physics, Academia Sinica, Taipei, Taiwan 11529, Republic of China
  • 3Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
  • 4School of Physics, University of Chinese Academy of Sciences, Beijing 100049, China

  • *Corresponding author. wei.wang@sjtu.edu.cn
  • huajun_phy@sjtu.edu.cn
  • hnli@phys.sinica.edu.tw
  • §lucd@ihep.ac.cn
  • zpxing@sjtu.edu.cn

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Issue

Vol. 104, Iss. 1 — 1 July 2021

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