Published November 14, 2008 | Version v1
Journal article

Convergence of the Chiral Expansion in Two-Flavor Lattice QCD

  • 1. High Energy Accelerator Research Organization (KEK), Tsukuba 305-0801 (Japan)
  • 2. Riken BNL Research Center, Upton, New York 11973 (United States)
  • 3. Graduate School of Pure and Applied Sciences, University of Tsukuba, Tsukuba 305-8571 (Japan)
  • 4. Physics Department, Center for Theoretical Sciences, and National Center for Theoretical Sciences, National Taiwan University, Taipei 10617, Taiwan (China)
  • 5. The Niels Bohr Institute, The Niels Bohr International Academy, Blegdamsvej 17 DK-2100 Copenhagen O Denmark (Denmark)
  • 6. School of High Energy Accelerator Science, The Graduate University for Advanced Studies (Sokendai), Tsukuba 305-0801 (Japan)
  • 7. Research Center for Applied Sciences, Academia Sinica, Taipei 115, Taiwan (China)
  • 8. Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502 (Japan)

Description

We test the convergence property of the chiral perturbation theory using a lattice QCD calculation of pion mass and decay constant with two dynamical quark flavors. The lattice calculation is performed using the overlap fermion formulation, which realizes exact chiral symmetry at finite lattice spacing. By comparing various expansion prescriptions, we find that the chiral expansion is well saturated at the next-to-leading order for pions lighter than ∼450 MeV. Better convergence behavior is found, in particular, for a resummed expansion parameter ξ, with which the lattice data in the pion mass region 290-750 MeV can be fitted well with the next-to-next-to-leading order formulas. We obtain the results in two-flavor QCD for the low energy constants l3 and l4 as well as the pion decay constant, the chiral condensate, and the average up and down quark mass

Additional details

Publishing Information

Journal Title
Physical Review Letters
Journal Volume
101
Journal Issue
20
Journal Page Range
p. 202004-202004.5
ISSN
0031-9007
CODEN
PRLTAO

Optional Information

Notes
(c) 2008 The American Physical Society
Collaborations
JLQCD Collaboration; TWQCD Collaboration