Published June 1, 2009 | Version v1
Journal article

Coulomb-gauge ghost and gluon propagators in SU(3) lattice Yang-Mills theory

  • 1. Research Center for Nuclear Physics, Osaka University, Ibaraki-shi, Osaka 567-0047 (Japan)
  • 2. Max-Planck-Institut fuer Meteorologie, D-20146 Hamburg (Germany)
  • 3. Humboldt-Universitaet zu Berlin, Institut fuer Physik, D-12489 Berlin (Germany)
  • 4. Karl-Franzens-Universitaet Graz, Institut fuer Physik, A-8010 Graz (Austria)
  • 5. Research Institute for Information Science and Education, Hiroshima University, Higashi-Hiroshima 739-8521 (Japan)
  • 6. Integrated Information Center, Kochi University, Akebono-cho, Kochi 780-8520 (Japan)
  • 7. CSSM, School of Chemistry and Physics, University of Adelaide, SA 5005 (Australia)

Description

We study the momentum dependence of the ghost propagator and of the space and time components of the gluon propagator at equal time in pure SU(3) lattice Coulomb-gauge theory carrying out a joint analysis of data collected independently at the Research Center for Nuclear Physics, Osaka and Humboldt University, Berlin. We focus on the scaling behavior of these propagators at β=5.8,...,6.2 and apply a matching technique to relate the data for the different lattice cutoffs. Thereby, lattice artifacts are found to be rather strong for both instantaneous gluon propagators at a large momentum. As a byproduct we obtain the respective lattice scale dependences a(β) for the transversal gluon and the ghost propagator which indeed run faster with β than two-loop running, but slightly slower than what is known from the Necco-Sommer analysis of the heavy quark potential. The abnormal a(β) dependence as determined from the instantaneous time-time gluon propagator, D44, remains a problem, though. The role of residual gauge-fixing influencing D44 is discussed.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
79
Journal Issue
11
Journal Page Range
p. 114504-114504.16
ISSN
0556-2821
CODEN
PRVDAQ

Optional Information

Notes
(c) 2009 The American Physical Society