Published September 1, 2011
| Version v1
Journal article
Lattice simulations and infrared conformality
- 1. Department of Physics, Sloane Laboratory, Yale University, New Haven, Connecticut 06520 (United States)
- 2. Theoretical Physics Department, Fermi National Accelerator Laboratory, Batavia, Illinois 60510 (United States)
- 3. Department of Physics, Boston University, Boston, Massachusetts 02215 (United States)
Description
We examine several recent lattice-simulation data sets, asking whether they are consistent with infrared conformality. We observe, in particular, that for an SU(3) gauge theory with 12 Dirac fermions in the fundamental representation, recent simulation data can be described assuming infrared conformality. Lattice simulations include a fermion mass m that is then extrapolated to zero, and we note that this data can be fit by a small-m expansion, allowing a controlled extrapolation. We also note that the conformal hypothesis does not work well for two theories that are known or expected to be confining and chirally broken, and that it does work well for another theory expected to be infrared conformal.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.84.054501;
- arXiv
- arXiv:1106.2148v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 84
- Journal Issue
- 5
- Journal Page Range
- p. 054501-054501.6
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43083335
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CHIRAL SYMMETRY; COMPUTERIZED SIMULATION; EXPANSION; EXTRAPOLATION; FERMIONS; GAUGE INVARIANCE; LATTICE FIELD THEORY; MASS; SU-3 GROUPS; SYMMETRY BREAKING
- Descriptors DEC
- CONSTRUCTIVE FIELD THEORY; FIELD THEORIES; INVARIANCE PRINCIPLES; LIE GROUPS; MATHEMATICAL SOLUTIONS; NUMERICAL SOLUTION; QUANTUM FIELD THEORY; SIMULATION; SU GROUPS; SYMMETRY; SYMMETRY GROUPS
Optional Information
- Notes
- (c) 2011 American Institute of Physics