Restoration of the chiral limit in Pauli-Villars-regulated light-front QED
- 1. Department of Physics, University of Minnesota-Duluth, Duluth, Minnesota 55812 (United States)
- 2. Department of Physics, Southern Methodist University, Dallas, Texas 75275 USA, and Department of Physics, University of Minnesota-Duluth, Duluth, Minnesota 55812 (United States)
Description
The dressed-electron eigenstate of Feynman-gauge QED is computed in light-front quantization with a Fock-space truncation to include at most the one-photon/one-electron sector. The theory is regulated by the inclusion of three massive Pauli-Villars (PV) particles, one PV electron, and two PV photons. In particular, the chiral-limit is investigated, and the correct limit is found to require two PV photons, not just one as previously thought. The renormalization and covariance of the electron current are also analyzed. We find that the plus component is well behaved and use its spin-flip matrix element to compute the electron's anomalous moment. The dependence of the moment on the regulator masses is shown to be slowly varying when the second PV photon is used to guarantee the correct chiral limit.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.79.114017;
- arXiv
- arXiv:0902.4443v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 79
- Journal Issue
- 11
- Journal Page Range
- p. 114017-114017.11
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41042758
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CHIRALITY; COMPUTERIZED SIMULATION; ELECTRONS; MASS; MATRIX ELEMENTS; PHOTONS; QUANTIZATION; QUANTUM ELECTRODYNAMICS; RENORMALIZATION; SPACE; SPIN FLIP
- Descriptors DEC
- BOSONS; ELECTRODYNAMICS; ELEMENTARY PARTICLES; FERMIONS; FIELD THEORIES; LEPTONS; MASSLESS PARTICLES; PARTICLE PROPERTIES; QUANTUM FIELD THEORY; SIMULATION
Optional Information
- Notes
- (c) 2009 The American Physical Society