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      Solvable Models Of Infrared Gupta-Bleuler Quantum Electrodynamics

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          Abstract

          Hamiltonian models based on two different infrared approximations are studied in order to obtain an explicit comparison with the standard analysis of the infrared contributions, occurring in the relativistically covariant perturbative formulation of Quantum Electrodynamics. Moller operators, preserving respectively the Hilbert scalar product, for the Coulomb-gauge models, and an indefinite metric, for the models formulated in Feynman's gauge, are obtained in the presence of an infrared cutoff, after the removal of an adiabatic switching and with the aid of a suitable mass renormalization. In the presence of a dipole approximation, spurious contributions to the infrared factors are shown to necessarily arise in Feynman's gauge, with respect both to the Coulomb-gauge model and to the amplitudes of Quantum Electrodynamics, and the connection of this result with a recent work on the Gupta-Bleuler formulation of non-relativistic models is discussed. It is finally proven that by dropping the dipole approximation and adopting an expansion around a fixed charged particle four-momentum, first introduced and employed in the study of the infrared problem by Bloch and Nordsieck, the infrared diagrammatic is fully reproduced and spurious low-energy effects are avoided.

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          Most cited references24

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          Note on the Radiation Field of the Electron

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                Author and article information

                Journal
                03 September 2010
                2011-10-24
                Article
                1009.0637
                cfa0ddc7-d051-4a2b-b0a6-1e88d37ea14e

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                47B50, 46C20, 46L60, 81Q10
                18 pages, no figures, revised version with an extended treatment of issues connected with an indefinite metric
                math-ph hep-th math.MP quant-ph

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