Extended Hamiltonian Formalism of the Pure Space-Like Axial Gauge Schwinger Model
Y. Nakawaki, G. McCartor

TL;DR
This paper develops an infrared divergence-free Hamiltonian formalism for the pure space-like axial gauge Schwinger model, using auxiliary coordinates and different gauge prescriptions, culminating in an operator solution in the Coulomb gauge.
Contribution
It introduces a novel Hamiltonian formalism for the axial gauge Schwinger model that avoids infrared divergences by switching gauge prescriptions and coordinate representations.
Findings
Infrared divergences are canceled using ML and PV prescriptions.
Operator solutions are obtained in the axial and Coulomb gauges.
Representation space is of indefinite metric, indicating gauge choice independence.
Abstract
We demonstrate that pure space-like axial gauge quantizations of gauge fields can be constructed in ways which are free from infrared divergences. We begin by constructing an axial gauge formulation in auxiliary coordinates: . For \theta less than \pi\over 4 we can take as the evolution parameter and construct a traditional canonical formulation of the temporal gauge Schwinger model in which residual gauge fields dependent only on are static canonical variables. Then we extrapolate the temporal gauge operator solution into the axial region, \theta > \pi \over 4, where is taken as the evolution parameter. In the axial region we find that we have to change representations of the residual gauge fields from one realizing the PV prescription to one realizing the ML prescription in order for the…
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