Light-front gauge propagator reexamined-II
Alfredo T. Suzuki, J.H.O.Sales

TL;DR
This paper reexamines the light-front gauge propagator, proposing a new method with two Lagrange multipliers to eliminate residual gauge freedom and produce a well-defined, Lorentz non-invariant propagator.
Contribution
It introduces a novel gauge fixing approach using two Lagrange multipliers, resulting in a complete and exact light-front propagator free of residual gauge ambiguities.
Findings
Achieves a well-defined light-front propagator without residual gauge freedom
Provides an exact propagator with explicit gauge fixing terms
Results in a Lorentz non-invariant but consistent propagator
Abstract
Gauge fields are special in the sense that they are invariant under gauge transformations and \emph{``ipso facto''} they lead to problems when we try quantizing them straightforwardly. To circumvent this problem we need to specify a gauge condition to fix the gauge so that the fields that are connected by gauge invariance are not overcounted in the process of quantization. The usual way we do this in the light-front is through the introduction of a Lagrange multiplier, , where is the external light-like vector, i.e., , and is the vector potential. This leads to the usual light-front propagator with all the ensuing characteristics such as the prominent pole which has been the subject of much research. However, it has been for long recognized that this procedure is incomplete in that there remains a residual gauge freedom…
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Taxonomy
TopicsAstronomical Observations and Instrumentation
