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📄 Abstract
Abstract: A Minkowskian physics-informed neural network approach (M--PINN) is
formulated to solve the Dyson--Schwinger integral equations (DSE) of quantum
electrodynamics (QED) directly in Minkowski spacetime. Our novel strategy
merges two complementary approaches: (i) a dispersive solver based on Lehmann
representations and subtracted dispersion relations, and (ii) a M--PINN that
learns the fermion mass function $B(p^2)$, under the same truncation and
renormalization configuration (quenched, rainbow, Landau gauge) with the loss
integrating the DSE residual with multi--scale regularization, and
monotonicity/smoothing penalties in the spacelike branch in the same way as in
our previous work in Euclidean space. The benchmarks show quantitative
agreement from the infrared (IR) to the ultraviolet (UV) scales in both
on-shell and momentum-subtraction schemes. In this controlled setting, our
M--PINN reproduces the dispersive solution whilst remaining computationally
compact and differentiable, paving the way for extensions with realistic
vertices, unquenching effects, and uncertainty-aware variants.
Submitted
October 6, 2025
Key Contributions
This paper formulates a novel Minkowskian physics-informed neural network (M-PINN) approach to directly solve Dyson-Schwinger integral equations (DSE) of quantum electrodynamics (QED) in Minkowski spacetime. It merges a dispersive solver with an M-PINN that learns the fermion mass function, achieving quantitative agreement with dispersive solutions across scales while being computationally compact and differentiable.
Business Value
Advances fundamental understanding in theoretical physics, potentially leading to new insights and computational tools for complex physical systems.