Growth estimates for Dyson-Schwinger equations
Karen Yeats

TL;DR
This paper transforms Dyson-Schwinger equations into differential equations using Hopf algebra, analyzes their convergence properties, and establishes bounds linking primitive graph growth to the entire theory.
Contribution
It introduces a novel reduction of Dyson-Schwinger equations to differential equations and links primitive graph growth bounds to the overall theory's behavior.
Findings
Derived a system of differential equations from Dyson-Schwinger equations.
Established a relation between primitive graph growth and the entire theory's growth.
Proved that Lipatov bounds for primitives imply bounds for the full theory.
Abstract
Dyson-Schwinger equations are integral equations in quantum field theory that describe the Green functions of a theory and mirror the recursive decomposition of Feynman diagrams into subdiagrams. Taken as recursive equations, the Dyson-Schwinger equations describe perturbative quantum field theory. However, they also contain non-perturbative information. Using the Hopf algebra of Feynman graphs we will follow a sequence of reductions to convert the Dyson-Schwinger equations to the following system of differential equations, \[ \gamma_1^r(x) = P_r(x) - \sgn(s_r)\gamma_1^r(x)^2 + (\sum_{j \in \mathcal{R}}|s_j|\gamma_1^j(x)) x \partial_x \gamma_1^r(x) \] where , is the set of amplitudes of the theory which need renormalization, is the anomalous dimension associated to , is a modified version of the function for the primitive…
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Taxonomy
TopicsAdvanced Topics in Algebra · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
