Fast Evaluation of Feynman Diagrams

TL;DR

This paper introduces a new numerical method for evaluating Feynman diagram integrals using generalized sinc functions, transforming integrals into rapidly computable sums without Monte Carlo methods.

Contribution

The authors develop a sinc-based approximation method that converts Feynman integrals into Gaussian sums, enabling faster and more precise numerical evaluation of complex diagrams.

Findings

Method efficiently evaluates third and fourth order diagrams.

Approximations can be made arbitrarily accurate.

Applicable to scalar field theories in Euclidean space.

Abstract

We develop a new representation for the integrals associated with Feynman diagrams. This leads directly to a novel method for the numerical evaluation of these integrals, which avoids the use of Monte Carlo techniques. Our approach is based on based on the theory of generalized sinc ($\sin(x)/x$) functions, from which we derive an approximation to the propagator that is expressed as an infinite sum. When the propagators in the Feynman integrals are replaced with the approximate form all integrals over internal momenta and vertices are converted into Gaussians, which can be evaluated analytically. Performing the Gaussians yields a multi-dimensional infinite sum which approximates the corresponding Feynman integral. The difference between the exact result and this approximation is set by an adjustable parameter, and can be made arbitrarily small. We discuss the extraction of regularization independent quantities and demonstrate, both in theory and practice, that these sums can be evaluated quickly, even for third or fourth order diagrams. Lastly, we survey strategies for numerically evaluating the multi-dimensional sums. We illustrate the method with specific examples, including the the second order sunset diagram from quartic scalar field theory, and several higher-order diagrams. In this initial paper we focus upon scalar field theories in Euclidean spacetime, but expect that this approach can be generalized to fields with spin.