On the photon self-energy to three loops in QED

A bstract We compute the photon self-energy to three loops in Quantum Electrodynamics. The method of differential equations for Feynman integrals and a complete ϵ -factorization of the former allow us to obtain fully analytical results in terms of iterated integrals involving integration kernels related to a K3 geometry. We argue that our basis has the right properties to be a natural generalization of a canonical basis beyond the polylogarithmic case and we show that many of the kernels appearing in the differential equations, cancel out in the final result to finite order in ϵ . We further provide generalized series expansions that cover the whole kinematic space so that our results for the self-energy may be easily evaluated numerically for all values of the momentum squared. From the local solution at p 2 = 0, we extract the photon wave function renormalization constant in the on-shell scheme to three loops and confirm its agreement with previously obtained results.

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-03-19
DOI
https://doi.org/10.1007/jhep03(2025)148
Citations
16
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
29.92
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article

On the photon self-energy to three loops in QED

Christoph Nega, Lorenzo Tancredi, Felix Forner
16 citations
Journal of High Energy Physics
Black Holes and Theoretical Physics
29.92
article

On the photon self-energy to three loops in QED

Christoph Nega, Lorenzo Tancredi, Felix Forner
article en
16 citations

Abstract

A bstract We compute the photon self-energy to three loops in Quantum Electrodynamics. The method of differential equations for Feynman integrals and a complete ϵ -factorization of the former allow us to obtain fully analytical results in terms of iterated integrals involving integration kernels related to a K3 geometry. We argue that our basis has the right properties to be a natural generalization of a canonical basis beyond the polylogarithmic case and we show that many of the kernels appearing in the differential equations, cancel out in the final result to finite order in ϵ . We further provide generalized series expansions that cover the whole kinematic space so that our results for the self-energy may be easily evaluated numerically for all values of the momentum squared. From the local solution at p 2 = 0, we extract the photon wave function renormalization constant in the on-shell scheme to three loops and confirm its agreement with previously obtained results.

Journal of High Energy PhysicsVol. 2025(3)
Technical University of Munich (DE)
Openalex Percentile: Top 0%
Black Holes and Theoretical Physics
29.92
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