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From infinity to four dimensions: higher residue pairings and Feynman integrals

Sebastian Mizera, Andrzej Pokraka

2020Journal of High Energy Physics60 citationsDOIOpen Access PDF

Abstract

A bstract We study a surprising phenomenon in which Feynman integrals in D = 4 − 2 ε space-time dimensions as ε → 0 can be fully characterized by their behavior in the opposite limit, ε → ∞ . More concretely, we consider vector bundles of Feynman integrals over kinematic spaces, whose connections have a polynomial dependence on ε and are known to be governed by intersection numbers of twisted forms. They give rise to differential equations that can be obtained exactly as a truncating expansion in either ε or 1 /ε . We use the latter for explicit computations, which are performed by expanding intersection numbers in terms of Saito’s higher residue pairings (previously used in the context of topological Landau-Ginzburg models and mirror symmetry). These pairings localize on critical points of a certain Morse function, which correspond to regions in the loop-momentum space that were previously thought to govern only the large- D physics. The results of this work leverage recent understanding of an analogous situation for moduli spaces of curves, where the α′ → 0 and α′ → ∞ limits of intersection numbers coincide for scattering amplitudes of massless quantum field theories.

Topics & Concepts

PhysicsModuli spaceFeynman diagramMassless particleQuantum field theoryScattering amplitudeMathematical physicsPure mathematicsHypersurfaceMorse theoryPath integral formulationDifferential formIntersection (aeronautics)QuantumMonodromyInfinityModuliVector spaceTopological quantum field theoryKinematicsContext (archaeology)Eigenvalues and eigenvectorsTheoretical physicsDifferential equationPosition and momentum spacePoisson algebraPolynomialSpace (punctuation)Quantum mechanicsInvariant (physics)Vector bundleHomotopy and Cohomology in Algebraic TopologyQuantum Mechanics and Non-Hermitian PhysicsBlack Holes and Theoretical Physics
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