Abstract

We present the complete formula for the cusp anomalous dimension at four loops in QCD and in maximally supersymmetric Yang-Mills. In the latter theory it is given by {left.{Gamma}_{mathrm{cusp},mathrm{A}}right|}_{alpha_s^4}=-{left(frac{alpha_sN}{pi}right)}^4left[frac{73{pi}^6}{20160}+frac{zeta_3^2}{8}+frac{1}{N^2}left(frac{31{pi}^6}{5040}+frac{9{zeta}_3^2}{4}right)right]. Our approach is based on computing the correlation function of a rectangular light-like Wilson loop with a Lagrangian insertion, normalized by the expectation value of the Wilson loop. In maximally supersymmetric Yang-Mills theory, this ratio is a finite function of a cross-ratio and the coupling constant. We compute it to three loops, including the full colour dependence. Integrating over the position of the Lagrangian insertion gives the four-loop Wilson loop. We extract its leading divergence, which determines the four-loop cusp anomalous dimension. Finally, we employ a supersymmetric decomposition to derive the last missing ingredient in the corresponding QCD result.

Highlights

  • We present the complete formula for the cusp anomalous dimension at four loops in QCD and in maximally supersymmetric Yang-Mills

  • Null polygon Wilson loops and the cusp anomalous dimension are of special interest in N = 4 super Yang-Mills theory

  • Extending the integrability approach to predicting nonplanar corrections to the cusp anomalous dimension is currently under active investigation. Another remarkable property of N = 4 super Yang-Mills theory (sYM) theory is that light-like Wilson loops describe the asymptotic behaviour of off-shell correlation functions in the light-like limit, when the operators approach the position of vertices of null polygon, and they are dual in the planar limit to the so-called MHV on-shell scattering amplitudes

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Summary

Cusp anomalous dimension from a correlation function

The connection between infrared asymptotics of on-shell scattering amplitudes and form factors and ultraviolet divergences of semi-infinite cusped Wilson loops has been previously used to obtain the cusp anomalous dimension. We follow another approach to computing the cusp anomalous dimension that relies on the relation between off-shell correlation functions of local operators and light-like Wilson loops

The quartic Casimir terms in different gauge theories
The cusp anomalous dimension from a finite ratio of Wilson loops
The Wilson loop integrand from a correlation function
Definition of the integral family
Integrand analysis via improved Baikov variables
Analytic computation of the master integrals
Wilson loop with Lagrangian insertion at three loops
Cusp anomalous dimension from integration over Lagrangian insertion
Conclusion and outlook
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