Table of Contents
Fetching ...

EW and QCD One-Loop Amplitudes with RECOLA

Stefano Actis, Ansgar Denner, Lars Hofer, Andreas Scharf, Sandro Uccirati

TL;DR

RECOLA provides an automated framework to compute SM amplitudes at NLO, addressing the need for general EW and QCD computations with many external legs. It extends Dyson–Schwinger recursion to one-loop amplitudes by representing them as linear combinations of tensor integrals with loop-specific currents and a novel color-flow recursion. The code integrates COLLIER for tensor integrals and supports full SM with counterterms, R2 terms, complex-mass scheme, and dipole subtraction preparation; its two-phase workflow makes it efficient in both generation and phase-space evaluation. The approach enables scalable, reusable computation of structure-dressed amplitudes, reducing memory usage and demonstrating practical performance on representative multi-leg processes.

Abstract

We present the computer code RECOLA for the computation of EW and QCD amplitudes in the Standard Model at next-to-leading order. One-loop amplitudes are represented as linear combinations of tensor integrals whose coefficients are calculated by means of recursive relations similar to Dyson-Schwinger equations. A novel treatment of colour enables us to recursively construct the colour structure of the amplitude efficiently. RECOLA is linked with the library COLLIER for the computation of the tensor integrals.

EW and QCD One-Loop Amplitudes with RECOLA

TL;DR

RECOLA provides an automated framework to compute SM amplitudes at NLO, addressing the need for general EW and QCD computations with many external legs. It extends Dyson–Schwinger recursion to one-loop amplitudes by representing them as linear combinations of tensor integrals with loop-specific currents and a novel color-flow recursion. The code integrates COLLIER for tensor integrals and supports full SM with counterterms, R2 terms, complex-mass scheme, and dipole subtraction preparation; its two-phase workflow makes it efficient in both generation and phase-space evaluation. The approach enables scalable, reusable computation of structure-dressed amplitudes, reducing memory usage and demonstrating practical performance on representative multi-leg processes.

Abstract

We present the computer code RECOLA for the computation of EW and QCD amplitudes in the Standard Model at next-to-leading order. One-loop amplitudes are represented as linear combinations of tensor integrals whose coefficients are calculated by means of recursive relations similar to Dyson-Schwinger equations. A novel treatment of colour enables us to recursively construct the colour structure of the amplitude efficiently. RECOLA is linked with the library COLLIER for the computation of the tensor integrals.

Paper Structure

This paper contains 6 sections, 20 equations, 1 table.