Abstract

The scattering equations provide a powerful framework for the study of scattering amplitudes in a variety of theories. Their derivation from ambitwistor string theory led to proposals for formulae at one loop on a torus for 10 dimensional supergravity, and we recently showed how these can be reduced to the Riemann sphere and checked in simple cases. We also proposed analogous formulae for other theories including maximal super-Yang-Mills theory and supergravity in other dimensions at one loop. We give further details of these results and extend them in two directions. Firstly, we propose new formulae for the one-loop integrands of Yang-Mills theory and gravity in the absence of supersymmetry. These follow from the identification of the states running in the loop as expressed in the ambitwistor-string correlator. Secondly, we give a systematic proof of the non-supersymmetric formulae using the worldsheet factorisation properties of the nodal Riemann sphere underlying the scattering equations at one loop. Our formulae have the same decomposition under the recently introduced Q-cuts as one-loop integrands and hence give the correct amplitudes.

Highlights

  • Their derivation from ambitwistor string theory led to proposals for formulae at one loop on a torus for 10 dimensional supergravity, and we recently showed how these can be reduced to the Riemann sphere and checked in simple cases

  • We showed that formulae on the torus, such as the ACS and n-gon conjectures, reduce to ones on the Riemann sphere

  • We review how ambitwistor string amplitude formulae on the torus can be reduced to the Riemann sphere

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Summary

Introduction

They were found to underpin the remarkable formulae for tree-level scattering amplitudes in gauge theory and gravity that arise from twistor-string theories [22] and the more recent CHY formulae [14] The derivation of these formulae from ambitwistor string theories [10] led to proposals for formulae for loop amplitudes on higher-genus Riemann surfaces by Adamo, Casali and Skinner (ACS) [23], following the standard string paradigm. They extended the CHY formulae for type II supergravity in 10 dimensions to 1-loop in terms of scattering equations on an elliptic curve (and, in principle, to g-loops on curves of genus g).

The scattering equations on a torus
From a torus to a Riemann sphere
Supersymmetric theories
Supergravity
Super-Yang-Mills theory
Checks
Non-supersymmetric theories
General form of the one-loop scattering equations
Contributions of GSO sectors and the NS Pfaffian
Checks on all-plus amplitudes
Proof for non-supersymmetric amplitudes at one-loop
Factorisation I — scattering equations and measure
Factorisation II — integrands
The n-gon integrand Let us first consider the n-gon integrand
The Parke-Taylor factor
UV behaviour of the one-loop amplitudes
Discussion
A Solutions to the four-point 1-loop scattering equations
B Motivation from ambitwistor heterotic models
C The NS part of the integrand
D Dimensional reduction
Full Text
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