Abstract

The scattering equations give striking formulae for massless scattering amplitudes at tree level and, as shown recently, at one loop. The progress at loop level was based on ambitwistor string theory, which naturally yields the scattering equations. We proposed that, for ambitwistor strings, the standard loop expansion in terms of the genus of the worldsheet is equivalent to an expansion in terms of nodes of a Riemann sphere, with the nodes carrying the loop momenta. In this paper, we show how to obtain two-loop scattering equations with the correct factorization properties. We adapt genus-two integrands from the ambitwistor string to the nodal Riemann sphere and show that these yield correct answers, by matching standard results for the four-point two-loop amplitudes of maximal supergravity and super-Yang-Mills theory. In the Yang-Mills case, this requires the loop analogue of the Parke-Taylor factor carrying the colour dependence, which includes non-planar contributions.

Highlights

  • The Cachazo-He-Yuan (CHY) formulas provide remarkable tree-level expressions for scattering amplitudes in theories of massless particles, written as an integral over marked points on the Riemann sphere

  • In [9,10], we showed how the torus formulas reduce to formulas on a nodal Riemann sphere, by means of integration by parts in the moduli space of the torus

  • We proposed that an analogous reduction was possible at any genus, leading to a new formalism that could become a practical tool in the computation of scattering amplitudes

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Summary

INTRODUCTION

The Cachazo-He-Yuan (CHY) formulas provide remarkable tree-level expressions for scattering amplitudes in theories of massless particles, written as an integral over marked points on the Riemann sphere. The CHY formulas themselves originate in ambitwistor-string theory [4]: this provided a loop-level formulation [5,6] giving new formulas at genus one (torus) [5,7] and two [8] for type II supergravities in 10 dimensions. An alternative approach [16] applies higher-dimensional tree-level rules for the integration of the scattering equations to give diagrams for a scalar theory; our aim here is to give a framework that yields loop integrands on a nodal Riemann sphere for complete amplitudes. We characterize these degenerate solutions here, but leave the subtler nonsupersymmetric integrands for the future

FROM HIGHER GENUS TO THE SPHERE
THE 2-LOOP SCATTERING EQUATIONS
Poles and factorization
I as at
Degenerate and regular solutions
SUPERSYMMETRIC TWO-LOOP AMPLITUDES
Four-point supergravity integrand
Four-point super-Yang-Mills integrand
DISCUSSION
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