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Two-Loop Scattering Amplitudes from the Riemann Sphere

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 sta...

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Detalles Bibliográficos
Autores principales: Geyer, Yvonne, Mason, Lionel, Monteiro, Ricardo, Tourkine, Piotr
Lenguaje:eng
Publicado: 2016
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.94.125029
http://cds.cern.ch/record/2202933
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author Geyer, Yvonne
Mason, Lionel
Monteiro, Ricardo
Tourkine, Piotr
author_facet Geyer, Yvonne
Mason, Lionel
Monteiro, Ricardo
Tourkine, Piotr
author_sort Geyer, Yvonne
collection CERN
description 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.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2016
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spelling cern-22029332023-10-04T08:19:09Zdoi:10.1103/PhysRevD.94.125029http://cds.cern.ch/record/2202933engGeyer, YvonneMason, LionelMonteiro, RicardoTourkine, PiotrTwo-Loop Scattering Amplitudes from the Riemann SphereParticle Physics - TheoryThe 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.The scattering equations give striking formulas 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 world sheet 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 color dependence, which includes nonplanar contributions.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.arXiv:1607.08887CERN-TH-2016-172DAMTP-2016-54CERN-TH-2016-172DAMTP-2016-54oai:cds.cern.ch:22029332016-07-29
spellingShingle Particle Physics - Theory
Geyer, Yvonne
Mason, Lionel
Monteiro, Ricardo
Tourkine, Piotr
Two-Loop Scattering Amplitudes from the Riemann Sphere
title Two-Loop Scattering Amplitudes from the Riemann Sphere
title_full Two-Loop Scattering Amplitudes from the Riemann Sphere
title_fullStr Two-Loop Scattering Amplitudes from the Riemann Sphere
title_full_unstemmed Two-Loop Scattering Amplitudes from the Riemann Sphere
title_short Two-Loop Scattering Amplitudes from the Riemann Sphere
title_sort two-loop scattering amplitudes from the riemann sphere
topic Particle Physics - Theory
url https://dx.doi.org/10.1103/PhysRevD.94.125029
http://cds.cern.ch/record/2202933
work_keys_str_mv AT geyeryvonne twoloopscatteringamplitudesfromtheriemannsphere
AT masonlionel twoloopscatteringamplitudesfromtheriemannsphere
AT monteiroricardo twoloopscatteringamplitudesfromtheriemannsphere
AT tourkinepiotr twoloopscatteringamplitudesfromtheriemannsphere