Next-to-leading non-global logarithms in QCD

Abstract Non-global logarithms arise from the sensitivity of collider observables to soft radiation in limited angular regions of phase space. Their resummation to next-to-leading logarithmic (NLL) order has been a long standing problem and its solution is relevant in the context of precision all-or...

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Main Authors: Andrea Banfi, Frédéric A. Dreyer, Pier Francesco Monni
Format: Article
Language:English
Published: SpringerOpen 2021-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP10(2021)006
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spelling doaj-5a60737b7dc74ca7a2a68cac7f8118f82021-10-03T11:56:32ZengSpringerOpenJournal of High Energy Physics1029-84792021-10-0120211013610.1007/JHEP10(2021)006Next-to-leading non-global logarithms in QCDAndrea Banfi0Frédéric A. Dreyer1Pier Francesco Monni2Department of Physics and Astronomy, University of SussexRudolf Peierls Centre for Theoretical Physics, Clarendon LaboratoryCERN, Theoretical Physics DepartmentAbstract Non-global logarithms arise from the sensitivity of collider observables to soft radiation in limited angular regions of phase space. Their resummation to next-to-leading logarithmic (NLL) order has been a long standing problem and its solution is relevant in the context of precision all-order calculations in a wide variety of collider processes and observables. In this article, we consider observables sensitive only to soft radiation, characterised by the absence of Sudakov double logarithms, and we derive a set of integro-differential equations that describes the resummation of NLL soft corrections in the planar, large-N c limit. The resulting set of evolution equations is derived in dimensional regularisation and we additionally provide a formulation that is manifestly finite in four space-time dimensions. The latter is suitable for a numerical integration and can be generalised to treat other infrared-safe observables sensitive solely to soft wide-angle radiation. We use the developed formalism to carry out a fixed-order calculation to O α s 2 $$ \mathcal{O}\left({\alpha}_s^2\right) $$ in full colour for both the transverse energy and energy distribution in the interjet region between two cone jets in e + e − collisions. We find that the expansion of the resummed cross section correctly reproduces the logarithmic structure of the full QCD result.https://doi.org/10.1007/JHEP10(2021)006JetsQCD Phenomenology
collection DOAJ
language English
format Article
sources DOAJ
author Andrea Banfi
Frédéric A. Dreyer
Pier Francesco Monni
spellingShingle Andrea Banfi
Frédéric A. Dreyer
Pier Francesco Monni
Next-to-leading non-global logarithms in QCD
Journal of High Energy Physics
Jets
QCD Phenomenology
author_facet Andrea Banfi
Frédéric A. Dreyer
Pier Francesco Monni
author_sort Andrea Banfi
title Next-to-leading non-global logarithms in QCD
title_short Next-to-leading non-global logarithms in QCD
title_full Next-to-leading non-global logarithms in QCD
title_fullStr Next-to-leading non-global logarithms in QCD
title_full_unstemmed Next-to-leading non-global logarithms in QCD
title_sort next-to-leading non-global logarithms in qcd
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2021-10-01
description Abstract Non-global logarithms arise from the sensitivity of collider observables to soft radiation in limited angular regions of phase space. Their resummation to next-to-leading logarithmic (NLL) order has been a long standing problem and its solution is relevant in the context of precision all-order calculations in a wide variety of collider processes and observables. In this article, we consider observables sensitive only to soft radiation, characterised by the absence of Sudakov double logarithms, and we derive a set of integro-differential equations that describes the resummation of NLL soft corrections in the planar, large-N c limit. The resulting set of evolution equations is derived in dimensional regularisation and we additionally provide a formulation that is manifestly finite in four space-time dimensions. The latter is suitable for a numerical integration and can be generalised to treat other infrared-safe observables sensitive solely to soft wide-angle radiation. We use the developed formalism to carry out a fixed-order calculation to O α s 2 $$ \mathcal{O}\left({\alpha}_s^2\right) $$ in full colour for both the transverse energy and energy distribution in the interjet region between two cone jets in e + e − collisions. We find that the expansion of the resummed cross section correctly reproduces the logarithmic structure of the full QCD result.
topic Jets
QCD Phenomenology
url https://doi.org/10.1007/JHEP10(2021)006
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