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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Online Access: | https://doi.org/10.1007/JHEP10(2021)006 |
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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 |
work_keys_str_mv |
AT andreabanfi nexttoleadingnongloballogarithmsinqcd AT fredericadreyer nexttoleadingnongloballogarithmsinqcd AT pierfrancescomonni nexttoleadingnongloballogarithmsinqcd |
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1716845116415541248 |