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Second-order QCD corrections to event shape distributions in deep inelastic scattering
We compute the next-to-next-to-leading order (NNLO) QCD corrections to event shape distributions and their mean values in deep inelastic lepton–nucleon scattering. The magnitude and shape of the corrections varies considerably between different variables. The corrections reduce the renormalization a...
Autores principales: | , , , |
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Lenguaje: | eng |
Publicado: |
2019
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1140/epjc/s10052-019-7528-3 http://cds.cern.ch/record/2688982 |
_version_ | 1780963693874380800 |
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author | Gehrmann, T. Huss, A. Mo, J. Niehues, J. |
author_facet | Gehrmann, T. Huss, A. Mo, J. Niehues, J. |
author_sort | Gehrmann, T. |
collection | CERN |
description | We compute the next-to-next-to-leading order (NNLO) QCD corrections to event shape distributions and their mean values in deep inelastic lepton–nucleon scattering. The magnitude and shape of the corrections varies considerably between different variables. The corrections reduce the renormalization and factorization scale uncertainty of the predictions. Using a dispersive model to describe non-perturbative power corrections, we compare the NNLO QCD predictions with data from the H1 and ZEUS experiments. The newly derived corrections improve the theory description of the distributions and of their mean values. |
id | cern-2688982 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2019 |
record_format | invenio |
spelling | cern-26889822021-11-12T20:34:11Zdoi:10.1140/epjc/s10052-019-7528-3http://cds.cern.ch/record/2688982engGehrmann, T.Huss, A.Mo, J.Niehues, J.Second-order QCD corrections to event shape distributions in deep inelastic scatteringhep-phParticle Physics - PhenomenologyWe compute the next-to-next-to-leading order (NNLO) QCD corrections to event shape distributions and their mean values in deep inelastic lepton–nucleon scattering. The magnitude and shape of the corrections varies considerably between different variables. The corrections reduce the renormalization and factorization scale uncertainty of the predictions. Using a dispersive model to describe non-perturbative power corrections, we compare the NNLO QCD predictions with data from the H1 and ZEUS experiments. The newly derived corrections improve the theory description of the distributions and of their mean values.We compute the next-to-next-to-leading order (NNLO) QCD corrections to event shape distributions and their mean values in deep inelastic lepton-nucleon scattering. The magnitude and shape of the corrections varies considerably between different variables. The corrections reduce the renormalization and factorization scale uncertainty of the predictions. Using a dispersive model to describe non-perturbative power corrections, we compare the NNLO QCD predictions with data from the H1 and ZEUS experiments. The newly derived corrections improve the theory description of the distributions and of their mean values.arXiv:1909.02760CERN-TH-2019-140IPPP/19/68ZU-TH 39/19oai:cds.cern.ch:26889822019-09-06 |
spellingShingle | hep-ph Particle Physics - Phenomenology Gehrmann, T. Huss, A. Mo, J. Niehues, J. Second-order QCD corrections to event shape distributions in deep inelastic scattering |
title | Second-order QCD corrections to event shape distributions in deep inelastic scattering |
title_full | Second-order QCD corrections to event shape distributions in deep inelastic scattering |
title_fullStr | Second-order QCD corrections to event shape distributions in deep inelastic scattering |
title_full_unstemmed | Second-order QCD corrections to event shape distributions in deep inelastic scattering |
title_short | Second-order QCD corrections to event shape distributions in deep inelastic scattering |
title_sort | second-order qcd corrections to event shape distributions in deep inelastic scattering |
topic | hep-ph Particle Physics - Phenomenology |
url | https://dx.doi.org/10.1140/epjc/s10052-019-7528-3 http://cds.cern.ch/record/2688982 |
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