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QCD Corrections to Radiative $\Upsilon$ Decays

We calculate the next-to-leading order perturbative QCD corrections to the photon energy spectrum in radiative Upsilon decays We have calculated the next-to-leading order perturbative QCD corrections to the photon energy spectrum in radiative Upsilon decays. The higher-order corrections significantl...

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Autor principal: Krämer, Michael
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.60.111503
http://cds.cern.ch/record/385436
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author Krämer, Michael
author_facet Krämer, Michael
author_sort Krämer, Michael
collection CERN
description We calculate the next-to-leading order perturbative QCD corrections to the photon energy spectrum in radiative Upsilon decays We have calculated the next-to-leading order perturbative QCD corrections to the photon energy spectrum in radiative Upsilon decays. The higher-order corrections significantly modify the shape of the spectrum, in particular at large photon energies, and thereby reduce the discrepancy between experimental data and previous leading-order predictions. The next-to-leading order calculation of the photon energy spectrum allows a more reliable determination of the strong coupling constant from radiative Upsilon decays by restricting the analysis to the region of the energy spectrum that can be described by NLO perturbation theory.
id cern-385436
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
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spelling cern-3854362023-03-14T20:33:30Zdoi:10.1103/PhysRevD.60.111503http://cds.cern.ch/record/385436engKrämer, MichaelQCD Corrections to Radiative $\Upsilon$ DecaysParticle Physics - PhenomenologyWe calculate the next-to-leading order perturbative QCD corrections to the photon energy spectrum in radiative Upsilon decays We have calculated the next-to-leading order perturbative QCD corrections to the photon energy spectrum in radiative Upsilon decays. The higher-order corrections significantly modify the shape of the spectrum, in particular at large photon energies, and thereby reduce the discrepancy between experimental data and previous leading-order predictions. The next-to-leading order calculation of the photon energy spectrum allows a more reliable determination of the strong coupling constant from radiative Upsilon decays by restricting the analysis to the region of the energy spectrum that can be described by NLO perturbation theory.We have calculated the next-to-leading order perturbative QCD corrections to the photon energy spectrum in radiative Upsilon decays. The higher-order corrections significantly modify the shape of the spectrum, in particular at large photon energies, and thereby reduce the discrepancy between experimental data and previous leading-order predictions. The next-to-leading order calculation of the photon energy spectrum allows a more reliable determination of the strong coupling constant from radiative Upsilon decays by restricting the analysis to the region of the energy spectrum that can be described by NLO perturbation theory.hep-ph/9904416CERN-TH-99-106CERN-TH-99-106oai:cds.cern.ch:3854361999-04-22
spellingShingle Particle Physics - Phenomenology
Krämer, Michael
QCD Corrections to Radiative $\Upsilon$ Decays
title QCD Corrections to Radiative $\Upsilon$ Decays
title_full QCD Corrections to Radiative $\Upsilon$ Decays
title_fullStr QCD Corrections to Radiative $\Upsilon$ Decays
title_full_unstemmed QCD Corrections to Radiative $\Upsilon$ Decays
title_short QCD Corrections to Radiative $\Upsilon$ Decays
title_sort qcd corrections to radiative $\upsilon$ decays
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.60.111503
http://cds.cern.ch/record/385436
work_keys_str_mv AT kramermichael qcdcorrectionstoradiativeupsilondecays