Strong radiative corrections to W b bbar production in p pbar collisions

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dc.creatorEllis, R. K.
dc.creatorVeseli, S.
dc.date1998-10-26
dc.date.accessioned2026-07-07T10:52:57Z
dc.date.available2026-07-07T10:52:57Z
dc.descriptionWe calculate the strong radiative corrections to the process p pbar -> W(->e nu) g^*(->b bbar). At the Tevatron this process is the largest background to the associated Higgs boson production p pbar -> W(-> e nu) H(-> b bbar). The calculation is based on the subtraction procedure, and the corrections are found to be significant.
dc.description8 pages, latex, 4 postscript figures included
dc.identifierhttps://arxiv.org/abs/hep-ph/9810489
dc.identifierhttp://arxiv.org/abs/hep-ph/9810489
dc.identifierPhys.Rev.D60:011501,1999
dc.identifierdoi:10.1103/PhysRevD.60.011501
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/185326
dc.subjectHigh Energy Physics - Phenomenology
dc.titleStrong radiative corrections to W b bbar production in p pbar collisions
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