The Milan factor for jet-shape observables

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dc.creatorSalam, G. P.
dc.date1998-05-14
dc.date.accessioned2026-07-07T04:03:52Z
dc.date.available2026-07-07T04:03:52Z
dc.descriptionThis talk discusses and explains the two-loop corrections, also known as the Milan factor, for power corrections to jet-shape observables.
dc.description6 pages, uses moriond.sty (included). Contribution to "Rencontres de Moriond, QCD and hadronic interactions," Les Arcs, France, April 1998, and to "DIS98, 6th International Workshop on Deep Inelastic Scattering," Brussels, Belgium, April 1998
dc.identifierhttps://arxiv.org/abs/hep-ph/9805323
dc.identifierhttp://arxiv.org/abs/hep-ph/9805323
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/47847
dc.subjectHigh Energy Physics - Phenomenology
dc.titleThe Milan factor for jet-shape observables
dc.typetext

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