Vectors + Multijet Theory with BlackHat and Sherpa

Vectors + Multijet Theory with BlackHat and Sherpa
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Vectors Multijet Theory with BlackHat and Sherpa David A. Kosower Institut de Physique Théorique, CEASaclay on behalf of the BlackHat Collaboration Carola Berger, Z. Bern, Giovanni Diana, L. Dixon, Fernando Febres Cordero, Darren Forde,

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Vectors + Multijet Theory with BlackHat and Sherpa David A. Kosower Institut de Physique Théorique, CEA–Saclay
on behalf of the BlackHat Collaboration
Carola Berger, Z. Bern, Giovanni Diana, L. Dixon, Fernando Febres Cordero, Darren Forde, Tanju Gleisberg, Stefan Höche, Harald Ita, DAK, Daniel Maître, Kemal Ozeren with contributions by Kurt Barry (ATLAS)
HCP 2011 November 15, 2011<br>
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Next-to-Leading Order in QCD Precision QCD requires at least NLO

QCD at LO is not quantitative: large dependence on unphysical renormalization and factorization scales
NLO: reduced dependence, first quantitative prediction


Want this not just for basic processes, but for every signal and background one
Even more important with many jets<br>
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Why NLO? Reduction of scale dependence

NLO importance grows with increasing number of jets

Expect predictions reliable to 10–15%<br>