10–12 May 2012
U. Pittsburgh
US/Eastern timezone

Towards a more accurate prediction of W+b jet production with an automatized approach to one-loop calculations

10 May 2012, 15:30
30m
157 Benedum Hall (U. Pittsburgh)

157 Benedum Hall

U. Pittsburgh

(<a href="https://indico.cern.ch/conferenceDisplay.py/getPic?picId=2&amp;confId=156078" target="_blank">map</a>)

Speaker

Dr Laura Reina (CERN)

Description

We present results for the O(alpha_s) virtual corrections to qg ->W b bbar q' obtained with a new automatized approach to the evaluation of one-loop amplitudes in terms of Feynman diagrams. Together with the O(alpha_s) corrections to q qbar' -> W b bbar g, which can be obtained from our results by crossing symmetry, this represents the bulk of the next-to-leading order virtual QCD corrections to W b bbar + j and W b + j hadronic production, calculated in a fixed-flavor scheme with four light flavors. Furthermore, these corrections represent a well defined and independent subset of the 1-loop amplitudes needed for the NNLO calculation of W b bbar. Our approach was tested against several existing results for NLO amplitudes including selected O(alpha_s) one-loop corrections to W + 3j hadronic production. We discuss the efficiency of our method both with respect to evaluation time and numerical stability.

Summary

We present results for the O(alpha_s) virtual
corrections to qg ->W b bbar q' obtained with a
new automatized approach to the evaluation of one-loop
amplitudes in terms of Feynman diagrams. Together with
the O(alpha_s) corrections to q qbar' -> W b bbar g, which
can be obtained from our results by crossing symmetry, this
represents the bulk of the next-to-leading order virtual QCD
corrections to W b bbar + j and W b + j hadronic production,
calculated in a fixed-flavor scheme with four light flavors.
Furthermore, these corrections represent a well defined and
independent subset of the 1-loop amplitudes needed for the NNLO
calculation of W b bbar. Our approach was tested against several
existing results for NLO amplitudes including selected
O(alpha_s) one-loop corrections to W + 3j hadronic production.
We discuss the efficiency of our method both with respect to
evaluation time and numerical stability.

Author

Dr Laura Reina (CERN)

Presentation materials