NLO EW corrections for Sherpa ZZ -> llvv samples
Talks
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llvv meeting on 28 Cot 2019 EW corrections for ZZ (Sarah Heim): a talk that summarizes what we got from the theorists:
EW k-factors
EW k-factors. I would use d03-x01-y01 for now (Zvv pt, Zmass selection). The HM selection is in d05-x01-y01, you can see that the numbers are quite close but cut-off at 120 GeV.
The k factors we use are the average, and the uncertainty band spreads over the difference.
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KenjiHamano - 2020-03-23