NLO EW corrections for Sherpa ZZ -> llvv samples

Talks

* 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.

-- KenjiHamano - 2020-03-23

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Topic revision: r1 - 2020-03-23 - KenjiHamano
 
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