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D2HH lines: add monitoring and update selections

Merged Nico Kleijne requested to merge nkleijne/update_D2hh_lines into master

This MR updates the

D0hhD^0\rightarrow hh
lines. The changes are:

  • Add monitoring variables to be used during bandwidth division
  • Add a selections on decay time
    ctct
    of the
    D0D^0

Should me merged after !1225 (merged)

Edited by Nico Kleijne

Merge request reports

Merged by Rosen MatevRosen Matev 1 year ago (Jun 21, 2023 8:29am UTC)

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  • What is the improvement in efficiency obtained by introducing the IP selection in addition to the IPchi2 in the FilterTracks stage? It would be good to know the trade-off between the gain in physics and the slight decrease in throughput.

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    • f25b7688 - Higher pT and lower IP in FilterTracks

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    • Resolved by Dorothea Vom Bruch

      The proposal here is for commissioning stage, and it is intentionally loose. Further studies are ongoing, in particular in conjunction with the twin line on D0-KSHH decays (from @mamartin).

      For the exclusive D0-HH line we could set a tighter cut at the pre-filter level with no significant consequences. Nico already demonstrated that we can afford values up to IP>90microns with Run-3 design luminosity. The threshold at 60 microns is for commissioning and it is driven by studies performed in the past assuming a pT threshold for all HLT1 reconstructed tracks of 500 MeV (see https://indico.cern.ch/event/1118175/ ).

      While this pT threshold is ok for the D0-HH line, it might be too tight for the D0-KsHH, where both from Run 2 and 2022 data, we already know that low momentum tracks for this channel are of fundamental importance for efficiency. In conclusions, we believe that for commissioning stage the requirement in the FilterTracks —> “(pt>200MeV && IPCHI2>2) OR (pt>200MeV && IP>60microns)” would allow us performing all studies on both lines in preparation of high-lumi runs.

      I expect that the pT threshold could chance when luminosity will increase and it will be placed somewhere, between 200 and 500 MeV. This will depends on many factors, not only from the two exclusive lines mentioned in this MR. The IPCHI2 (and consequently the IP) cut will be accordingly modified to stay in the allowed throughput limits.

      Finally, I conclude by saying that these two exclusive lines do not have the primary goal of increasing the efficiency and the purity of the D0->hh and D0->KShh decay modes. For this we will exploit TrackMVA and TwoTrackMVA [this is especially true for the two-body line, while for the D0->KShh there might be some room to improve]. Here, the goal is to have a robust line, with no cuts on CHI2-like variables, and with a negligible correlation between D0 momentum and proper decay time, which is very dangerous for high-precision time-dependent measurements (DeltaY, yCP, bin-flip KsPiPi, D->Kpi WS/RS, lifetimes(?), …). We expect these lines to be almost completely overlapped with TrackMVA lines and not to disturb the data taking (I have also in mind the final output of the corresponding HLT2 lines). If that should be the case, we can just tight our requirements on pT and IP.

  • mentioned in issue Moore#574 (closed)

  • Edited by Software for LHCb
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