Change LeptonID
The list of lines for which the NN cut is made available is the following:|
| MuonNN | Cut | BW division | Electron NN | Cut | BW division |
|---|---|---|---|---|---|
DiMuonDisplacedLine |
0.1 | Yes | Hlt1TrackElectronMVA |
0.7 | Yes |
DiMuonHighMassLine |
0.1 | Yes | DisplacedDielectronLine |
0.7 | Yes |
DiMuonNoIPLine |
0.95 | No | LowMassDielectronNoIPLine | 0.95 | Yes |
DiMuonDrellYanLine |
Chi2Corr cuts | No | LowMassDielectronDisplacedLine | 0.8 | Yes |
TrackMuonMVA |
0.1 | Yes | |||
Hlt1SMOG2DisplacedDiMuonLine |
Chi2Corr | No | |||
Hlt1SMOG2JpsiToMuMuTapLine |
Chi2Corr | No | |||
Hlt1SMOG2SingleMuon |
Chi2Corr | No | |||
DiMuonDisplacedSoftPTLine |
0.8 | No |
(Then actually all lines cutting on isElectron are changed since the MR also changes the defition of isElectron to be NN based > 0.6)
I have set different muonNN cuts following the logic that was chosen to select Chi2Corr cuts. These cuts are a bit more aggressive than Chi2Corr but hopefully it will help recover more efficiency as they should allow for much softer pT cuts. Then for some specific lines some more stringent cuts are chosen, these are especifically the Dark Photon lines.
This MR showcases an example to change the LeptonID based on the NN operators:
- Electrons: Define isElectron based on the NN setting a cut similarly efficient but reducing background twice as much:
NN
MB:
Hlt1DiElectronDisplaced: 21/ 10000, ( 423.00 +/- 35.37) kHz
jpsiee:
Hlt1DiElectronDisplaced: 2346// 10000, (10035.00 +/- 141.54) kHz
EoP
MB:
Hlt1DiElectronDisplaced: 47/ 10000, ( 141.00 +/- 20.52) kHz
jpsiee:
Hlt1DiElectronDisplaced: 2291/ 10000, ( 6873.00 +/- 126.08) kHz
ROC curves (A bit shaky because the fits are a bit unstable...)
| p_T \in [500,800] MeV | p_T \in [800,1200] MeV |
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| p_T \in [1200,2500] MeV | p_T \in [2500,4000] MeV |
|---|---|
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| p \in [3000,6000] MeV | p \in [6000,12000] MeV |
|---|---|
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| p \in [12000,20000] MeV | p > 20000 MeV |
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Features data(top) simulation (bottom): (slight cut on the NN to cleanup the electron background)
| EoP | EoP3x3 | delta_barycenter |
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| dispersion_x | dispersion_y | dispersion_xy |
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- Muons:
Go line by line and modify the Chi2Corr cut > 1.8 to loose cut of 0.1 which improves the background reduction also by 50% at the same efficiency point. In this example I modified the
DiMuonMassLinewhich shows these numbers for the Ks2MuMu as signal and MB as background. We see that we x10 lower rate on background, lowering the PT cut down to 0 MeV while keeping 50% more of the low PT muons.
NN
MB:
Hlt1DiMuonDisplaced: 9/ 10000, ( 27.00 +/- 9.00) kHz
ks2mumu:
Hlt1DiMuonDisplaced: 222/ 10000, ( 666.00 +/- 44.20) kHz
Chi2Corr and PT cut at 500 MeV
MB:
Hlt1DiMuonDisplaced: 91/ 10000, ( 273.00 +/- 28.49) kHz
ks2mumu:
Hlt1DiMuonDisplaced: 147/ 10000, ( 441.00 +/- 36.10) kHz
ROC curves (pion rejection:
| p_T \in [100,500] MeV | p_T \in [500,1000] MeV | p_T \in [1000,2000] MeV |
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| p \in [3000,7000] MeV | p \in [7000,12000 MeV | p > 12000 MeV |
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ROC curves (proton rejection, for this type of background the NN does not improve):
| p_T \in [500,1000] MeV | p_T \in [1000,2000] MeV |
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| p \in [3000,7000] MeV | p \in [7000,12000 MeV | p > 12000 MeV |
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Features data(top; muon vs proton)(mid; muon vs pion); simulation (bottom; actually trained on protons!):
| chi2coor | chi2uncorr | dtx |
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| dty | dty_velo |
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| Goes with: lhcb-datapkg/ParamFiles!128 (merged) (NN models update) |
Edit: I Have updated the roc curves, I'm refining the J/psi model, that's why they changed (are better).













































