Upload
others
View
3
Download
0
Embed Size (px)
Citation preview
Electron charge identification and study of the electroweakW±W±jj production with the ATLAS detector at 13 TeV
Giulia GonellaAlbert-Ludwigs-Universitat Freiburg
The Final HiggsTools Meeting
Durham, UK - September 12th, 2017
Overview
Vector boson scattering
The role in the EWK simmetry breaking investigation
Features
The WW channel
Background composition
Electron charge mis-identification: efficiencies measurement
Analysis overview
Electron charge mis-identification: background in the W±W±jj analysis
Summary
Giulia Gonella - W±W± jj production 12.09.2017 1 / 24
Why keeping working after the Higgs boson discovery?
• Is this the only Higgs boson in Nature?
• Is it doing the Higgs boson’s job?
Different paths to follow to answer (one or more of) these questions
Giulia Gonella - W±W± jj production 12.09.2017 2 / 24
Why keeping working after the Higgs boson discovery?
• Is this the only Higgs boson in Nature?
• Is it doing the Higgs boson’s job?
Different paths to follow to answer (one or more of) these questions
Giulia Gonella - W±W± jj production 12.09.2017 2 / 24
Many tools for the higgs investigation
• Measuring with higher precision its properties and couplings
• Investigating the high mass region
• Measuring the electroweak (EWK) vector boson interactions
The Standard Model (SM)
lagrangian predicts triple (TGC)
and quartic (QGC) gauge bosons
vertices
Lgauge = −1
4BµνBµν −
1
4W aµνWµν
a
= LGC + LTGC + LQGC
! Pure EWK verteces are suppressed by αEWK → rare processes
Ultimately: aiming to study quartic couplings
Giulia Gonella - W±W± jj production 12.09.2017 3 / 24
Many tools for the higgs investigation
• Measuring with higher precision its properties and couplings
• Investigating the high mass region
• Measuring the electroweak (EWK) vector boson interactions
The Standard Model (SM)
lagrangian predicts triple (TGC)
and quartic (QGC) gauge bosons
vertices
Lgauge = −1
4BµνBµν −
1
4W aµνWµν
a
= LGC + LTGC + LQGC
! Pure EWK verteces are suppressed by αEWK → rare processes
Ultimately: aiming to study quartic couplings
Giulia Gonella - W±W± jj production 12.09.2017 3 / 24
The role of Vector Bosons Scattering
• CERN Large Hadron Collider is providing promising statistics to access these
processes
• quartic couplings can be accessed in Vector Boson Scattering signatures
At hadron colliders VBS can be idealized as VVjj
at leading order (LO):
• two vector bosons (i.e. their respective decay products)
• two outgoing jets
BUT
VBS diagrams are not separately gauge invariant and must be studied in conjunction
with additional Feynman diagrams leading to the same VVjj final state.
Giulia Gonella - W±W± jj production 12.09.2017 4 / 24
VVjj final state diagrams
Theoretically there are two classes of physical processes.
• Electroweak production: Only Weak interaction
• O(α6EWK )
• VBS signal in it
• It contains also:
purely EWK process which give the same final state
processes with 3 decaying vector boson (only 1 decaying hadronically)
Giulia Gonella - W±W± jj production 12.09.2017 5 / 24
VVjj final state diagrams
Theoretically there are two classes of physical processes.
• Electroweak production: Only Weak interaction
• Strong production: Both strong and EWK interaction
• O(α4EWKα
2S )
Giulia Gonella - W±W± jj production 12.09.2017 6 / 24
WW scattering
Without a light SM Higgs boson the VBS amplitude of longitudinally polarized W
bosons increases with√
s and violates unitarity at energies around 1 TeV.
↓
The SM Higgs boson should avoid this problem
WW scattering is a key process to probe EWKSBWe can establish if the Higgs boson can preserve unitarity of the VBS at all energies
• Test of the Higgs boson nature
• The discovered Higgs boson
contribute fully to the EWKSB
↓
WW interaction remain weak at high
energies
• Model independent research ofalternative theory
• The discovered Higgs boson is
partially responsible for the EWKSB
↓
WW interaction get strong at high
energy
arXiv:1412.8367
Giulia Gonella - W±W± jj production 12.09.2017 7 / 24
Choosing the right process: W±W±jj channel
C. Gumpert, PhD Thesis, CERN-THESIS-2014-290
W±W±jj production:
• lower background from QCD production: σEWK/σQCD '11 ( σEWK/σQCD '0.6
for opposite sign)
The same-charge selection restricts the number of diagrams involved
Giulia Gonella - W±W± jj production 12.09.2017 8 / 24
Choosing the right process: W±W±jj channel
C. Gumpert, PhD Thesis, CERN-THESIS-2014-290
W±W±jj production:
• lower background from QCD production: σEWK/σQCD '11 ( σEWK/σQCD '0.6
for opposite sign)
The same-charge selection restricts the number of diagrams involved
Giulia Gonella - W±W± jj production 12.09.2017 8 / 24
Background composition
SM processes can mimic the signature ``′ + E missT +2 jets
Type Sources Reduction
1 SC leptons
WZ+jets
veto on third leptonZZ+jets
ttV
2 OC charge mis-ID
tt → `ν`νbb b-jet veto +SC req.
W±W∓ + jets
Z/γ∗+jets→ `±`∓+jets large E missT +mZ peak excl.
3 Jets, γ mis-reco
W +jets
tt → `νjjbbb-jet veto+E miss
Tsingle top
Wγ+jets tight isolation+veto on third lepton
Giulia Gonella - W±W± jj production 12.09.2017 9 / 24
It’s important to keep in mind that the other SM processes have muchlarger cross section compared to our signal!
pp
total (x2)
inelastic
JetsR=0.4
dijets
incl .
γ
fid.
pT > 125 GeV
pT > 25 GeV
nj ≥ 1
nj ≥ 2
nj ≥ 3
pT > 100 GeV
W
fid.
nj ≥ 0
nj ≥ 1
nj ≥ 2
nj ≥ 3
nj ≥ 4
nj ≥ 5
nj ≥ 6
nj ≥ 7
Z
fid.
nj ≥ 1
nj ≥ 2
nj ≥ 3
nj ≥ 4
nj ≥ 5
nj ≥ 6
nj ≥ 7
nj ≥ 0
nj ≥ 1
nj ≥ 2
nj ≥ 3
nj ≥ 4
nj ≥ 5
nj ≥ 6
nj ≥ 7
ttfid.
total
nj ≥ 4
nj ≥ 5
nj ≥ 6
nj ≥ 7
nj ≥ 8
t
tot.
Zt
s-chan
t-chan
Wt
VVtot.
ZZ
WZ
WW
ZZ
WZ
WW
ZZ
WZ
WW
γγ
fid.
H
fid.
H→γγ
VBFH→WW
ggFH→WW
H→ZZ→4ℓ
H→ττ
total
WV
fid.
Vγ
fid.
Zγ
W γ
ttW
tot.
ttZ
tot.
ttγ
fid.
WjjEWK
fid.
ZjjEWK
fid.
WWExcl.
tot.
Zγγ
fid.
Wγγ
fid.
WWγ
fid.
ZγjjEWKfid.
VVjjEWKfid.
W ±W ±
WZ
σ[p
b]
10−3
10−2
10−1
1
101
102
103
104
105
106
1011 Theory
LHC pp√s = 7 TeV
Data 4.5 − 4.9 fb−1
LHC pp√s = 8 TeV
Data 20.3 fb−1
LHC pp√s = 13 TeV
Data 0.08 − 36.1 fb−1
Standard Model Production Cross Section Measurements Status: July 2017
ATLAS Preliminary
Run 1,2√s = 7, 8, 13 TeV
Giulia Gonella - W±W± jj production 12.09.2017 10 / 24
The challenges
Many challenges enter this analysis:
• very low cross-section compared to other SM processes
• many SM backgrounds can be reduced with dedicated cuts, but still some of
them need to be estimated
• big impact of background from non-prompt leptons (fakes)
• big impact of background from charge mis-reconstruction
↓
always better to estimate these backgrounds with data-driven methods (“Data model
data better than Monte Carlo”)
In the following focus on charge mis-identification background
In order to estimate the charge mis-ID background it’s important to precisely know
the probability of an electron to have its charge wrongly reconstructed:
• measurement of electron charge mis-identification efficiencies
• data-driven estimation of background from charge mis-identification
Giulia Gonella - W±W± jj production 12.09.2017 11 / 24
The source of charge mis-ID
Charge (mis-)reconstruction
• Conversion of bremsstrahlung photon
e-primary electron
conversion electron
γbrem
e+
e-primary electron
reconstructed electronwith wrong charge
γbrem
e+
• Wrong track reconstruction
primary electron
reconstructed electronwith wrong charge
• very rare effects
• very hard to properly model in detector simulation
• the effect have to be measured on data
In ATLAS objects measurements are performed inside Combined Performance groups. This one in particular has
been carried out in the Electron-photon CP group
Giulia Gonella - W±W± jj production 12.09.2017 12 / 24
The source of charge mis-ID
Charge (mis-)reconstruction
• Conversion of bremsstrahlung photon
e-primary electron
conversion electron
γbrem
e+
e-primary electron
reconstructed electronwith wrong charge
γbrem
e+
• Wrong track reconstruction
primary electron
reconstructed electronwith wrong charge
• very rare effects
• very hard to properly model in detector simulation
• the effect have to be measured on data
In ATLAS objects measurements are performed inside Combined Performance groups. This one in particular has
been carried out in the Electron-photon CP group
Giulia Gonella - W±W± jj production 12.09.2017 12 / 24
The source of charge mis-ID
Charge (mis-)reconstruction
• Conversion of bremsstrahlung photon
e-primary electron
conversion electron
γbrem
e+
e-primary electron
reconstructed electronwith wrong charge
γbrem
e+
• Wrong track reconstruction
primary electron
reconstructed electronwith wrong charge
• very rare effects
• very hard to properly model in detector simulation
• the effect have to be measured on data
In ATLAS objects measurements are performed inside Combined Performance groups. This one in particular has
been carried out in the Electron-photon CP group
Giulia Gonella - W±W± jj production 12.09.2017 12 / 24
Measuring the efficiencies
GeVllM60 70 80 90 100 110 120
even
ts/G
eV
0
500
1000
1500
2000
2500
3000
310×
OS events
SS events
ATLAS Work in progress
• Double differential measurement in
4×6 bins in pT × |η|
• measured in Z → e+e− events
• εi probability electron charge mis-reconstructed in
bin i . Assume εi independent
Nexpsc = np = n
[(1− εi ) εj +
(1− εj
)εi
]Building likelihood function:
• binomial counting: probability of nsc SC events:( nnsc
)pnsc (1− p)n−nsc
• approximated Poisson distribution
P(nsc|εi , εj
)=
(Nexpsc )nsc e−Nexp
sc
nsc!≡ L(εi , εj )
• L =∏
i,j L(εi , εj )
Efficiencies obtained by minimizing −ln(L)
|η|0 0.5 1 1.5 2 2.5
mis
-ID
∈
3−10
2−10
1−10
[25,60] GeV∈ T
p
[60,90] GeV∈ T
p
[90,130] GeV∈ T
p
[130,1000] GeV∈ T
p
ATLAS Internal, 2016 data-133.9 fb
Tp
40 60 80 100 120 140
mis
-ID
∈3−10
2−10
1−10
ATLAS Internal, 2016 data-133.9 fb
[0.0,0.6]∈| η| [0.6,1.1]∈| η| [1.1,1.52]∈| η| [1.52, 1.7]∈| η| [1.7, 2.3]∈| η| [2.3, 2.5]∈| η|
arxiv:1612.01456Giulia Gonella - W±W± jj production 12.09.2017 13 / 24
Measuring the efficiencies
GeVllM60 70 80 90 100 110 120
even
ts/G
eV
0
500
1000
1500
2000
2500
3000
310×
OS events
SS events
ATLAS Work in progress
• Double differential measurement in
4×6 bins in pT × |η|
• measured in Z → e+e− events
• εi probability electron charge mis-reconstructed in
bin i . Assume εi independent
Nexpsc = np = n
[(1− εi ) εj +
(1− εj
)εi
]Building likelihood function:
• binomial counting: probability of nsc SC events:( nnsc
)pnsc (1− p)n−nsc
• approximated Poisson distribution
P(nsc|εi , εj
)=
(Nexpsc )nsc e−Nexp
sc
nsc!≡ L(εi , εj )
• L =∏
i,j L(εi , εj )
Efficiencies obtained by minimizing −ln(L)
|η|0 0.5 1 1.5 2 2.5
mis
-ID
∈
3−10
2−10
1−10
[25,60] GeV∈ T
p
[60,90] GeV∈ T
p
[90,130] GeV∈ T
p
[130,1000] GeV∈ T
p
ATLAS Internal, 2016 data-133.9 fb
|η|0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
] 0R
adia
tion
leng
th [X
0
0.5
1
1.5
2
2.5 ServicesTRTSCTPixelBeam-pipe
ATLASSimulation
arxiv:1612.01456Giulia Gonella - W±W± jj production 12.09.2017 13 / 24
Scale factors
Tp
40 60 80 100 120 140
rate
s
3−10
2−10
1−10
datamcATLAS Internal
[1.52, 1.7]∈| η|
Tp
40 60 80 100 120 140
SF
SS
0.6
0.8
1
1.2
1.4
|η|0 0.5 1 1.5 2 2.5
rate
s
3−10
2−10
1−10 datamcATLAS Internal
[90, 130] GeV∈ T
p
|η|0 0.5 1 1.5 2 2.5
SF
SS
0.6
0.8
1
1.2
1.4
• efficiencies highly dependent on process and kinematic
selection
• scale factors are produce where these effects cancel
• they can also be used to study the effeiciencies of other
processes
• scale factors are derived for right charge and wrong
charge electrons to correct MC
SFwrong =εdata
εMCSFright =
1− εdata
1− εMC
0.8506 1.0662 0.8508 1.0948
0.7524 0.6884 0.7634 1.1763
0.6716 0.7525 0.9382 0.9647
0.6803 0.6679 0.7773 0.9437
0.9007 1.0002 0.9707 1.0326
0.9095 1.0091 1.1332 0.9740
GeVT
p40 60 80 100 120 140
|η|
0
0.5
1
1.5
2
2.5
0.7
0.8
0.9
1
1.1
1.0000 1.0000 1.0003 0.9997
1.0002 1.0007 1.0010 0.9989
1.0007 1.0012 1.0006 1.0006
1.0021 1.0047 1.0052 1.0023
1.0010 1.0000 1.0011 0.9979
1.0024 0.9995 0.9894 1.0030
GeVT
p40 60 80 100 120 140
|η|
0
0.5
1
1.5
2
2.5
0.7
0.8
0.9
1
1.1
• corrections for wrong charge electrons up to ∼30%
• corrections for right charge electrons never bigger than 0.5%Giulia Gonella - W±W± jj production 12.09.2017 14 / 24
Prelude: W±W±jj analysis topology
• 2 high-pT jets in the forward regions
(2 jets with highest pT )
• No color exchange in the hard
scattering process → rapidity gap in
the central part of the detector
• large mjj and mWWjj
jj y∆
0 1 2 3 4 5 6 7 8 9
arbi
trar
y un
its
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.1jj, electroweak±W± W
jj, strong±W± WATLAS Internal
Plot: "CutNJets/DYjj"
[GeV]jjm
0 100 200 300 400 500 600 700 800 900 1000
arbi
trar
y un
its
3−10
2−10
jj, electroweak±W± W
jj, strong±W± WATLAS Internal
Plot: "CutNJets/Mjj"
Two analysis regions could be defined, using the EWK specific topologies as
discriminant cuts:
• Inclusive region: signal = EWK+QCD
• VBS region: signal = EWK → additional cut on |∆yjj | > 2.4Giulia Gonella - W±W± jj production 12.09.2017 15 / 24
Prelude: W±W±jj analysis topology
• 2 high-pT jets in the forward regions
(2 jets with highest pT )
• No color exchange in the hard
scattering process → rapidity gap in
the central part of the detector
• large mjj and mWWjj
jj y∆
0 1 2 3 4 5 6 7 8 9
arbi
trar
y un
its
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.1jj, electroweak±W± W
jj, strong±W± WATLAS Internal
Plot: "CutNJets/DYjj"
[GeV]jjm
0 100 200 300 400 500 600 700 800 900 1000
arbi
trar
y un
its
3−10
2−10
jj, electroweak±W± W
jj, strong±W± WATLAS Internal
Plot: "CutNJets/Mjj"
Two analysis regions could be defined, using the EWK specific topologies as
discriminant cuts:
• Inclusive region: signal = EWK+QCD
• VBS region: signal = EWK → additional cut on |∆yjj | > 2.4Giulia Gonella - W±W± jj production 12.09.2017 15 / 24
Studies of EWK-QCD separation and interference
Interference between O(α4
QCD
)strong and O
(α6
EWK
)electroweak W±W±jj
production to be studied:
∣∣∣MWWjjSM
∣∣∣2 =∣∣∣MWWjj
QCD +MWWjjEWK
∣∣∣2 =∣∣∣MWWjj
QCD
∣∣∣2 +∣∣∣MWWjj
EWK
∣∣∣2 +∣∣∣MWWjj
INT
∣∣∣2
• interference varies from few percent to few ten-percent
• negative in some regions
• will be included as systematic uncertainty on the EWK
signal
Giulia Gonella - W±W± jj production 12.09.2017 16 / 24
Contributions at final selection
• analysis performed in four channels: eµ, µe, µµ and ee
• different background composition between channels
• main backgrounds: WZ , fakes and charge mis-ID (not µµ channel)
As anticipated the main challenges in this analysis are related to the fake background
and the charge mis-identification one
Giulia Gonella - W±W± jj production 12.09.2017 17 / 24
Charge mis-ID background
The technique
• charge mis-ID background estimated from data
• same-charge events are estimated from opposite-charge events
• opposite charge data are scaled with
w =ε1 + ε2 − 2ε1ε2
1− (ε1 + ε2 − 2ε1ε2)
[GeV]l0T
p20 40 60 80 100 120 140 160 180 200 220
effic
ienc
y
0.005
0.01
0.015
0.02
0.025
0.03
0.035
0.04bkg/ee/Zjetsbkg/ee/top/Nom/ttbar
ATLAS Work in progress-1= 13 TeV, 36.1 fbs
• ε1,2: charge mis-ID rates for e1,2
• rates appear to be process
dependent
Giulia Gonella - W±W± jj production 12.09.2017 18 / 24
The data-driven estimate
The final aim
We want a data-driven estimation of the charge mis-identification background
remaining in the SR
opposite-charge data
same-charge estimation
where
ε1,2: charge misID rates. P for `1,2 charge to be mis-identified
→ rates from data are needed to build the weights
Giulia Gonella - W±W± jj production 12.09.2017 19 / 24
From SF to rates
0.8506 1.0662 0.8508 1.0948
0.7524 0.6884 0.7634 1.1763
0.6716 0.7525 0.9382 0.9647
0.6803 0.6679 0.7773 0.9437
0.9007 1.0002 0.9707 1.0326
0.9095 1.0091 1.1332 0.9740
GeVT
p40 60 80 100 120 140
|η|
0
0.5
1
1.5
2
2.5
0.7
0.8
0.9
1
1.1
1.0000 1.0000 1.0003 0.9997
1.0002 1.0007 1.0010 0.9989
1.0007 1.0012 1.0006 1.0006
1.0021 1.0047 1.0052 1.0023
1.0010 1.0000 1.0011 0.9979
1.0024 0.9995 0.9894 1.0030
GeVT
p40 60 80 100 120 140
|η|
0
0.5
1
1.5
2
2.5
0.7
0.8
0.9
1
1.1
↓
• apply the SF to MC so that it matches the probability of mis-identification of data
• get rates from MC using the truth information
ε =wrong charge ele
all ele
0.00023 0.00018 0.00021 0.00016 0.00022 0.00026 0.00057 0.00166
0.00036 0.00037 0.00027 0.00033 0.00016 0.00031 0.00083 0.00214
0.00057 0.00086 0.00050 0.00052 0.00051 0.00050 0.00148 0.00287
0.00138 0.00121 0.00135 0.00098 0.00083 0.00133 0.00266 0.00565
0.00214 0.00221 0.00212 0.00148 0.00141 0.00196 0.00377 0.01195
0.00396 0.00268 0.00273 0.00100 0.00277 0.00527 0.00511 0.01435
0.00434 0.00597 0.00594 0.00423 0.00334 0.00610 0.00932 0.01826
0.00987 0.00984 0.01071 0.00859 0.00738 0.01039 0.01937 0.03169
0.00777 0.00666 0.00830 0.00711 0.00457 0.00930 0.01841 0.03699
0.00847 0.00758 0.00797 0.00781 0.00727 0.00888 0.02190 0.03853
0.00711 0.00792 0.00806 0.00940 0.00741 0.01330 0.02139 0.03957
0.01196 0.00948 0.01290 0.01050 0.01097 0.01368 0.02636 0.044380.01029 0.01171 0.01532 0.01407 0.01311 0.02164 0.03569 0.053570.02454 0.02373 0.02548 0.02640 0.02288 0.03324 0.05156 0.094270.01930 0.02662 0.02645 0.03144 0.03297 0.03627 0.05422 0.088030.01754 0.02799 0.02593 0.03324 0.03276 0.04560 0.05427 0.09273
GeVl0T
p30 40 50 60 70 80 90
l0 |η|
0
0.5
1
1.5
2
2.5
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
Giulia Gonella - W±W± jj production 12.09.2017 20 / 24
Energy corrections needed
Up to this point of the workflow a simple scaling is applied to OC data:
• the integral is modified
• the distribution of charge flip estimation is identical to OC data one
• SC events have lower energy wrt OC one, because of the energy leakage due to
Bremsstrahlung emission
arbi
trar
y un
its
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.1 data, same-charge
data, opposite-chargeATLAS Work in progress-1 = 13 TeV, 36.1 fbs
[GeV]llm
75 80 85 90 95 100 105
ratio
00.5
11.5
2
Giulia Gonella - W±W± jj production 12.09.2017 21 / 24
Energy corrections needed
Up to this point of the workflow a simple scaling is applied to OC data:
• the integral is modified
• the distribution of charge flip estimation is identical to OC data one
• SC events have lower energy wrt OC one, because of the energy leakage due to
Bremsstrahlung emission
arbi
trar
y un
its
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.1 data, same-charge
DY MC, opposite-charge
DY MC, same-charge
data, opposite-charge
ATLAS Work in progress-1 = 13 TeV, 36.1 fbs
[GeV]llm
75 80 85 90 95 100 105
ratio
00.5
11.5
2
Giulia Gonella - W±W± jj production 12.09.2017 21 / 24
Energy corrections needed
Up to this point of the workflow a simple scaling is applied to OC data:
• the integral is modified
• the distribution of charge flip estimation is identical to OC data one
• SC events have lower energy wrt OC one, because of the energy leakage due to
Bremsstrahlung emission
arbi
trar
y un
its
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.1 data, same-charge
charge flip estimate
DY MC, opposite-charge
DY MC, same-charge
data, opposite-charge
ATLAS Work in progress-1 = 13 TeV, 36.1 fbs
[GeV]llm
75 80 85 90 95 100 105
ratio
00.5
11.5
2
Giulia Gonella - W±W± jj production 12.09.2017 21 / 24
The scaling and the smearing
The four-momentum of OC data used for the estimation is modified
• pT is shifted towards smaller values
• pT is smeared to match the worse resolution
pcorrectedT = pscaled
T + dE
The scaling is based on the energy response
response =preco
T
ptruthT
− 1
which is different for correctly reconstructed and wrongly reconstructed electrons
- 1l0,truth
T/pl0,reco
Tp
0.8− 0.6− 0.4− 0.2− 0 0.2 0.4 0.6 0.8
arbi
trar
y un
its
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08 stat. unc. Drell-YanATLAS Internal
-1 = 13 TeV, 36.1 fbs
channelν±eν±e
- 1l0,truth
T/pl0,reco
Tp
0.8− 0.6− 0.4− 0.2− 0 0.2 0.4 0.6 0.8
l0 η
2.5−
2−
1.5−
1−
0.5−
0
0.5
1
1.5
2
2.5
0
500
1000
1500
2000
2500
3000
3500
4000ATLAS Internal
-1 = 13 TeV, 36.1 fbs
channelν±eν±e
Giulia Gonella - W±W± jj production 12.09.2017 22 / 24
The scaling and the smearing
The four-momentum of OC data used for the estimation is modified
• pT is shifted towards smaller values
• pT is smeared to match the worse resolution
pcorrectedT = pscaled
T + dE
The scaling is based on the energy response
response =preco
T
ptruthT
− 1
which is different for correctly reconstructed and wrongly reconstructed electrons
- 1l0,truth
T/pl0,reco
Tp
0.8− 0.6− 0.4− 0.2− 0 0.2 0.4 0.6 0.8
arbi
trar
y un
its
0
0.01
0.02
0.03
0.04
0.05
0.06 stat. unc. Drell-YanATLAS Internal
-1 = 13 TeV, 36.1 fbs
channelν±eν±e
- 1l0,truth
T/pl0,reco
Tp
0.8− 0.6− 0.4− 0.2− 0 0.2 0.4 0.6 0.8
l0 η
2.5−
2−
1.5−
1−
0.5−
0
0.5
1
1.5
2
2.5
0
5
10
15
20
25
30
35
40ATLAS Internal-1 = 13 TeV, 36.1 fbs
channelν±eν±e
Giulia Gonella - W±W± jj production 12.09.2017 22 / 24
The estimation in the ee channel
Eve
nts
/ 1 G
eV
0
200
400
600
800
1000
1200
1400 Data stat. unc.±W± W Top
VV + VVV γ W+
γ Z+ charge-flip
fakes
ATLAS Internal-1 = 13 TeV, 36.1 fbs
channelν±eν±e
[GeV]llm
70 75 80 85 90 95 100 105 110
Dat
a / M
C
00.20.40.60.8
11.21.41.61.8
2E
vent
s / 5
GeV
0
500
1000
1500
2000
2500
3000 Data stat. unc.
±W± W Top VV + VVV γ W+
γ Z+ charge-flip
fakes
ATLAS Internal-1 = 13 TeV, 36.1 fbs
channelν±eν±e
[GeV]l0
Tp
20 40 60 80 100 120 140 160 180 200 220
Dat
a / M
C
00.20.40.60.8
11.21.41.61.8
2
Eve
nts
/ 0.2
0
200
400
600
800
1000
1200 Data stat. unc.±W± W Top
VV + VVV γ W+
γ Z+ charge-flip
fakes
ATLAS Internal-1 = 13 TeV, 36.1 fbs
channelν±eν±e
l0η
2− 1− 0 1 2
Dat
a / M
C
00.20.40.60.8
11.21.41.61.8
2
• the ee channel is dominated by charge mis-ID background
• the estimation seems to match quite nicely with data
• studies and optimizations ongoing
Giulia Gonella - W±W± jj production 12.09.2017 23 / 24
Summary
Two main working areas have been shown...
→ electron charge mis-ID SF measurement
• performed within the ATLAS e/γ combined performance group
• official recommendations provided to physics analyses inside the collaboration
• the work will be documented in the e/γ paper
→ estimation of the charge mis-ID background in the W±W±jj analysis
• process of estrapolation of the rates for the analysis has been shown
• the impact of this background is huge in the SR, much work needed to get a
precise estimation
• the technique for this has been studied and implemented inside the analysis
framework
• further corrections have been performed
WW scattering is a key process for SM and EWSB mechanism
• same charge final state is a clean signature of electroweak production
• on the other side the low cross-section and the large background from charge
mis-identification make the W±W±jj analysis a difficult path
Very challenging time yet to come to put Standard Model to stringent test
Giulia Gonella - W±W± jj production 12.09.2017 24 / 24
Phase space for fiducial cross sections (slide 8)
• Sherpa
• defined at parton level
• plepT ≥ 25 GeV
• |ηlep | ≤ 2.5
• ∆R lep ≥ 0.3
• minimum m`` of all charged lepton pair combinations ≥ 20 GeV
• at least 2 jets pjetT ≥30 GeV
• |ηjet | ≤ 4.5
• ∆R lep,jet ≥ 0.3
• mjj ≥ 500 GeV
• |∆η| ≥ 2.4
ATLAS Run 1 results in the W±W±jj channel
First evidence for W±W±jj production and EWK-only W±W±jj production @ 8 TeV
σfidincl = 2.1 ± 0.5 (stat) ± 0.3 (syst) fb
• Significance: 4.5σ
• σexp = 1.52 ± 0.11 fb
σfidVBS = 1.3 ± 0.4 (stat) ± 0.2 (syst) fb
• Significance: 3.6σ
• σexp = 0.95 ± 0.06 fb
Goal for Run 2
Measurement of the EWK production cross section → 5σ observation reachable within
LHC operation plans
Yields Run 1 analysis
Inclusive region VBS region
e±e± e±µ± µ±µ± e±e± e±µ± µ±µ±
W±W±jj QCD 0.89 ± 0.15 2.5 ± 0.4 1.42 ± 0.23 0.25 ± 0.06 0.71 ± 0.14 0.38 ± 0.08
W±W±jj EWK 3.07 ± 0.30 9.0 ± 0.8 4.9 ± 0.5 2.55 ± 0.25 7.3 ± 0.6 4.0 ± 0.4
Total background 6.8 ±1.2 10.3 ± 2.0 3.0 ± 0.6 5.0 ± 0.9 8.3 ± 1.6 2.6 ± 0.5
Total predicted 10.7 ± 1.4 21.7 ± 2.6 9.3 ± 1.0 7.6 ± 1.0 15.6 ± 2.0 6.6 ± 0.8
Data 12 26 12 6 18 10
50 signal candidates with 20 background expectation for ISR
34 signal candidates with 16 background expectation for VBS
Fiducial regions Run 1 analysis
Two fiducial regions are defined to follow the selections applied in the analysis
• Inclusive region:• 2 same sign leptons with
• pT > 25 GeV
• |η| < 2.5
• m`` > 20 GeV
• ∆R`` =√
(∆Φ)2 + (∆η)2 > 0.3
• At least 2 anti-kt jets with
• R = 0.4
• pT > 30 GeV
• |η| < 4.5
• ∆R`j > 0.3
• mjj (highest pT jets) > 500 GeV
• E missT > 40 GeV
• VBS region: cuts above + rapidity cut
|∆yjj | > 2.4
Run 1 event selection
Events selection used for the analysis:
• event cleaning
• exactly two selected leptons with m`` > 20 GeV
• veto events with additional veto leptons
• q`1× q`2
> 0
• pT > 25 GeV
• |m`` −mZ | > 10 GeV in the ee channel
• E missT ≥ 40 GeV
• at least two jets with pT > 30 GeV and |η| < 4.5
• b-jet veto
• mjj > 500 GeV
• |∆yjj | > 2.4 - VBS analysis region
Cross section changes from 8 TeV to 13 TeV
Signal samples generated with Sherpa 2.1.1, LO up to 3 additional partons:
QCD EWK
8 TeV 13 TeV 13 TeV/8 TeV 8 TeV 13 TeV 13 TeV/8 TeV
σprod [fb] 10.1 25.9 2.6 16.4 43.0 2.6
Rates dependency on material
• Rate of wrongly reconstructed charge strongly depends on material distribution:
Z and R for the first detector interaction using Z MC truth:
wrong sign interact primarily with beam pipe and pixel
Current selection
• p`1,`2T >27 GeV → under optimization studies
• m`` > 20 GeV → under optimization studies
• q`1× q`2
> 0
• 3rd lepton veto
• pjT > 30 GeV → under optimization studies
• |η|j < 4.5
• E missT ≥ 30 GeV
• mjj > 500 GeV → under optimization studies
• |∆yjj | > 2.4 → under optimization studies
Energy correction derivation
• response is derived
response =preco
T
ptruthT
− 1
for right charge and wrong charge electrons, differentially in η
• defining α as
α =1 + responseright
1 + responsewrong
• pT is corrected as:
pscaledT =
poldT
α
• smearing is based on dE , random number in Gauss distribution:
dE = Gauss
(0 ,sqrt
(err2
wrong
(1 + responsewrong )2−
err2right
(1 + responseright )2
))pscaled
T
Acceptances and efficiencies for W±W±jj
• Calculated on Sherpa 2.2.1
• σtotEWK = 37.4fb and σtot
QCD = 23.5fb
• acceptance on fiducial selection is a few percent
→ σfidEWK = 1.97fb and σtot
QCD = 0.30fb
CMS analysis - Selection and yields
ATLAS CMS
dataset 2015+2016 2016
Ldx 36.1 fb−1 35.9 fb−1
p`T 26 GeV 25/20 GeV
|η| 2.5 2.4/2.5
pjT /E j
T 25/30 GeV 30 GeV
m`` 20 GeV 20 GeV
E missT 30 GeV 40 GeV
Z -veto (ee) 15 GeV 15 GeV
mjj 500 GeV 500 GeV
∆yjj/∆ηjj 2.4 2.5
max(z∗` ) - 0.75
veto 3` < 10 GeV <10 GeV
veto τhad - >18 GeV
veto b-jet 3 3
With respect to ATLAS analysis:
• less WZ background
• higher non-prompt
Zeppenfeld variable z∗ =
∣∣∣η`−(ηj1|ηj2
)/2∣∣∣∣∣∣∆ηjj
∣∣∣
CMS analysis - Some details
General information
• charge flip rate: 0.01% in the barrel, 0.3% in the endcap (ATLAS: 0.07% barrel,
3.5% endcap)
• charge flip contribution estimated from MC with data scale factors
• fake-factor method yields 30% uncertainty
• third lepton CR (with Z mass window) yields 20%-40% uncertainty
• significance extracted from 2-dim fit in m`` and mjj
Signal:
• purely EWK6, contributions from EWK4 are subtracted
• theoretical uncertainties 12% (αs ), 5% (PDF) and 4.5% (EWK6-EWK4
interference)
• LO cross-section from Madgraph (also signal sample): σtheofid = 4.25± 0.21 fb−1
Cross section result:
σfid (W±W±jj) = 3.83± 0.66(stat.)± 0.35(syst.) fb
CMS analysis - BSM interpretation
Anomalous Quartic Couplings
• EFT lagrangian of nine C- and
P-conserving dim-8 operators
modifying quartic couplings
Doubly charged Higgs boson
• Doubly charged Higgs bosons
predicted by models with Higgs triplet
field
• couplings depend on m(H±) and
sin2 θH
• Georgi-Machacek model of Higgs
triplet considered
• limits presented for
σVBF (H±±)× B(H±± →W±W±)
and sH ≡ sin θH
Scale factor systematics
Four sources:
• m`` variation (nominal: 15GeV)
• trigger matchig requirement on sub-leading candidate
• background subtraction on/off
• truth matching comparison
These are combined and propagated in the derivation of the data-driven background
→ variation up/down (7-15%)
→ energy correction on/off (2-7%)