Tau Reconstruction at CMS - University of California,...
Transcript of Tau Reconstruction at CMS - University of California,...
Tau Reconstruction at CMS
Evan Friis
Outline
• Taus at hadron colliders
• Tau ID algorithms at CMS
• Tau ID measurements in 2010
• Z→ττ standard candle
• SVfit: τ pair mass reconstruction
• MSSM H→ττ
Tau ID at hadron colliders
• Exciting new physics signals could appear in tau channels
• QCD Jets can fake taus
• QCD background is very large!
• Dominant background in many analyses is fake taus
0.1 1 1010-7
10-6
10-5
10-4
10-3
10-2
10-1
100
101
102
103
104
105
106
107
108
109
10-7
10-6
10-5
10-4
10-3
10-2
10-1
100
101
102
103
104
105
106
107
108
109
WJS2009
jet(ETjet > 100 GeV)
jet(ETjet > s/20)
jet(ETjet > s/4)
Higgs(MH=120 GeV)
200 GeV
LHCTevatron
eve
nts
/ sec
for L
= 1
033 c
m-2s-1
b
tot
proton - (anti)proton cross sections
W
Z
t
500 GeV
(nb
)
s (TeV)http://projects.hepforge.org/mstwpdf/plots/plots.html
Particle Flow Algorithm
• Clusters and links signals from all subdetectors
• Produces a list of particle candidates
• To the user looks just like Monte Carlo
taus in CMS are built using Particle Flow objects
h h0 e μ γ
2/21!"#$%&'()*&+,*--*(.(/0123441(
!"#$"%#&'()*#(+,$)%-.#(/.0&(,.10$%)*2!"#$"%#&'()*#(+,$)%-.#(/.0&(,.10$%)*2
5/64
/"+7-*$7
0/64
/"+7-*$7
8$&9:7
,*-*9-#$
;&$-%9"*<="#>
8?*("%7-(#=(%',%@%,+&"(;&$-%9"*7(%7(-?*'(+7*,(-#(A+%",(B*-7C(-#(
,*-*$D%'*(-?*(D%77%'E(-$&'7@*$7*(*'*$EFC(-#($*9#'7-$+9-(&',(
%,*'-%=F(-&+7(=$#D(-?*%$(,*9&F(;$#,+9-7C(-#(-&E(A(B*-7(G(
F. Beaudette
Particle Flow Performance
Et-60 -50 -40 -30 -20 -10 0 10 20 30 40
#
0
50
100
150
200
250
300
350
400
450
Particle Flow Jets
Calo Tower Jets
Jet Transverse Energy Resolution
50 GeV Et tau
CMS Preliminary
Particle Flow
Tau ET resolution
SIM Particle Flow resolvesoverlaps in subdectors
Improves resolution
Traditional CMS Tau ID
geometrically defined isolationdefine geometric region around tau
candidate and require low detector activity
see CMS PAS PFT-08-001
relies on the fact that taus are more collimated than QCD
CMS Physics Technical Design Report (PTDR) results use these algorithms
!"#$%"&"'()*"+,-$./0$1/0$23$%"425$6(7"8$
!"
#$%%"&'(")*+,"-./"
012.3&."4"!"!"(",+"5&"
678$94:19;"8$3<"19=<".>5"$7<?=")+@".$4:A"
"!".BC.81&.9=$D"E1;9$=?8."<2":$F8<914"'G>'H"I.4$J"("KG>KHL"MG>MHL"$)"#.%<9"
"!"N1&"=<"8.4<9%=8?4="MO"""KO"KPL"$)"""KO"KPL"$)"""KG"KH"KGL"$)"""KH"KG"KH"19"'GQ.="
I.4$J%"C8.F<&19$9=DJ"19=<":$F8<9%R"
Decay Mode CMS Tau IDParticle Flow algorithm allowsexamination of meson content
two new algorithms:Hadrons Plus Strips (HPS) algorithm
Tau Neural Classifier (TaNC) algorithm
GOAL:optimize tau identification for individual tau decay modes
Hadrons Plus Strips Algorithmbuild signal components combinatorially
cluster gammas into π0 candidates using η-φ strips
γ γ γ
γ
φ
η
π0
π0
π+
π+ π0
π+ π+ π-
build all possible tausthat have a ʻtau-likeʼ multiplicity
from the seed jet
tau that is ʻmost isolatedʼ with compatible mvis
is the final tau candidate associated to the seed jet0.05
0.20
Tau Neural Classifiera neural network for each decay mode
cluster gammas into π0 candidates by combinatoric pairs compatible with mπ0
γ γ γ
γ
φ
η
π0
π0π+
π+ π0
π+ π0 π0
π+ π+ π-
π+ π+ π- π0
signal objects are defined using shrinking cone
depending on decay mode
a different neural networkis applied!
Tau Performancemeasuring the fake rate is easy
(no lack of background at the LHC)
fake rate is different for W+jets, multi-jet, heavy flavor
independently measuring signal efficiency is hard
in practice efficiency extracted in situ in Z and Higgs analyses
Fake Rate measurement8 6 Fake–rate measurement
0 20 40 60 80 100 120 140 160180 200
fake
rate
from
jets
!
-310
-210 Data"µ#W
Simulation"µ#W
QCDj Data
QCDj Simulation
DataµQCD
SimulationµQCD
TaNC loose
-1=7 TeV, 36 pbsCMS Preliminary 2010,
(GeV/c)T
jet p0 50 100 150 200
Sim
ulat
ion
Dat
a-Si
m.
-0.20
0.2 0 20 40 60 80 100 120 140 160180 200
fake
rate
from
jets
!-310
-210
Data"µ#W
Simulation"µ#W
QCDj Data
QCDj Simulation
DataµQCD
SimulationµQCD
HPS loose
-1=7 TeV, 36 pbsCMS Preliminary 2010,
(GeV/c)T
jet p0 50 100 150 200
Sim
ulat
ion
Dat
a-Si
m.
-0.20
0.2
Figure 5: Probabilities of quark and gluon jets to pass “loose” working points of the TaNC (left)
and HPS (right) algorithms as a function of jet pT for QCD, QCD µ-enriched and W type events.
Fake-rate measured in data are represented by solid symbols and compared to MC prediction
represented by open symbols.
efficiency!expected 0.1 0.2 0.3 0.4 0.5 0.6
fake
rate
from
jets
!m
easu
red
-310
-210
efficiency!expected 0.1 0.2 0.3 0.4 0.5 0.6
fake
rate
from
jets
!m
easu
red
-310
-210
PTDR, W+jetµPTDR, QCD
TaNC, W+jetµTaNC, QCD
HPS, W+jetµHPS, QCD
-1=7 TeV, 36 pbsCMS Preliminary 2010,
Figure 6: The measured fake–rate as a function of MC estimated efficiency for all working
points for QCD µ-enriched and W data samples. The PTDR points represent results of the
fixed cone algorithm based on the PF taus.
open points = simulation closed points = data
TANC HPS
red is W+jets purple is heavy flavor
TAU-11-001
Tau ID Performance
purple info box
8 6 Fake–rate measurement
0 20 40 60 80 100 120 140 160180 200
fake
rate
from
jets
!
-310
-210 Data"µ#W
Simulation"µ#W
QCDj Data
QCDj Simulation
DataµQCD
SimulationµQCD
TaNC loose
-1=7 TeV, 36 pbsCMS Preliminary 2010,
(GeV/c)T
jet p0 50 100 150 200
Sim
ulat
ion
Dat
a-Si
m.
-0.20
0.2 0 20 40 60 80 100 120 140 160180 200
fake
rate
from
jets
!
-310
-210
Data"µ#W
Simulation"µ#W
QCDj Data
QCDj Simulation
DataµQCD
SimulationµQCD
HPS loose
-1=7 TeV, 36 pbsCMS Preliminary 2010,
(GeV/c)T
jet p0 50 100 150 200
Sim
ulat
ion
Dat
a-Si
m.
-0.20
0.2
Figure 5: Probabilities of quark and gluon jets to pass “loose” working points of the TaNC (left)
and HPS (right) algorithms as a function of jet pT for QCD, QCD µ-enriched and W type events.
Fake-rate measured in data are represented by solid symbols and compared to MC prediction
represented by open symbols.
efficiency!expected 0.1 0.2 0.3 0.4 0.5 0.6
fake
rate
from
jets
!m
easu
red
-310
-210
efficiency!expected 0.1 0.2 0.3 0.4 0.5 0.6
fake
rate
from
jets
!m
easu
red
-310
-210
PTDR, W+jetµPTDR, QCD
TaNC, W+jetµTaNC, QCD
HPS, W+jetµHPS, QCD
-1=7 TeV, 36 pbsCMS Preliminary 2010,
Figure 6: The measured fake–rate as a function of MC estimated efficiency for all working
points for QCD µ-enriched and W data samples. The PTDR points represent results of the
fixed cone algorithm based on the PF taus.
3X improvement since PTDR
TAU-11-001
Tag & Probe efficiency• Preselect Z→τμτhad using loose isolation + Z analysis cuts
• Fit ττ Mvis passing/failing spectra composition
• Method robust against Higgs contamination in Z peak
4 4 Efficiency of tau reconstruction and identification.
data driven background estimates instead of the MC templates and by varying invariant mass
ranges for the fit. All checks demonstrated consistent results within the uncertainties of the
method.
)2 visible mass (GeV/cjet!µ
20 40 60 80 100 120 140 160 180 200
num
ber o
f eve
nts
0
10
20
30
40
50
60
70Data
-! +! " *#Z/QCDW + jets
-µ +µ " *#Z/ + jetstt
-1=7 TeV, 36 pbsCMS Preliminary 2010,
)2 visible mass (GeV/cjet!µ
20 40 60 80 100 120 140 160 180 200
num
ber o
f eve
nts
0
20
40
60
80
100
120Data
-! +! " *#Z/QCDW + jets
-µ +µ " *#Z/ + jetstt
-1=7 TeV, 36 pbsCMS Preliminary 2010,
Figure 2: The visible invariant mass of the µτjet system for preselected events which passed
(left) and failed (right) the HPS “loose” tau identification requirements compared to predictions
of the MC simulation.
Algorithm Fit data Expected MC DATA/MC
TaNC “loose” 0.76 ± 0.20 0.72 1.06 ± 0.30
TaNC “medium” 0.63 ± 0.17 0.66 0.96 ± 0.27
TaNC “tight” 0.55 ± 0.15 0.55 1.00 ± 0.28
HPS “loose” 0.70 ± 0.15 0.70 1.00 ± 0.24
HPS “medium” 0.53 ± 0.13 0.53 1.01 ± 0.26
HPS “tight” 0.33 ± 0.08 0.36 0.93 ± 0.25
HPS “loose” combined fit [4] 0.94 ± 0.09
HPS “loose” ττ to µµ, ee fit [4] 0.96 ± 0.07
Table 1: Efficiency for hadronic tau decays to pass TaNC and HPS tau identification criteria
measured by fitting the Z → τ+τ−signal contribution in the samples of the “passed” and
“failed” preselected events. The errors of the fit represent statistical uncertainties. The last
column represents the data to MC correction factors and their full uncertainties including sta-
tistical and systematic components. Data to MC ratios for the tau reconstruction efficiency
measured using fits to the measured Z production cross sections as described in [4] are also
shown.
Results of the fits are summarized in Table 1. The values measured in data, “Fit data” are com-
pared with the expected values, “Expected MC”, obtained by repeating the fitting procedure
on simulated events. The performance of the tau algorithms on preselected events is expected
to be approximately 30% higher than for an inclusive sample of taus, without pre-selection.
In general the absolute value of the efficiency depends on pT and η requirements, which are
applied in each individual physics analysis, therefore the main goal of this measurement is to
perform the data to MC comparison and to determine data to MC correction factors and their
uncertainties. With the current data sample the statistical uncertainties of the fits are in the
result: DATA/MC ≅ 1.0 ± 25%
HPS loose HPS loose
PASSED FAILED
TAU-11-001
Zττ cross section
• Analysis goal: understand taus at CMS
• Four channels: μ-had, e-had, e-μ, μ-μ
• ~25% τ-ID uncertainty limits utility as test of Standard model
• Instead: believe in lepton universalityand use Z peak to measure τ-ID
• Combined fit of all channels
•! N = Nobs – Nbgr
Background Contribution Nbgr estimated from Data
(using 1-3 complementary Methods, depending on Channel)
•! Acceptance taken from Monte Carlo
(POWHEG + TAUOLA, PYTHIA with CMS Z2 tune for Hadronization)
•! Efficiency factorized into independent Terms
Each Term either measured directly in Data or taken from Monte Carlo
and applying Data/MC Correction factor measured from Data
•! Branching Ratios for !+!- to decay into µ + !had, e + !had, e + µ, µ + µ
taken from PDG
•! Luminosity measured with Precision of 4%
Christian Veelken Higgs and Z ! !+!- in CMS 6
Cross-section Extraction
!
EWK-10-013
Z→ττ cross section6 7 Cross section measurement
Visible Mass [GeV]0 50 100 150 200
Even
ts /
(10
GeV
)
0
50
100
150
data!! " Z
t EWK+t QCD
yields from fit
CMS preliminary
= 7 TeVs at -136 pb
had!µ " !! "Z
Visible Mass [GeV]0 50 100 150 200
Even
ts /
(10
GeV
)
0
50
100
150
data!! " Z
t EWK+t QCD
yields from fit
CMS preliminary
= 7 TeVs at -136 pb
had! e" !! "Z
Invariant Mass [GeV]µe-0 50 100 150 200
Even
ts /
(10
GeV
)
0
10
20
30
40
50
data!! " Z
t EWK+t QCD
yields from fit
CMS preliminary
= 7 TeVs at -136 pbµ e" !! "Z
Invariant Mass [GeV]µ-µ0 50 100 150 200
Even
ts /
(10
GeV
)
1
10
210
310
data!! " Z
µµ "* # Z/ QCD
yields from fit
CMS preliminary
= 7 TeVs at -136 pbµµ " !! "Z
Figure 2: Visible mass distributions of the τµτhad (top left), τeτhad (top right), τeτµ (bottom left),and τµτµ (bottom right) final states.
τµτhad τeτhad τeτµ τµτµ
Acceptance: A 0.13 0.12 0.074 0.16Selection efficiency: � 0.40 0.25 0.55 0.17Mass window correction: fc 0.94 0.94 0.98 0.99
Table 3: Acceptance obtained with POWHEG for 60 < Mττ < 120 GeV and the selectionefficiency. The fraction of selected events outside the generator level mass window is alsoshown.
The measured values of the cross section for the four channels considered are:
σ (pp→ ZX)× B (Z→ ττ)µτ = 0.81± 0.07 (stat.)± 0.04 (syst.)± 0.09 (lumi.)± 0.19 (τ-ID) nb
σ (pp→ ZX)× B (Z→ ττ)eτ = 0.91± 0.11 (stat.)± 0.04 (syst.)± 0.10 (lumi.)± 0.21 (τ-ID) nbσ (pp→ ZX)× B (Z→ ττ)eµ = 0.99± 0.12 (stat.)± 0.06 (syst.)± 0.11 (lumi.) nb
σ (pp→ ZX)× B (Z→ ττ)µµ = 1.14± 0.25 (stat.)± 0.10 (syst.)± 0.12 (lumi.) nb.
The values are compatible with each other and with the next-to-next-to-leading-order (NNLO)175
final Zττ events selected
non-tau backgrounds measured from data
EWK-10-013
Combined Zττ Fitsimultaneously fit all channels for σz AND ετID
e-μ and μ-μ channels drive σZττ central value
Christian Veelken Higgs and Z ! !+!- in CMS
Measured Cross-Section in good Agreement with Theory Prediction (NNLO)
and CMS Measurement of Z/!* ! "+"-, l = e/µ Cross-section
Data/MC Correction factor for Tau Identification Efficiency compatible with 1.0
10
Simultaneous Fit Results
Combined:
" " BR(Z/!* ! !+!-) = 0.99 ± 0.06 (stat.) ± 0.08 (sys.) ± 0.04 (lumi.) nb
8 7 Cross Section Measurement
Table 4: The measured values of the cross section from the four final states considered. The
statistical, systematic and luminosity uncertainties are given. The uncertainty associated to the
τhad reconstruction and identification efficiency, τhad − ID, is shown separately.
Final state σ (pp → ZX)× B (Z → τ+τ−) nb stat. syst. lumi. τ ID
τµτhad 0.83 0.07 0.04 0.03 0.19
τeτhad 0.94 0.11 0.03 0.04 0.22
τeτµ 0.99 0.12 0.06 0.04
τµτµ 1.14 0.27 0.04 0.05
(left), where the likelihood contours for the best estimates of the cross section and the τhad effi-
ciency scale factor are shown. In addition to the one-standard-deviation contour, the contours
for which the likelihood L is reduced by 2∆ ln L = 2.30 and 6.18 compared to the maximum
vaue are also shown, corresponding to a coverage of 68% and 95% in the 2-parameter plane,
respectively. The value of the cross section extracted from the fit is
σ (pp → ZX)× B�Z → τ+τ−� = 1.00 ± 0.05 (stat.)± 0.08 (syst.)± 0.04 (lumi.) nb,
which is compared to the individual final state measurements in Fig. 3 (right). The value for218
the cross section is dominated by the dilepton final states which have smaller systematic un-219
certainties. In the simultaneous fit, the τhad-ID scale factor is measured to be 0.93 ± 0.09.220
A more precise value of the hadronic tau reconstruction efficiency can be obtained by perform-221
ing a fit of the τµτhad and τeτhad final states, where the cross section is fixed to the value mea-222
sured by CMS in the electron and muon decay channels, σ (pp → ZX)× B (Z → e+e−, µ+µ−)223
= 0.931 ± 0.026 (stat.)± 0.023 (syst.)± 0.102 (lumi.) nb [6]. The extracted value of the τhad-ID224
scale factor is 0.96± 0.07, which corresponds to a tau identification efficiency of (47.4± 3.3)% in225
data, for hadronically decaying tau leptons in the Z → τ+τ− sample with visible pT > 20 GeV226
within the detector acceptance.227
-ID Efficiency (data/sim)had!0.6 0.8 1 1.2 1.4
) [n
b]!!
" B
(Z
# Z
X)
"(p
p $
0.7
0.8
0.9
1
1.1
1.2
1.3
68% CL
95% CL
central value
$ 1 ±
CMS
= 7 TeVs at -136 pb
) [nb]!! " B(Z # ZX) "(pp $0.5 1 1.5 2 2.5
NNLO, FEWZ+MSTW08 [PDF4LHC 68% CL] (60-120 GeV)
µµ ee, "Z µ! + e!
µ! + µ!
had! + µ!
had! + e!
(combined) !! "Z
luminosity uncertainty not shown
CMS = 7 TeVs at -136 pb
Figure 3: Likelihood contours for the joint parameter estimation of the cross section and the
τ-identification (left). The fitted central values (solid line) and their estimated 1σ uncertainties
(dashed lines) are also shown. Summary of the measured Z → τ+τ− cross sections in the
τµτhad, τeτhad, τeτµ, and τµτµ final states, in the invariant mass range of 60 < Mτ+τ− < 120 GeV
(right). The inner error bar represents the statistical uncertainty. The extracted cross section
from the combined fit and the NNLO theoretical prediction are also shown.
assume σZττ = σZee/μμ →ετID MC/DATA = 0.96±0.07Taus are well understood objects at CMS!
fitted ετID MC/DATA = 0.93±0.09
EWK-10-013
searches with taus
Tau pair mass reconstruction• Searches for new resonances to taus
• Tau pair invariant mass is the most natural observable
• Tau decays have invisible component
• Recovery methods:
• Collinear approximation
• SVfit algorithm
• Missing Mass algorithm (see Alexeiʼs talk)
The Collinear Approximation• Assume neutrinos collinear with visible products
• Approximates true ττ mass
τvis1
τvis2
MET
METx = P ν1 sin θ1 cos φ1 + P ν
2 sin θ2 cos φ2
METy = P ν1 sin θ1 sin φ1 + P ν
2 sin θ2 sin φ2
Very sensitive to MET angular resolution!
~45% of events thrown awaydue to unphysical negative energies
SVfit mass reconstructionparameterize the physics of tau decays
maximize a likelihood function w.r.t. the tau decay parameters
• decay phase-space
• reconstructed neutrinos and measured MET
• “pT-balance” regularization
• compatibility with tracker information (optional)
likelihood terms:
Decay Parameterizationa τ decay can be completely described by:
θ Rest frame angle between boost and visible decay productions
φ Azimuthal angle of visible decay products about boost direction
minvis Mass of invisible decay
product system (minvis = 0 for τhad)
R Flight distance in lab frame
Decay Parameterizationreconstructing the tau energy
Evis = m2τ+m2
vis−m2νν
2mτ
rest frame visible energy:
sin θLAB = pvis sin θpLAB
vis
Lorentz invariant component of visible momentum
Solve Lorentz transformation along boost for γ
pLABvis cos θLAB = γβEvis + γpvis cos θ
ELABτ = γmτ
Decay Parameterizationreconstructing the tau direction
sin θLAB = pvis sin θpLAB
vis
constrains τ direction to lie on cone with angle θLAB about visible momentum
azimuthal fit parameter φ determines direction
flight path R determineslocation of decay vertex
(optional) PV
θL
φ
R
uvis
Phase Space Likelihood• Two or three-body decay
• Hadronic decays trivial
• Leptonic decays depend on mνν
Decays are assumed to be isotropic: |M|2 = 1
Investigating extending term to account for polarization correlations between taus
Possible handle to separate Higgses from Zs!
3.2 Likelihood for tau decay 5
laboratory frame of the visible momentum component parallel to the tau direction:
P̄viscos θ̄ = γEvis + βγPvis
cos θ
⇒ γ =Evis[
�Evis�2 +
�P̄vis
cos θ̄�2 −
�Pvis
cos θ�2]1/2 − Pvis
cos θP̄viscos θ̄
(Evis)2 − (Pvis cos θ)2,
Eτ = γmτ
The energy of the tau lepton in the laboratory frame as function of the measured visible mo-155
mentum depends on two of the three parameters only - the rest frame opening angle θ and the156
invariant mass mνν of the neutrino system. The direction of the tau lepton momentum vector157
is not fully determined by θ and mνν, but is constrained to lie on the surface of a cone of open-158
ing angle θ̄ (given by equation 2), the axis of which is given by the visible momentum vector.159
The tau lepton four–vector is fully determined by the addition of the third parameter φ̄, which160
describes the azimuthal angle of the tau lepton with respect to the visible momentum vector.161
3.2 Likelihood for tau decay162
The probability density functions for the tau decay kinematics are taken from the kinematics
review of the PDG [12]. The likelihood is proportional to the phase–space volume for two–
body (τ → τhadν) and three–body (τ → eνν and τ → µνν) decays. For two–body decays the
likelihood depends on the decay angle θ only:
dΓ ∝ |M|2 sin θdθ
For three–body decays, the likelihood depends on the invariant mass of the neutrino system
also:
dΓ ∝ |M|2 ((m2τ − (mνν + mvis)2)(m2
τ − (mνν −mvis)2))1/2
2mτmννdmνν sin θdθ (3)
In the present implementation of the SVfit algorithm, the matrix element is assumed to be163
constant, so that the likelihood depends on the phase–space volume of the decay only1.164
3.2.1 Likelihood for reconstructed missing transverse momentum165
Momentum conservation in the plane perpendicular to the beam axis implies that the vectorial166
sum of the momenta of all neutrinos produced in the decay of the tau lepton pair matches the167
reconstructed missing transverse momentum. Differences are possible due to the experimental168
resolution and finite PT of particles escaping detection in beam direction at high |η|.169
The Emiss
Tresolution is measured in Z → µ+µ− events selected in the 7 TeV data collected by
CMS in 2010. Corrections are applied to Monte Carlo simulated events to match the resolution
measured in data. The momentum vectors of reconstructed Emiss
Tand neutrino momenta given
by the fit parameters are projected in direction parallel and perpendicular to the direction of the
τ+τ− momentum vector. For both components, a Gaussian probability function is assumed.
The width and mean values of the Gaussian in parallel (“�”) and perpendicular (“⊥”) direction
1The full matrix elements for tau decays may be added in the future, including terms for the polarization of the
tau lepton pair, which is different in Higgs and Z decays [19].
MET likelihood• Compare SV-fitted neutrinos to
measured missing transverse energy
• Resolution of MET parameterized by ΣET of the event
• Resolution measured in Z→μμ events
Zμμ events
PT - balance likelihoodto reduce background one must apply
kinematic thresholds on visible decay products
significantly biases the kinematic distributions
3.3 Secondary vertex information 7
]2 [GeV/c!!SV fit M0 50 100 150 200 250 300 3500
0.02
0.04
0.06
0.08
0.1
0.12
0.14 balanceTwith p balanceTwithout p
Figure 1: Distribution of di–tau invariant mass reconstructed by the SVfit algorithm in simu-
lated Higgs events with MA = 130 GeV /c2. The SVfit algorithm is run in two configurations,
with (blue) and without (red) the PT–balance likelihood term included in the fit.
Visible energy fraction0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.02
0.04
0.06
0.08
0.1 cutTbefore P cutTafter P
Visible energy fraction0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.02
0.04
0.06
0.08
0.1
0.12 cutTbefore P
cutTafter P
Figure 2: Normalized distributions of the fraction of total tau decay energy carried by the muon
(left) and hadronic constituents (right) in simulated Higgs events with MA = 130 GeV /c2. The
distribution is shown before (blue) and after (red) the requirement on the PT of the visible decay
products described in section 5.1.
The motivation to add the PT–balance likelihood to the SVfit is to add a “regularization” term172
which compensates for the effect of PT cuts applied on the visible decay products of the two tau173
leptons. In particular for tau lepton pairs produced in decays of resonances of low mass, the174
visible PT cuts significantly affect the distribution of the visible momentum fraction x = EvisEτ
.175
The effect is illustrated in figures 2 and 3. If no attempt would be made to compensate for176
this effect, equations 3.2, 3 would yield likelihood values that are too high at low x, resulting177
in the SVfit to underestimate the energy of visible decay products (overestimate the energy of178
neutrinos) produced in the tau decay, resulting in a significant tail of the reconstructed mass179
distribution in the high mass region. The τ+τ− invariant mass distribution reconstructed with180
and without the PT–balance likelihood term is shown in figure 1. A significant improvement181
in resolution and in particular a significant reduction of the non–Gaussian tail in the region of182
high masses is seen.183
3.3 Secondary vertex information184
The parametrization of the tau decay kinematics described in section 3.1 can be extended to185
describe the production and decay of the tau. As the flight direction of the tau is already fully186
for Z/H μ-had channel: pTμ > 15 GeV, pThad > 20 GeV
τ → μνν τ → τhν H(130)H(130)
pT balance term: probability for decay pT from mass M
PT - balance likelihoodterm which represents the probability P(pT | Mττ)
first assume isotropic decay of resonance M at rest
each decay product has P(pT)Piso(pT ) ∝ pT�
1− (2pT /M)2
smear with Gaussian and add Gamma to account for resolution and non-zero boost
Ptotal(pT ) ∝ Piso(pT )⊗ exp(− p2T
2s2) + aΓ(pT , k, θ)
smear, Gamma fraction and shape are fitted as first order functions of Mττ
Tracking constraint
• Use tracker information
• Constrain fitted SV to lie on track with error
• Constrain flight time R
• Not currently used.Working to understandalignment issues.
Taus have non-negligible lifetime: cτ = 87µm
θL
φ
R
uvis
track
SV
SVfit Performance
]2 [GeV/c!!M0 50 100 150 200 250
Even
ts
0
50
100
150
200
250
300SV fit
Collinear approx.
CMS Preliminary=30" tan!!#(120)$
= 7 TeVs
]2 [GeV/c!!M0 50 100 150 200 250
a.u.
0
0.02
0.04
0.06
0.08
0.1
0.12
0.14 SV fit
Collinear approx.
CMS Preliminary Simulation! ! "Z
= 7 TeVs
normalized to unity normalized to luminosity
SV fit has better resolution than collinear approximation (left)SV fit has twice the acceptance as the collinear solution (right)
SVfit Performance
]2mass [GeV/c0 50 100 150 200 250 300
a.u.
0
0.02
0.04
0.06
0.08
0.1
0.12
0.14
0.16
0.18
0.2
0.22 SV fit
Visible mass
1.88!Visible mass
CMS Preliminary=30" tan##$(160)%
= 7 TeVs
SVfit peaks at di-tau massbetter relative resolution that visible mass
Extensions to SVfit
• Implement tracking likelihood
• Improve pT-balance parameterization
• Use polarization information
• Integration instead of maximization (similar to DLM, MMC)
• Extend code to fit N leptons
• Application to W→τν, H++, etc
currently under development
MSSM H→ττ Search• Taus one of the best handles for MSSM
• Benefit from tanβ enhancement σ and BR
• Search performed with three channels:
• μ + τhad
• e + τhad
• μ + e
• Tau ID correction factor floats in final fit,constrained by Z peak & 25% tag-probe
• All backgrounds measured from data
purple info box
MSSM H→ττ Search
4 5 Systematic Uncertainties
!"#$%&'()*+,#-'!) .
/
/*
)/*
/**
)**
0**
1**
!"#$%&'()*+,#-'!) .
%23+4256+72&&+(,#-'!).* /** )** 0** 1**
*
89"#:
;
<=>?+%%; !!, !@
7A+B+)**+,#-'!)
=CD+E6#F575$26G0H+49I/+++J+K#-
Figure 1: The reconstructed tau pair invariant mass distribution on linear (above) and log (be-
low) scales, for the sum of the eτh, µτh, and eµ final states, comparing the observed distributions
(data points with error bars) to the sum of the expected backgrounds (shaded histograms). The
contribution from a Higgs boson signal (mA = 200 GeV/c2) is also shown, with normalization
corresponding to the 95% upper bound.
results
final Mττ distributionof all channels
no bumps
HIG-10-002
MSSM Expected Limits46 17 Results
]2m(A) [GeV/c100 200 300 400 500
)!!"
BR
(h#
$Ex
pect
ed li
mit
on
1
10
210
310-1 = 7 TeV, L = 35 pbsCMS Preliminary,
had! µ " !!
had! e " !! µ e " !!
Combined
]2m(A) [GeV/c100 200 300 400 500
)!!"
BR
(h#
$Ex
pect
ed li
mit
on
1
10
210
310-1 = 7 TeV, L = 35 pbsCMS Preliminary,
had! µ " !!
had! e " !! µ e " !!
Combined
Figure 33: The expected Bayesian limits on σ× BR(H → ττ) in pb obtained for τe-τhad, τµ-τhad
and τe-τµ final states separately and for their combination using the visible mass, Mvis in fit (leftplot) and fully reconstructed mass, Mττ in the fit
τe-τµ final states separately and for their combination using the visible mass, Mvis in fit (left690
plot) and fully reconstructed mass, Mττ in the fit.
]2m(A) [GeV/c100 200 300 400 500
)!!"
BR(
h#
$O
bser
ved
limit
on
1
10
210
310-1 = 7 TeV, L = 35 pbsCMS Preliminary,
had! µ " !!
had! e " !! µ e " !!
Combined
]2m(A) [GeV/c100 200 300 400 500
)!!"
BR(
h#
$O
bser
ved
limit
on
1
10
210
310-1 = 7 TeV, L = 35 pbsCMS Preliminary,
had! µ " !!
had! e " !! µ e " !!
Combined
Figure 34: The observed Bayesian limits on σ× BR(H → ττ) in pb obtained for τe-τhad, τµ-τhad
and τe-τµ final states separately and for their combination using the visible mass, Mvis in fit (leftplot) and fully reconstructed mass, Mττ in the fit
691
Figure 35 shows the expected and observed limits on σ × BR(H → ττ) in pb obtained from692
combination of τe-τhad, τµ-τhad and τe-τµ final states using the visible mass, Mvis in fit (left plot)693
and fully reconstructed mass, Mττ in the fit.694
Figure 36 shows the expected and observed limits on σ × BR(H → ττ) in pb obtained from695
combination of τe-τhad, τµ-τhad and τe-τµ final states using the visible mass, Mvis and fully re-696
constructed mass, Mττ in the fit.697
Figure 37 shows the expected limits obtained for τe-τhad, τµ-τhad and τe-τµ final states separately698
and for their combination using the visible mass, Mvis in fit (left plot) and fully reconstructed699
mass, Mττ in the fit.700
Visible mass SVfitExpected Bayesian 95% CL limits
on σH × BR(H→ττ)
SVfit improves limit by 10%
100 200 300 400 5001
10
210
310had! µ " !!
had! e " !! µ e " !!
Combined
HIG-10-002
MSSM Observed Limitobserved limit on σH × BR(H→ττ)
5
signal and the main background, Z → ττ, equally. This effectively allows the observed Z → ττ112
events to provide an in situ calibration of this efficiency, except for Higgs masses near that of113
the Z. Near the Z mass, the tau identification efficiency uncertainty dominates in the eτh and114
µτh channels and the eµ channel provides the greatest sensitivity.115
6 Results116
The mass spectra show no evidence for the presence of a Higgs boson signal, and we set 95%117
C.L. upper bounds on the Higgs boson cross section times the tau pair branching ratio (denoted118
σφ · Bττ) using a Bayesian method assuming a uniform prior in σφ · Bττ. The invariant mass119
spectrum in Fig. 1 shows the contribution of a Higgs boson signal corresponding to mA = 200120
GeV/c2
with σφ · Bττ = 8.71 pb, the value above which we exclude at 95% C.L.121
Figure 2 shows the observed 95% C.L. upper bound on σφ · Bττ as a function of mA, where we122
use as our signal acceptance model the combined spectra from the gg and bb̄ production pro-123
cesses for h, A, and H, assuming tan β = 30 [22]. The plot also shows the one- and two-standard124
deviation range of expected upper limits for various potential experimental outcomes. The125
observed limits are well within the expected range assuming no signal. The observed and126
expected upper limits are shown in Table 2.127
!"#$%&$'()*+,-.-+/00$%+"1/2'#
344
344
34
3544 644 )44
78+++9:$;<!5=
900
>=?9
=++90"=
@44
,AB+C%$DE7E2F%G6H+0"I3+++J+K$;
A$'EF2+$L0$MN$'3 +$L0$MN$'+%F2O$5 +$L0$MN$'+%F2O$
Figure 2: The expected one- and two-standard-deviation ranges (blue bands) and observed
(red line) 95% C.L. upper limits on σφ · Bττ as a function of mA.
We can interpret the upper limits on σφ · Bττ in the MSSM parameter space of tan β versus mA128
for an example scenario. We use here the mmax
h[23] benchmark scenario in which MSUSY = 1129
TeV/c2; XPQt = 2MSUSY; µ = 200 GeV/c
2; Mg̃ = 800 GeV/c
2; M2 = 200 GeV/c
2; and Ab = At,130
where MSUSY denotes the common soft-SUSY-breaking squark mass of the third generation;131
Xt = Atµ/ tan β the stop mixing parameter; At and Ab the stop and sbottom trilinear couplings,132
respectively; µ the Higgsino mass parameter; Mg̃ the gluino mass; and M2 the SU(2)-gaugino133
mass parameter. The value of M1 is fixed via the GUT relation M1 = (5/3)M2 sin θw/ cos θw.134
HIG-10-002
Interpretation in tanβ 7
!"#$%&'()*)+,&-$$$./$0123$$$4$5'6
7
87
97
/7
:,+
37
.7
;7
"##"$*<$$$$=>'+,&)?@$"#A#B$C$3$5'6D;E$!FGF$'H>(IJ'J$&'K)?+=
377 877 .77*L$$$MN'6O!8P
3;7 8;7
*,H
$Q3 $:<'?&-$!"#$'H>(IJ'J
5'R,:&?+$'H>(IJ'JGS%$'H>(IJ'J$!"#$'H0'>:'J
Figure 3: Region in the parameter space of tan β versus mA excluded at 95% C.L. in the context
of the MSSM mmaxh scenario, with the effect of ±1σ theoretical uncertainties shown. The other
shaded regions show the 95% C.L. excluded regions from the LEP and Tevatron experiments.
[4] G. Guralnik, C. Hagen, and T. Kibble Phys. Rev. Lett. 13 (1964) 585.156
[5] P. W. Higgs Phys. Rev. 145 (1966) 1156.157
[6] E. Witten Phys. Lett. B 105 (1981) 267.158
[7] S. P. Martin, “A Supersymmetry Primer”, arXiv:hep-ph/9709356 (1997). and references159
therein.160
[8] CDF and D0 Collaboration arXiv:hep-ex/1003.3363 (2010).161
[9] LEP Higgs Working Group Collaboration Eur. Phys. J. C47 (2006) 547–587.162
[10] CMS Collaboration, “The CMS experiment at the CERN LHC”, J. Instrum. 0803:S08004163
(2008).164
[11] CMS Collaboration, “Electron reconstruction and identification at sqrt(s) = 7 TeV”, CMS165
Physics Analysis Summary EGM-10-004 (2010).166
[12] CMS Collaboration, “Performance of muon identification in pp collisions at√
s = 7 TeV”,167
CMS Physics Analysis Summary MUO-10-002 (2010).168
[13] CMS Collaboration, “Particle-Flow Event Reconstruction in CMS and Performance for169
Jets, Taus, and Emiss”, CMS Physics Analysis Summary PFT-09-001 (2009).170
[14] CMS Collaboration, “Commissioning of the Particle-Flow Reconstruction in171
Minimum-Bias and Jet Events from pp Collisions at 7 TeV”, CMS Physics Analysis172
Summary PFT-10-002 (2010).173
HIG-10-002
Summary• Large improvements in τ-ID since PTDR
• Tau fake rates & efficiency measured in real data
• Z→ττ cross section measured withhigh precision
• Taus well understood at CMS
• SVfit method improves Mττ resolution
• CMS sets new limits on MSSM using taus
backup
Particle Flow AlgorithmCMS Preliminary
4 2 Commissioning of the link algorithm
(a) (b)
Figure 3: Charged-hadron tracks (lines with squares, representing the hits measured in the
tracker and the various extrapolation positions to the ECAL and HCAL) each linked to (a) one
or two ECAL clusters and (b) an HCAL cluster (dots). Each square represents a calorimeter
cell. The grey area is proportional to the logarithm of the energy measured in each cell. The
clusters represented by a star are linked to neither of the two tracks, and are therefore photon
candidates.
(a) (b)
Figure 4: Track-cluster link distance in (a) the ECAL and (b) the HCAL, for tracks with pT larger
than 1 GeV/c, in the data (dots with error bars) and in the simulation (histogram). The typical
cell size is 0.02 in the ECAL and 0.1 in the HCAL.
ECAL Entrance
ECAL Entrance
HCAL Entrance
HCAL Entrance
cluster linked to trackunlinked clustertracker hit
see CMS PAS PFT-10-002
Particle Flow Performance
invariant mass of PF photon pairs
2 2 Calorimeter response to photons and charged hadrons
The photon-pair invariant-mass distribution is shown in Fig. 1 along with a fit by a Gaussian
for the signal, added to an ad hoc function for the background. From this fit, an average re-
constructed mass of 135.2 ± 0.1 MeV/c2and a resolution of 13.2 ± 0.1 MeV/c2
are obtained, to
be compared with the prediction from the Geant-based simulation of 136.9 ± 0.2 MeV/c2for
the mass and 12.8 ± 0.2 MeV/c2for the resolution. The agreement with the world average π0
mass of 135 MeV/c2[8] is better than 1%, and the agreement between data and simulation is
at the same level. This agreement validates the photon energy scale used in the particle-flow
reconstruction algorithm.
)2Mass (GeV/c0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5
Num
ber o
f pho
ton
pairs
0
5000
10000
15000
20000
)2Mass (GeV/c0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5
Num
ber o
f pho
ton
pairs
0
5000
10000
15000
20000
CMS Preliminary 2010
2 0.1 MeV/ c± = 135.2 fit0!m
2 0.1 MeV/ c± = 13.2 0!m"
-17-TeV Data, 0.1 nb
(a)
)2Mass (GeV/c0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5
Num
ber o
f pho
ton
pairs
0
500
1000
1500
2000
)2Mass (GeV/c0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5
Num
ber o
f pho
ton
pairs
0
500
1000
1500
2000
CMS Preliminary 2010
2 0.2 MeV/ c± = 136.9 fit0!m
2 0.2 MeV/ c± = 12.8 0!m"
Simulation
(b)
Figure 1: Photon-pair invariant-mass distribution in the barrel (|η| < 1.0) for the data (a) and
the simulation (b).
2.2 Calorimeter response to hadrons
A charged or neutral hadron can deposit energy in the electromagnetic calorimeter and in the
hadron calorimeter. The hadron energy E is obtained with a simple linear calibration of the
resulting EECAL and EHCAL cluster energies [2]. This calibration is essential in the reconstruc-
tion of neutral hadrons, but also in the detection of neutral particles overlapping with charged
hadrons. The calibration is assumed to be identical for charged and neutral hadrons, and has so
far been obtained from single hadrons produced with the fast simulation of the CMS detector.
To verify the calibration procedure, a clean selection of charged hadrons was made in which
the charged-hadron candidate was required to have a track with pT > 1 GeV/c, p > 3 GeV/cand at least 15 hits, of which at least two in the pixel layers. The requirement on the number of
hits was tightened to up to 21 hits when the track points to the end-cap regions, which feature
more tracker layers. These stringent criteria are meant to select particles having high-quality
tracks with a robust momentum measurement and that reach the calorimeter without experi-
encing nuclear interactions with the tracker material. The hadron identification was ensured by
requiring the track to be linked to a cluster in the hadron calorimeter with EHCAL > 1 GeV. An
isolation requirement was applied by requesting that no other tracks be linked to this cluster,
which is loose enough to allow for a very large sample of tracks to be extracted.
Figures 2a and 2b display the average calibrated calorimeter response in the barrel (here de-
fined as |η| < 1.4) and in the end-caps (1.4 < |η| < 2.4) for the selected charged hadrons in
the data, with a comparison to the raw calorimeter response, as a function of the track mo-
mentum. The slope of the cluster calibration curve is close to unity up to the largest energies
available so far. Small deviations from unity at low momentum, however, can be observed in
7 TeV Data, 0.1 nb-1
Et-60 -50 -40 -30 -20 -10 0 10 20 30 40
#
0
50
100
150
200
250
300
350
400
450
Particle Flow Jets
Calo Tower Jets
Jet Transverse Energy Resolution
50 GeV Et tau
CMS Preliminary
Particle Flow
Tau ET resolution Mass of photon pair [GeV/c2]
SIM
Shrinking Cone Algorithmreduce QCD by applying isolation requirement
require a leading candidate with pT > 5 within ΔR < 0.1 of jet axis
signal objects are those with ΔR < ΔRsig of the lead candidate
isolation objects are those in the region ΔRsig < ΔR < 0.5
about the lead candidate
∆R =�
∆φ2 + ∆η2
∆Rsig = 5.0/EjetT
Zττ selections
Trigger
Events triggered by single Electron/Muon Triggers
PT thresholds 9-15 GeV, depending on instantaneous Luminosity
Lepton Selection
Electrons Muons had. ! Decays
PT > 15 GeV PT > 15 GeV PT > 20 GeV
|!| < 2.4 |!| < 2.1 |!| < 2.4
isolated isolated “loose” Tau id.
Veto against e/µ
Opposite Charge Lepton Pair
Transverse Mass
e + !had, µ + !had: MT(l + MET) < 40 GeV
e + µ: MT(e + MET ) < 50 GeV && MT(µ + MET) < 50 GeV
Veto Events with additional isolated Leptons
For µ + !had, e + !had and e + µ Channels, µ + µ Channel different (Backup)
Christian Veelken Higgs and Z ! !+!- in CMS 5
Event Selection
Zττ yields
CMS Data, 36 pb-1 @ 7 TeV
Background Estimates quoted in Table obtained from Data-driven Methods
> 600 Z ! !+!- Signal Events selected in CMS Data
Christian Veelken Higgs and Z ! !+!- in CMS 7
Event Yields
Z recoil correctionbefore correction after correction
MET resolution better in Monte Carlo than data
Project MET in directions parallel and perpendicular to Z and parametrize as function of Z pT
Zμμ events Zμμ events
sub title
“full” !+!- Mass visible Mass
34
Observed vs. expected Limits by Channel
control plotsHiggs Search Lepton PT and !: µ + !had Channel
Christian Veelken Higgs and Z ! !+!- in CMS 26
control plotsHiggs Search Lepton PT and !: e + !had Channel
Christian Veelken Higgs and Z ! !+!- in CMS 27
Largest Uncertainty: hadronic Tau Identification Efficiency
!!!"had Identification Efficiency constrained by Ratio of Event Yields
in semi-leptonic/leptonic Channels
!! Determine Z " "+"- Cross-section by simultaneous Fit of all four Channels
Christian Veelken Higgs and Z " "+"- in CMS 25
Z ! !+!- Systematic Uncertainties
Christian Veelken Higgs and Z ! !+!- in CMS 28
Christian Veelken Higgs and Z ! !+!- in CMS 29
Christian Veelken Higgs and Z ! !+!- in CMS 30