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Physics with CMS Hadron Calorimeter

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Dh(qq) 4.4. M(qq) 1TeV. mini jet veto. MET 100GeV. Only forward jets are. positive signal! ... during construction. all tiles. B) Moving radio active source: ... – PowerPoint PPT presentation

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Title: Physics with CMS Hadron Calorimeter


1
Physics with CMS Hadron Calorimeter
  • Shuichi Kunori
  • U. of Maryland
  • 24-Nov-2000
  • .
  • Jet,MET,tau
  • Some physics channels
  • Calibration

2
Pion Response Linearlity
ECAHLHCAL Non compensating calorimeter
CMS Simulation
96H2 Teast Beam Data
ET3 GeV pion in 0lthlt5
EEC a x H1 H2 HO
3.0 GeV
1.0
0.9
1.5 GeV
0.8
3
0
5
h
0
200
400GeV
P
3
Jet Response and Correction( CMSIM/ORCA)
Et-eta dependent correction for QCD jets
Et(corr)a b x ET(rec) c x ET(rec)2
No-pileup
gt Different corrections for L1 jets, tau-jets
and b-jets gt Luminosity dependent.
4
Correction and Pileup Energy_at_ 10E34
lt17.3gt in-time min-bias events
Resolution after corrections is worse because
pileup fluctuations are not removed by the
average correction.
Event-by-event correction e.g. algorithm
developed for heavy ion collision. (I.Vardanian)
5
Low Et Jets and Pile-up
Reco with pile-up
Reco w/o pile-up
Generated
(Rlt0.7)
Fake jets lt 40GeV
gt core of jets gt smaller cone
(A.Krokhotine)
6
Seed Cut
No cut
2 GeV / (0.087x0.087)
Et(reco)
gt 10 GeV
gt 20 GeV
gt 30GeV
Suppression of fake jets! but still many
fakes remaining.
7
Low ET Jets and Threshold
35ltET(gen)lt45geV
ET(quark)20GeV
0.5GeV
1.0GeV
(A.Krokhotine)
(I.Vardanian)
Lower threshold is better!
Electronics noise and occupancy define the
threshold. gtgt aim at 0.5GeV/tower _at_ 10E34
8
MET Response
(H-gtbb)
(0.5GeV Thrshold)
9
MET for Signal Events with Pile-up and Tower
Threshold
With 17.3 min-bias events
No min-bias
GeV
Tower EcalHcal
gtgt Not much pile-up effect with this
resolution! gtgt Resolution gets worse as threshold
increase.
10
MET Resolution
QCD Jets with no neutrino/muon
(no pile-up)
Ex S (Ex-tower) Ey S (Ey-tower)
Any way to improve this?
e.g. ExExS ( D(Ex-jet)) EyEyS ( D(Ey-jet))
Does this work?
11
Attempt to improve L1 METwith Jet Correction
(S.Abdoulline)
12
L1 Trigger- Jets/Tau
13
L1 Jet Trigger
(P.Chumney)
14
Sample L1 Rates and Cutoffs_at_10E33
15
Sample L1 Rates and Cutoff_at_ 10E34
16
Single Top -gt Wb -gt lnb
CMS Note 1999/048
Measurement of - Vtb - properties and
decays of top - background process to new
physics
Event Selection only one charged lepton
PT gt 20GeV in hlt2.5 only one cnetral
jet ET gt 20GeV in hlt2.5
(jet veto against tt) b-tagged
(20ltETlt100GeV) forward tagging jet
ETgt50GeV in 2.5lthlt4.0 MET gt
20GeV W Mass (lepton MET)
50ltMTlt100GeV Di-jet mass outside M(Z0)
top mass cut 140ltM(Wb)lt180GeV
250pb
10pb
50pb
Background toptop 800pb W2jets
W3jets
17
Single Top - Kinematics

ET (b-quark) h
PT (lepton) h
lt2.5
20-100
lt2.5
gt20GeV
0
200
0
200
-4
4
-2
2
ET (tagging jet) h
MT (ln)
MET
2.5-4.0
gt50GeV
50-100
gt20GeV
0
200
-4
4
0
0
200
200
18
Top Mass
b/c tagging efficiency and fake
. - very old
parametrization used in this analysis-
M(Wb)

20-100GeV
S / N 3.5 / 1.0 66 signal events / 100pb 30
housrs _at_ 10E33. Efficiency 1.2

Charm rate and fake rate play important role in
background rejection.
19
H(170) -gt WW -gt lnln
(CMS Note 1998/089)
1.24pb
Event Selection (total 11 cuts)
two opposite sign leptos - PT cuts
(20GeV,10GeV) - angle between two
leptons jet veto - ETgt20GeV in
hlt2.4 removed Mass (WW) - M gt
140GeV
Results - number of events (5fb-1) H
/ tt / WW 54 / 35 / 28 - good channel for
discovery - background need good
understanding - jet veto
important.
Background tt -gt (Wb)(Wb) -gt(lnb)(lnb)
62.5pb WW(continum) -gt lnln 7.4pb
20
ttH(110) -gt (lnb) (jjb) (bb)
primary selection 4 b-tags M(bb)
lepton
M(bb)
Jet energy correction without 19
with 14
(V.Drollinger S.Arcelli)
21
Higgs Couplings
22
qqH(135), H -gt 2t -gt ej
(A.Nikitenko)
Cuts Et(e) gt 15GeV, h(e)lt2.4 Et(t) gt
30GeV, h(t)lt2.4 Et(q) gt 40GeV, h(q)lt5.0
Dh(q1q2)gt4.4, M(q1q2) gt1TeV mini-jet
veto . Result H / Zjj(QCD)/ Zjj(EW
)/ Wjjj 6.7-0.3 / 0.63 / 0.74
/ 0.14 for 30fb-1 (generated
by S.Illyin, comphep)
HF acceptance for tagging jets ( 0 / 1 / 2 )
jets (47,46, 7) --gt need both HE and HF
23
qqH(135) Mass Resolution
Need to improve mass with MET!
24
H -gt invisible
Black Hole _at_ low luminosity
CMS has studied H(500) -gt tt -gt jj, ej
H(200) -gt tt -gt jj, ej qqH(135) -gt tt -gt
ej and look promising _at_ 1034 More challenging
channel is qqH(120-400) -gt invisible
ET(q) gt 40GeV, h(q)lt5.0 Dh(qq) gt4.4
M(qq)gt1TeV mini jet veto
METgt100GeV Only forward jets are
positive signal!
Need high luminosity to close the hole (with
Higgs channels shown on right).
(O.J.Eboil and D.Zeppenfeld, MADPH-00-1191)
25
Optimization of HF Fiber Spacing
Simulation done with test beam data and
PYTHIA for two longitudinal segmentaion.
5mm spacing was chosen.
(V.Kolosov)
26
HCAL Calibration Tools(light -gt ADC -gt
Jets/MET/tau)
E) Test beam - normalization between GeV vs. ADC
vs. A,B,C,D - ratios elec/pion, muon/pion -
before assembly a few wedges F) Physics events
(in-situ) - mip signal, link to HO muon - calo
energy scale (e/pi) charged hadron - physics
energy scale photonjet balancing Zjet
balancing di-jets balancing di-jet mass W-gtjj in
top decay gtgt non-linear response gtgt pile-up
effect
A) Megatile scanner - Co60 gamma source - each
tile light yield - during construction all
tiles B) Moving radio active source - Co60 gamma
source - full chain gain - during CMS-open
(manual) all tiles - during off beam time
(remote) tiles in layer 0 9 C) UV Laser - full
chain timing, gain-change - during off beam
time tiles in layer 0 9 all RBX D) Blue LED -
timing, gain change - during the off beam
time all RBX
27
One Scenario (HB/HE)
(same to HF)
1) Before megatile insertion - megatile scanner
all tiles - moving wire source all
tiles . 2.1) After megatile insertion - moving
wire source all tiles / 2 layer - UV laser
2 layers/wedge .
2.2) After megatile insertion - test beam
a few wedges. . 3) Before closing
the CMS - moving wire source all tiles - UV
laser blue LED all RBX (do 3, about
once/year) . 4) Beam off times - moving
wire source 2layer/wedge - UV laser
2 laer/wedge - UV laser blue
LED all RBX . 5) Beam on (in situ) - jets
/ tau / MET ECALHCAL
Absolute calib. Accuracy of 2 for single particle
Monitor for change with time Accuracy lt 1
once/month
a few times/day (?)
28
In Situ Calibration(Physics Event Trigger)
A) Min-bias events trigger - estimation of
pile-up energy. - normalization within each
eta-ring. - isolated low ET charged tracks B)
QCD Jet trigger (pre-scaled) - normalization
within each eta-ring - normalization at the
HB-HE-HF boundary - test on uniformity over full
h range. - dijet balancing to normalize ET scale
in h rings. C) tau trigger - isolated high Et
charged tracks (Etgt30GeV) D) muon trigger
(isolated) - good for monitoring. - probably too
small energy deposit for calibration.
2 accuracy with 1k events in HF
29
In Situ Calibration (2)
E) 1 photon 1 jet - ET Scale over full h
range by photon-jet balancing Note - depend
on ECAL Et scale - sensitive to ISR ( FSR) F) Z
(-gt ee, mm ) 1 jet - ET Scale over full h
range by Z-jet balancing Note - depend on
Tracker and/or ECAL - sensitive to ISR ( FSR)
30
Photon-Jet balancingfor HF Jets
(tagging jets)
E.Dorshkevich,V.Gavrilov CMS Note 1999/038
Using Et( g ) gt 40GeV, h (g ) lt 2.4 - minimize
MET with 4000 g Et(calib) C(S)(h)
Et(Short) C(L)(h)
Et(Long) - 2.3 days at 10E33 with 1 efficiency
before
after
Accuracy lt 1-5 for Etgt40GeV
31
Z (ee,mm) - jet balancing
ET
CDF Data (100pb-1) energy scale accuracy to
5 for Etgt30GeV
Jets
50
CMS 700k events/month at 10E33 h
(lep.)lt2.6 ET(jet)gt40GeV
Z0
0
0
50
100 GeV
Freeman Wu (Fermilab-TM-1984)
32
In Situ Calibration (3)
F) Top trigger (1 lepton jets 2 b-tags) - ET
scale by Mass(jj) for W in Top decay.
Parameterized simulation
Peak 69.6 GeV sigma 7.2 GeV
Mass(jj) Rlt0.4
45000 events / month at 10E33 with double
b-tagging.
Not depend on ISR!
0
100
Freeman Wu (Fermilab-TM-1984)
33
Summary (1)
  • Energy Resolution and Scale
  • Simple Jet energy correction is working in MC
    world.
  • Need to extend it to MET and tau.
  • We have been using very simple weighting method
    to sum energies in ECAL and HCAL.
  • look for better method(s), e.g. energy depend
    weights, use of fine segments in ECAL, use of
    Tracker, etc.
  • In-situ calibration will provide absolute scale.
  • Need plan to cover energy calibration up to the
    highest energy.
  • High Luminosity
  • Low ET jets/MET (lt100GeV) at high luminosity is
    very challenging for both trigger and offline
    analyses.
  • Need good algorithms to remove fake jets and to
    subtract pile-up energy.

34
Summary (2)
  • Physics with HCAL
  • Much of physics analyses depend on jets, MET and
    tau.
  • Forward tagging jet become more and more
    important, e.g. studies on property of Higgs.
  • Calibration and Monitoring
  • Need to develop complete scenario.
  • All the tools should be ready on day-1 of data
    taking and calibration has to be done in 1-3
    months for quick publication of physics results.
  • JetMET Physics Group (S.Eno)
  • http//home.fnal.gov/sceno.main.html
  • The group is expanding. -- Need better
    communication.
  • Web, VRVS, local coordination.
  • Next milestone May 2001- HLT in DAQ TDR.
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