PHYSICS WITH LHC EARLY DATA
ONE OF THE LAST „PROPHETIC” TALKS ON THIS SUBJECT – HOPEFULLY
We may have some two month of the Machine operation in 2008
LONG HISTORY ...
I will extensively use:
Fabiola GIANOTTI – CERN, ATLAS 2004
Wouter VERKERKE – NIKHEF, AOW Paris 2005
Fabiola GIANOTTI – CERN, ATLAS 2007
http://www.njp.org/
10.1088/13672630/9/9/332
Fabrice HUBAUT CPPM/IN2P3, ATLAS & CMS I lepsza referencja
Pamela FERRARI ATLAS & CMS asXiv hepex 0705.3021v2
Albrert De ROECK – CERN, KITF Seminar, 1 Apr 2008
Anna KACZMARSKA – IFJ PAN – Institute Seminar 16 Feb 2008
What energy at the start ?
900 GeV
10 TeV
12 TeV
14 TeV
LHC machine status and schedule
A rather extensive meeting took place on 3
rdMarch between the DG R Aymar, J Engelen
and ATLAS represented by M Nessi and PJ
During this meeting we were informed about the machine status, we had a chance to
explain our schedule, and to give input to the LHC start-up strategy discussions
The main conclusions, which are still valid, were:
- The current planning of the LHC is such that the machine is expected to be cold by
by mid-June, and first injections could start soon after, from end June onwards
- CERN Management will give ATLAS a warning signal 2 months before we have to start
closing, currently expected by mid-April (around RRB) when the progress on the machine
will be known from the cooldown status of further sectors
- Experience from power tests in Sector 4-5 showed that several magnets need training,
starting somewhere above 5 TeV equivalent
- The first physics run (typically 2 months) in 2008 will be at 10 TeV (or slightly above), the
energy will be defined in April when experience from Sector 5-6 will also be available
Similar statements were also made during this Council Week, in addition it was said that
One can follow cooling states of sectors almost on line ...
Some LHC parameters
COLLISION ENERGY
7
TeV
INJECTION ENERGY
450 GeV
PROTONS PER BUNCH
1.1
1011
NUMBER OF BUNCHES
2808
NOMINAL BUNCH SPACING
25
ns
NOMINAL LUMINOSITY
10
34 cm
-2s
-1REVOLUTION TIME
88924
µs
(REVOLUTION FREQUENCY
11.2455 kHz) *
STORED BEAM ENERGY
336 MJ
BUNCH LENGTH
75.5 mm
LUMINOSITY LIFETIME
10 h
ACCELERATION TIME
20
min
WHAT IS THIS ALL FOR ?
Flagships:
Higgs searches
physics beyond the SM
supersymmetry
extra dimensions
precision physics (W, top, Higgs mass, ....)
bphysics
quarkgluon plasma
BUT – it is NOT the first day physics
. These goals and unprecedented complexity
of detectors (ATLAS and CMS) require first:
commissioning of detectors and triggers, first calibrations and alignment with
minimum bias and QCD jet production,
measure of some exclusive channels (e.g. Z > lepton lepton) to set the absolute
electron and mion ECAL energy scale
measure tt events to determine the absolute jet energy scale and understand
btagging in the inner detectors
Recently, prof. Peter W. Higgs has visited
the ATLAS detector.
Some say, that it is going to be the only
Higgs seen in ATLAS
Muon system:
(precision
chambers + triggers in air
core toroids B=4T mean
value) ,
σ
/pT ~ 7 % at 1 TeV
standalone
(e.g. H,A
µµ, H
4µ
)
Hadronic Calorimeters: (Fe scint
Cu-liquid argon)
σ
/E ~ 50%/
√
E
⊕
0.03
Jet, E
Tmissperformance
(e.g.
H
→τ τ
, H
→
bb)
Inner Detector:
(Silicon
pixels + strips
+TRT
particle ID (e/
π
) )
B=2T ,
σ
/p
T~ 4x10-4 p
T⊕
0.01
(e.g. H
→
bb)
Electromagnetic calorimeter : (Pb, liquid argon)
σ /E ~ 10%/√E , Uniform longitudinal segmentation
Provides: e/γ identification, energy and angular resolution, γ/jet , γ /π0 separation (e.g. H→γγ)
ATLAS
Length ~45m weight ~7000 t
H
e
ig
ht
~
2
2
m
„business plan”
A solid candidate
for the very early
valuable result:
it is enough to collect
10 000 events to
Considerable statistics
„easily
vailable”
to study and estimate
absolute scales
for
electron and mion
ECAL measurements
as well as for the
absolute jet energy
10 pb
-1 ATLAS preliminary1 pb
-1 ATLAS preliminaryJ/
ψ → µ µ
Y
→ µ µ
→
alignment of mion spectrometer,
momenta calibrations for the ID and mion
After all cuts:
~ 160 Z
→
µ µ
ev./day at L = 10
31(assume 30% data taking efficiency)
First picks: rediscovery of the „known physics” to demostrate the detector
understanding
After all cuts:
~ 4200 (800) J/
ψ
(Y)
→
µ µ
ev./day, L = 10
31LHC
~850 pb
σ
10% qq, 90% gg
Tevatron
~7 pb
σ
85% qq, 15% gg
Top production and decay at LHC
FASCINATING ROLE OF ttbar EVENTS : ONE GETS TO INTERESTING PHYSICS
SIMULTANEOUSLY CALIBRATING MANY HIGHER LEVEL RECONSTRUCTION
CONCEPTS SUCH AS JET ENERGY SCALES, BTAGGING AND MISSING ENERGY
I have learned that from Wouter Verkerke at Paris AOW in 2005 !
σ
tt(
tot
)
=
759±100 pb
N
evt~ 700/hour
3 2 1 2 1;
~
10
ˆ
=
sx
x
x
x
−s
gg
tt
tt
Top physics at LHC
Large ttbar production cross section at LHC
Production:
gluon
dominated at LHC,
quark
dominated at Tevatron
Top topology
Decay products are 2 W bosons
and two b quarks.
About 99.9% decays to Wb
For commissioning studies consider events
with one hadronic and one semi-leptonic
W decay (about 30% of the total ttbar cross
What can we learn from ttbar production?
–
Abundant clean source of b jets
●2 out of 4 jets in event are b jets
O(50%) a priori purity
(need to be careful with ISR
and jet reconstruction)
●Remaining 2 jets can be kinematically
identified (should form W mass) >
possibility for further purification
What can we learn from ttbar production?
–
Abundant source of W decays into light jets
●Invariant mass of jets should add
up to well known W mass
●Suitable for light jet energy scale
calibration (target prec. 1%)
–Caveat: should not use W mass in jet
assignment for calibration purpose
to avoid bias
●If (limited) btagging is available,
W jet assignment combinatorics
greatly reduced
What can we learn from ttbar production?
–
Known amount of missing energy
●4momentum of single neutrino in each
event can be constrained from event
kinematics
–
Inputs in calculation: m(top) from Tevatron,
bjet energy scale and lepton energy scale
How to identify ttbar events?
4 hard jets
(P
T>40 GeV)
1 hard lepton
(Pt >20 GeV)
Missing E
T(E
T>20 GeV)
●Restrict ourselves to basic (robust) quantities
–
Apply some simple cuts
–
Hard pT cuts really clean up
sample (ISR).
–
Possible because
of high production rate
Combined efficiency of requirements
is ~5% still have ~10 evts/hour
→
TOP CANDIDAT E
W CANDIDATE
m(top
had)
m(W
had)
Signalonly distributions (Full Simulation)
•
Clear top, W mass peaks visible
●Background due to misassignment of jets
– Easier to get top assignment right than to get W assignment right ●Masses shifted somewhat low
– Effect of (imperfect) energy calibrationL=300 pb
-1 (~1 week of running)S
mtop = 162.7±0.8 GeV MW = 78.1±0.8 GeV
Jet energy scale
calibration
possible from
shift in m(W)
S/B = 1.20
m(top
had)
m(W
had)
Signal + Wjets background (Full Simulation)
S/B = 0.45L=300 pb
-1 (~1 week of running) S/B = 0.27Jet energy scale calibration possible from shift in m(W) ●
Plots now include W+jets background
–
Background level roughly triples
–Signal still well visible
–Caveat: bkg. cross section quite uncertain
TOP CANDIDAT E W CANDIDATEL=300 pb
-1 (~1 week of running) TOP CANDIDAT E W CANDIDATEm(top
had)
m(Whad)m(top
had)
S/B = 0.45 S/B = 1.77 ●Now also exploit correlation between
m(top
had) and m(W
had)
–
Show m(top
had) only for events
with |m(jj)m(W)|<10 GeV
m(top
had)
m(top
had)
S/B = 0.45 S/B = 1.11L=300 pb
-1 (~1 week of running)|m(jl
ν
)-m
t|<30 GeV
•
Can also clean up sample by with
requirement on
m(jlν)
[semileptonic top]
– NB: There are two m(top) solutions for each candidate due to ambiguity in reconstruction of pZ of neutrino ●Also clean signal quite a bit
– m(W) cut not applied hereSignal + Wjets background (Full Simulation)
TOP CANDIDAT E W CANDIDATE W+jets (background) ‘random jet’, no b enhancement expected ttbar (signal) ‘always b jet if all jet assignment are OK’ b enrichment expected and observed
AOD b-jet probability
AOD b-jet probability
Clear
enhancement
observed!
Exploiting ttbar as bjet sample (Full Simulation)
●Simple demonstration use of ttbar sample to
provide b enriched jet sample
–
Cut on
m(W
had)
and m(top
had) masses
–
Look at bjet prob for
4
thjet
(must be bjet if
If we are lucky we may have
some interesting use of the LHC
machine already by this winter.
Any way, come to
Kraków EPS Conference
next year