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23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 11
ALICEALICE
A Large Ion Collider A Large Ion Collider ExperimentExperiment
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 22
ALICEALICE
The club of those who smash atomic nuclei The club of those who smash atomic nuclei against each other…against each other…• Why ?Why ? Attempt to dissolve the vacuum and rewind the Attempt to dissolve the vacuum and rewind the
timetime• How ?How ? Heat and compress matter Heat and compress matter• Observe a phenomenon which: Observe a phenomenon which:
Lasts in a second as much as a lightening in the 15 billions Lasts in a second as much as a lightening in the 15 billions years elapsed since the birth of the universe, years elapsed since the birth of the universe,
Creates a temperature equal to 100,000 times the Creates a temperature equal to 100,000 times the temperature in the heart of the sun andtemperature in the heart of the sun and
Compresses matter to densities such as all matter Compresses matter to densities such as all matter contained in the Kheops pyramid would fill a volume of the contained in the Kheops pyramid would fill a volume of the size of a pinhead. size of a pinhead.
Recreate “color”
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 33
In the heart of matterIn the heart of matter
Matter is built up from “elementary” particles, the mass is Matter is built up from “elementary” particles, the mass is concentrated inside the atomic nucleus.concentrated inside the atomic nucleus.
Stable matter in the universe is made of 4 elementary Stable matter in the universe is made of 4 elementary particles.particles.
O(10-10 m) O(10-15 m) < O(10-19 m)
QUARKS LEPTONS
é
é
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 44
The Standart ModelThe Standart Model
• The theory which explains the bricks of the universe and the forces through which they interact:
12 elementayconstituents
4 interactions
graviton photon W, Z gluon
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 55
Open questionsOpen questions
How did particles acquire mass ? How did particles acquire mass ? mm,g,g=0, m=0, mtt = 340.000 m = 340.000 me e !!
Does there exist an universal force from Does there exist an universal force from which all other forces derive ?which all other forces derive ?
Why does there exist 3 families of particles ?Why does there exist 3 families of particles ? What happened to anti matter ?What happened to anti matter ? Why is the stable universe colorless ?Why is the stable universe colorless ? What is the structure of the vacuum ?What is the structure of the vacuum ? What was the form of primordial matter ?What was the form of primordial matter ? Where does the mass of composite particles Where does the mass of composite particles
come from ?come from ?
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 66
Quantum Chromodynamics : the theory Quantum Chromodynamics : the theory of the strong interactionof the strong interaction
A formal theory:A formal theory:• Quarks carry a charge called Quarks carry a charge called ccoolloorr; there are 3 colors ; there are 3 colors RR, , BB, , GG
• Quarks interact by exchanging a gluon (mQuarks interact by exchanging a gluon (mgg=0) which carries a =0) which carries a color charge and its anti-charge !color charge and its anti-charge !
• The strong interaction is strong at large distance and weak at The strong interaction is strong at large distance and weak at small distance !small distance !
• The vacuum is filled with virtual quarks and anti-quarks pairsThe vacuum is filled with virtual quarks and anti-quarks pairs
• Observables can be calculated only when the interaction is weak !Observables can be calculated only when the interaction is weak !
MFFDiL aa
ˆ~
4
1
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 77
Quantum Chromodynamics : the theory Quantum Chromodynamics : the theory of the strong interactionof the strong interaction
Empirical adds on:Empirical adds on:
• Quarks (valence) are bound inside Quarks (valence) are bound inside hadrons (baryons and mesons) such as to hadrons (baryons and mesons) such as to form colorless objectsform colorless objects
• Interactions of valence quarks with the Interactions of valence quarks with the vacuum contribute to the mass of vacuum contribute to the mass of hadronshadrons
• It is not possible to isolate a color chargeIt is not possible to isolate a color charge
q q
F=kR1
q q
F=kR2
q q
F=kr2
F=kr1
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 88
Big Bang …Big Bang …Until 10-6 secondsafter the birth of the Universe, matter is colored: quarks and gluons move freely.
As soon as the universe has cooled down to about 1012 K, matter becomes colorless: quarks and gluons are locked forever in particles out of which only protons and neutrons have survived.
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 99
Let’s go backwardsLet’s go backwards
Why ?Why ? • Observe the strong interaction in actionObserve the strong interaction in action
How do elementary particles interactHow do elementary particles interact How did the interaction give rise to the How did the interaction give rise to the
composite particles which constitute the composite particles which constitute the universeuniverse
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1010
Let’s go backwardsLet’s go backwards How ?How ?
• Heating the vacuum to create high energy densities over Heating the vacuum to create high energy densities over a mesoscopic volumea mesoscopic volume
• Collisions between heavy ions accelerated at the speed Collisions between heavy ions accelerated at the speed of light provide the necessary “calories” of light provide the necessary “calories”
Compression Chaleur Plasma de quarks et gluons
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1111
Laboratory
2. The energy of collision is materialized into quarks and gluons
1. Accelerated ions will collide head on
The mini Big BangThe mini Big Bang
3. Quarks and gluons interact via the strong interaction: matter equilibrates
v/c = 0,99999993Lorentz Contraction: 7 fm 0,003 fm
t~10-24 sT~5×1012 K
4. The system expands and cools down
5. Quarks and gluons condensate into hadrons
t~10-23 sT~1012 K
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1212
Mini Big Bang : the movieMini Big Bang : the movie
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1313
Accelerating nucleiAccelerating nuclei Nuclei (atomes stripped off Nuclei (atomes stripped off
electrons) are accelerated by electrons) are accelerated by an electric fieldan electric field
The trajectory of nuclei are The trajectory of nuclei are bent by dipolar magnetic bent by dipolar magnetic fieldsfields
The flux of nuclei are focalised The flux of nuclei are focalised by quadrupol magnetic fieldsby quadrupol magnetic fields
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1414
LHC: world championLHC: world champion• 27 km circumference• 40 m underground• Cryogeny at 1.9 K
×10
12 Accelerates p @ 7×10Accelerates p @ 7×101212 eV & ions @ 2,76×10 eV & ions @ 2,76×101212 eV (99.999993% c) eV (99.999993% c) A collision generates up to 0,2×10A collision generates up to 0,2×10-3-3 Joules, T=1,000×10 Joules, T=1,000×1099 K K ~10~1088 ions cross 10 ions cross 1088 ions 10 ions 1066 times every second times every second Only 8.000 collisions every second, out of which 1% produce Only 8.000 collisions every second, out of which 1% produce
”extraordinary” events ”extraordinary” events
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1515
Thermodynamics : water, a known Thermodynamics : water, a known casecase
• Phase diagram; Equation of state (PV/T = Cte)• Phases and Phase transitions• Ordre of the transition and critical point
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1616
Thermodynamics of matter Thermodynamics of matter
We are here
The Big Bang started here
Pb collisions at LHC will take us there
And we will study this trajectory
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1717
QCD tells us…QCD tells us…
MFFDiL aa
ˆ~
4
1
Tc 173 MeV, mq0, Nf=2,3 Order of the transition : cross over c 0.3-1.3 GeV/fm3
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1818
Observing the phenomenonObserving the phenomenon Imagine…Imagine…
• You lived in a frozen world where water existed only as ice• and ice comes in only quantized sizes ~ ice cubes• and theoretical friends tell you there should be a liquid phase• and your only way to heat the ice is by colliding two ice cubes• So you form a “bunch” containing a billion ice cubes• which you collide with another such bunch• 10 million times per second• which produces about 1000 IceCube-IceCube collisions per
second• which you observe from the vicinity of Mars
Change the length scale by a factor of ~1013
You’re doing physics at LHC !
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 1919
ALICE : The answer to the ALICE : The answer to the challengechallenge
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2020
The todo programThe todo program About 16.000 particles cross the detectors in each collision ; the About 16.000 particles cross the detectors in each collision ; the
particle density reaches 90 particles per cmparticle density reaches 90 particles per cm22, near the interaction , near the interaction point !point !
Measure every particle individually: count them, localise their Measure every particle individually: count them, localise their trajectory, identify their nature, establish their 4-momentum ; trajectory, identify their nature, establish their 4-momentum ;
Localise the origin within a few Localise the origin within a few m ;m ;
Identify the interesting rare events in less than 100 Identify the interesting rare events in less than 100 s ;s ;
Store data 1,2 Go/s (2 CD/s) et 1 Po/an (a 4 Km high CD pile) ;Store data 1,2 Go/s (2 CD/s) et 1 Po/an (a 4 Km high CD pile) ;
Give access of data to 1,000 physicists spread in 80 institutes in Give access of data to 1,000 physicists spread in 80 institutes in 28 countries.28 countries.
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2121
Un champ magnétiqueUn champ magnétique
Identify the charge
Measure the momentum
Greater momentum
Smaller momentum
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2222
Sensitive materials in the way of Sensitive materials in the way of the particlesthe particles
t=0 t=t2t=t1 t=t3 t=t4
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2323
Internal trajectography (ITS): p, id
ALICE : Many cells everywhere …ALICE : Many cells everywhere … To localise, segmenting the system in hundreds of millions of To localise, segmenting the system in hundreds of millions of
sensitive cells ; sensitive cells ; Surround the interaction point with detector enveloppesSurround the interaction point with detector enveloppes
Time projection chambre (TPC) : p, pid
Transition radiation detector (TRD):
électrons
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2424
… … and a few specialized detectorsand a few specialized detectors
Muons spectrometre :• Passif absorber • B dipole• Trajectographe• Filter• Trigger
Photons
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2525
How does it workHow does it work Internal trajectographe : 6 layers of Si diodes with 2D localisation Internal trajectographe : 6 layers of Si diodes with 2D localisation
m
Si-pSi-n
-HV
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2626
3 technologies Si3 technologies Si
256 anodes, 294 m pitch
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2727
How does it workHow does it work The main trajectographe : 1 time projection chamberThe main trajectographe : 1 time projection chamber
-HVE E
Arrival time
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2828
TPC ALICETPC ALICE
Readout plane segmentation
18 trapezoidal sectors
each covering 20 degrees in azimuth
EE
510 cm
EE
88s
GAS VOLUME88 m3
DRIFT GAS90% Ne - 10%CO2
Pb P
E
E
5 m
5.6 m
1.6
400 V / cm
NE / CO2 88s
End plate
Central electrode
Drift volume
Co2 insulation
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 2929
Identification of particlesIdentification of particles
Measure energy loss
Trajectography: charge and momentum
Measure time of flight
p pp p
K K -
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3030
Still smarterStill smarter Distinguish relativistic electrons and pionsDistinguish relativistic electrons and pions
• When a relativisticparticle crosses an inhomogenuous medium an X ray is emitted
• Select the medium such as only electrons create the transition radiation
• Detect both the charged particle and the X ray
• Multi-wire chamber filled with a heavy gas (Xe)
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3131
And to be completeAnd to be complete Dense like lead and transparent like crystal to stop Dense like lead and transparent like crystal to stop
photons photons • Photons materialise as a cascade of electrons and positons
• Electrons excite atomes of the crystal
• Atomes deexcitent by emetting an UV radiation
•UV radiations are detected at one end of the crystal by a photodiode
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3232
From volts to bytesFrom volts to bytes
The signal of each cell (~16 millions) is procesed by The signal of each cell (~16 millions) is procesed by highly miniaturised electronic systems ;highly miniaturised electronic systems ;
The electric signal is digitalised to be processed by The electric signal is digitalised to be processed by computers ;computers ;
The information is transported by optical fibers.The information is transported by optical fibers.
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3333
Design the detectorDesign the detector Simulations : Simulations :
• Generate physics events at the best of our theoretical knowledgeGenerate physics events at the best of our theoretical knowledge
• Construct a virtual detecteor and simulate its response based of Construct a virtual detecteor and simulate its response based of our knowledge on the interactions of particles with matterour knowledge on the interactions of particles with matter
Tools :Tools :
• Programming techniques : object orientedProgramming techniques : object oriented
• Huge computing and storage capacities : distributed computingHuge computing and storage capacities : distributed computing
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3434
3 million volumes
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3535
What we should be prepared toWhat we should be prepared to
60 << 62 One collision : Pb+Pb @ 5.5 TeV
dN/dy = 8,000
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3636
What we should be prepared toWhat we should be prepared to
One event : p+p @ 14 TeV
20 collisions overlay
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3737
To process the dataTo process the data
Yerevan
CERN
Saclay
Lyon
Dubna
Capetown, ZA
Birmingham
Cagliari
NIKHEF
GSI
Catania
BolognaTorino
PadovaIRB
Kolkata, India
OSU/OSCLBL/NERSC
Merida
Bari
Nantes
Distributing ressources :• CPU• Data storage
Are distributed around the world
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3838
Exemple of physics signal (1)Exemple of physics signal (1)1. Ordinary matter1. Ordinary matter
Transverse momentum
dN
/dp
Fragmentationfunction
dN
/d
Relative angle
-180 O 18O
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 3939
Exemple of physics signal (1)Exemple of physics signal (1)2. Quark matter2. Quark matter
Transverse momentum
dN
/dp
Fonction de fragmentation
dN
/d
Relative angle
-18O O 18O
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 4040
Exemple of physics signal (2)Exemple of physics signal (2)1. Ordinary matter1. Ordinary matter
Mass
dN
/dp
J/cc
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 4141
Exemple of physics signal (2)Exemple of physics signal (2)2. Quark matter2. Quark matter
Mass
dN
/dp
J/cc
23 Juin 200323 Juin 2003 Yves SchutzYves Schutz 4242
ALICE todayALICE today