Sept 8-12, 2008 ICHIC-Goa School 1 Quark-Gluon Plasma – Introduction to Experiments Part - 1 Tapan Nayak VECC, Kolkata [email protected] [email protected]
Dec 26, 2015
Sept 8-12, 2008 ICHIC-Goa School 1
Quark-Gluon Plasma – Introduction to Experiments
Part - 1
Tapan NayakVECC, Kolkata
Sept 8-12, 2008 ICHIC-Goa School 2
The QCD Phase diagramT
empe
ratu
re
baryon density
Neutron stars
Early universe
nucleinucleon gas
hadron gascolour
superconductor
quark gluon plasmaTc
0
critical point ?
vacuum
CFL
High Temperature
High baryon density
DeconfinementChiral symmetry restoration
By increasing the
collision energy
Sept 8-12, 2008 ICHIC-Goa School 3
Why do we expect in a phase transition from hadronic phase to quark-gluon plasma?
/T4
Hadronic matter
Quark-gluon plasma
TTC
Hagedorn Limiting Temperature
is energy density and T is temperature. In hadronic phase both pions and nucleons are regarded as elementary particles, and the system would have a limiting temperature, called the Hagedorn temperature (QM ’84 proceedings). This is analogous to the boiling temperature of water. At around 100deg C even if heat supplied is more, most of the heat energies are used to forming bubbles and not increasing the kinetic energies of water molecules. Similarly in hadronic matter most energies are used to forming pion bubbles. The boilng temp is of the order of pion mass.
On the other hand, q-q interactions become weaker as the inter-quark distance becomes shorter (asymptotic freedom). The system behaves like free quarks and gluons. Therefore Stephan-Boltzmann law holds and there is no limiting temperature. Thus we expect a phase transition at T~TC.
Sept 8-12, 2008 ICHIC-Goa School 4
Stephan Boltzman limits for a free Quark Gluon gas
En
erg
y D
ensi
ty/
(Tem
per
atu
re)4
TC ~ 170 15 MeV
C ~ 0.7-1.2 GeV/fm3
0 ~ 0.16 GeV/fm3
F. Karsch, Prog. Theor. Phys. Suppl. 153, 106 (2004)
QCD EoS from Lattice
Recent Lattice results seem to give a value of Tc to be 190 MeV
T/Tc
Sept 8-12, 2008 ICHIC-Goa School 5
• Energy Density from experiments: Bjorken estimation
• Temperature from pT spectra of emitted particles (for example: pT spectra of
QCD EoS from Experiments
We can get some idea about the:
(1) Effective degrees of freedom (thermodynamic degeneracy) at a (2) Time () at which matter comes to approximate thermal equilibrium and starts to behave like a hydrodynamic fluid.
Problems arise in accessing Initial conditions:
Initial Energy densities
Initial Temperatures
Sept 8-12, 2008 ICHIC-Goa School 6
Initial Energy Density – Bjorken estimation
R2
dydz 0
Boost invariant hydrodynamics:
Bjorken 1983
d
dNm
R
dy
dE
R
chT
TBj
2
31
1)(
2
2
: proper timey : rapidity: pseudo-rapdityET: transverse energyNch : Number of charged particlesmT : transverse massR: effective transverse radius
Sept 8-12, 2008 ICHIC-Goa School 7
Initial Energy Density and Temperature
d
dNm
R
dy
dE
R
chT
TBj
2
31
1)(
2
2
and T
1. Pseudorapidity distribution of charged particles and photons
3. Rapidity distribution of transverse energy
2a. pT distributions and temperature
2b. Estimation of mean transverse mass, <mT>
4. Source size, R from HBT measurements
Sept 8-12, 2008 ICHIC-Goa School 8
In non-relativistic physics the Galileo law of summation of velocities is valid:
v2 = v1 + v (non-rel),
where v1 and v2 are the velocities measured in reference frames one of which moves at a velocity v with respect to the other.
In relativistic physics instead of the above, the Einstein law of summation of velocities is valid:
v2 = (v1 + v) / (1+v1v/c2) (relativistic)
This is non-additive one. This is inconvenient as difference in velocities of two particles depends on the choice of the moving reference frame.
To retain the property of additivity a new kinematic quantity – the rapidity (y) is introduced in relativistic kinematics . By definition:
y = ½ ln (c+v)/(c-v)
And with this, one can show that: y2 = y1 + y (relativistic)
Thus the difference yA – yB in rapidities of two particles in same in all moving reference frame.
Kinematics: What is Rapidity?
Sept 8-12, 2008 ICHIC-Goa School 9
Kinematics: y etc.
Heavy-ion Collision
Target
Projectile
p||
pT
p||
pT
y
dn/dyytarget ybeam
p||
pT
y
dn/dyytarget ybeam
β
z
z
pE
pEy ln
2
1
)/(tanh 1 Epy z
1tanh yy
Pseudorapidity:
)2/tan(ln
Sept 8-12, 2008 ICHIC-Goa School 10
Many quantities scale with Npart
or a combination of Npart and
number of collisions, Ncoll:• Transverse Energy• Particle Multiplicity• Particle Spectra
“Spectators”
“Spectators”
“Participants”
Zero-degreeCalorimeter
Detectors at 90o
The collision geometry (i.e. the impact parameter) determines the number of nucleons that participate in the collision
Centrality Selection: participants vs. Spectators
Sept 8-12, 2008 ICHIC-Goa School 11
RHIC BRAHMSPHOBOS
PHENIXSTAR
AGS
TANDEMS
RRelativistic elativistic HHeavy eavy IIon on CCollider (RHIC)ollider (RHIC)Brookhaven National Laboratory (BNL), Upton, NYBrookhaven National Laboratory (BNL), Upton, NY
v = 0.99995c = 186,000 miles/sec Au + Au at 200 GeV
Animation M. Lisa
Sept 8-12, 2008 ICHIC-Goa School 12
STAR Experiment at RHIC
Barrel EM Calorimeter
FTPCs
Time Projection Chamber
Silicon TrackerSVT & SSD
Endcap Calorimeter
Magnet
Coils
TPC Endcap & MWPC
Central Trigger Barrel & TOF
Beam Beam Counters
4.2 meters
Not Shown: pVPDs, ZDCs, and FPDs
TPC is at the heart of STAR
PMD
Sept 8-12, 2008 ICHIC-Goa School 13
TPC Gas Volume & Electrostatic Field Cage
• Gas: P10 ( Ar-CH4 90%-10% ) @ 1 atm
• Voltage : - 28 kV at the central membrane 135 V/cm over 210 cm drift path
420 CM
Self supporting Inner Field Cage: Al on Kapton using Nomex honeycomb; 0.5% rad length
Sept 8-12, 2008 ICHIC-Goa School 14
Pixel Readout of a Pad Plane Sector
A cosmic ray + deltaelectron
3 sigma threshold
Sept 8-12, 2008 ICHIC-Goa School 15
Gold GoldsNN = 130, 200 GeV
(center-of-mass energy per nucleon-nucleon collision)
1000’s of particles
Au on Au Event at RHICTwo-track separation 2.5 cm
Momentum Resolution < 2%
Space point resolution ~ 500 m
Rapidity coverage –1.8 < < 1.8
Sept 8-12, 2008 ICHIC-Goa School 16
Time Projection Chamber: 45 padrow, 2 meters (radius), dE/dx)8%, -1<Multi-gap Resistive Plate Chamber TOFr: 1 tray (~1/200), (t)=85ps
Hadron identification: STAR Collaboration, nucl-ex/0309012
Particle ID:
Sept 8-12, 2008 ICHIC-Goa School 17
Resonance K*(892) (770) f0(980) (1020) (1232) (1520) (1385)Decay channel K K K p p K
Branching Ratio % ~100 ~100 dominant 49.2 >99 22.5 88.2
Width [MeV] 50.7 150 40 to 100 4.46 ~120 15.6 35.8
Life time [fm/c] 4 1.3 40 ~1.75 13 5.6
Sept 8-12, 2008 ICHIC-Goa School 18
Particle ID using Topology & Combinatorics
Secondary vertex: Ks + p +
+ + K e++e-
Ks + + - K + + K -
p + - + + -
from K+ K- pairs
K+ K- pairs
m inv
m inv
same event dist.mixed event dist.
background subtracted
dn/dm
dn/dm
“kinks”
K +
Sept 8-12, 2008 ICHIC-Goa School 20
Shapes of dNch/d versus (s = 130)
dN
ch/d
(dN
ch/d)
/(½
Np
art)
0-3%
15-20
35-40
PHOBOS: nucl-ex/0106006
PHOBOS: 3% most central collisions <Nch> = 4200 470
Sept 8-12, 2008 ICHIC-Goa School 21Dec 11, 2007 DAE Nuclear Physics Symposium, Sambalpur 21
Particle production
Number of charged particles as a function of pseudorapidity
=> LHC predictions (Pb+Pb at 5.5TeV): 1100-2000
Extrapolation to LHCAu+Au 0-6% centrality
Sept 8-12, 2008 ICHIC-Goa School 22
Particle Density (dN/dvs. s1/2
WA98
WA97/NA57Phobos
NA49
E917/866
STARRESULTS
E877
PHENIX
BRAHMS
Phobos
Top 5% centrality
Sept 8-12, 2008 ICHIC-Goa School 23
2a. pT distributions and temperature
2b. Estimation of mean transverse mass, <mT>
Sept 8-12, 2008 ICHIC-Goa School 24
p+, p-, K+, K- spectra versus centrality: PRL 92 (2004) 171801
Bose-Einstein fits
mTmAe
/mt exponential fits
K-)1/( / effTmeA
+
Identified Particle Spectra Au+Au @ 200GeV
Sept 8-12, 2008 ICHIC-Goa School 26
Pressure, Flow, …
dd = dU + pdV = dU + pdV – entropy; p – pressure; U – energy; V – volume
= kBT, thermal energy per dof
In high-energy nuclear collisions, interaction among constituents and density distribution will lead to: pressure gradient pressure gradient collective flow collective flow
number of degrees of freedom (dof) Equation of State (EOS) The thermalization is not required – pressure gradient only depends on the density gradient and interactions. Space-time-momentum correlations!
Nu Xu
Sept 8-12, 2008 ICHIC-Goa School 27
Hadron Spectra from RHICp+p and Au+Au collisions at 200 GeV
sss
ss
uud
ud
Multi-strange hadron spectra are exponential in their shapes. STAR white papers - Nucl. Phys. A757, 102(2005).
mT pT2 m 2
f exp(mT /Tslope )
mor
e ce
ntra
l col
lisio
ns
0-5%
Freeze-out Systematic
At freeze-out:
The ‘temperature’ parameters Tfo seem to be around 100 -140 MeV.
v2 continuously rise with beam energy. A clear increase in averaged velocity parameters r - increase of the ‘pressure’ in the system at RHIC.
When v2 crosses zero, a plateau appears for Tfo and r at beam energy ~ 5 GeV.
STAR: -mesons
200 GeV A+A collisions:- The multi-strange baryons productions , are enhanced in A+A collisions- The -meson productions are also enhanced, but may be with different trends The enhancements are NOT due to Canonical Ensample Suppression!
PRL. 98 (2007) 062301 (nucl-ex/0606014); PRL in print, nucl-ex/ 0703033; nucl-ex/ 0705.2511
Sept 8-12, 2008 ICHIC-Goa School 31
Blast Wave Fits: Tfo vs.
1) 1) , , KK, and , and pp change change smoothly from peripheral smoothly from peripheral to central collisions.to central collisions.
2) At the most central2) At the most central collisions, collisions, TT reaches reaches
0.6c.0.6c.
3) Multi-strange particles 3) Multi-strange particles ,, are found at higher are found at higher TTfofo
and lower and lower TT
light hadrons movelight hadrons move with higher velocitywith higher velocity compared to strangecompared to strange hadronshadrons
STAR: NPA715, 458c(03); PRL 92, 112301(04); 92, 182301(04).
200GeV Au + Au collisions200GeV Au + Au collisions
Nu Xu
Sept 8-12, 2008 ICHIC-Goa School 32
-meson Flow: Partonic Flow
“-mesons are produced via coalescence of seemingly thermalized quarks in central Au+Au collisions. This observation implies hot and dense matter with partonic collectivity has been formed at RHIC”
QM2008: J. Chen; X.B. Wang
Sept 8-12, 2008 ICHIC-Goa School 33
EoS Parameters at RHIC
In central Au+Au collisions at RHIC - partonic freeze-out:
*Tpfo = 165 ± 10 MeV weak centrality dependence
vpfo ≥ 0.2 (c)
- hadronic freeze-out:*Tfo = 100 ± 5 (MeV) strong centrality
dependence
vfo = 0.6 ± 0.05 (c)
Systematic study are needed to understand the centrality dependence of the EoS parameters * Thermalization assumed
Nu Xu
Sept 8-12, 2008 ICHIC-Goa School 35
Transverse energy (ET) is the energy produced transverse to the beam direction.This is generated due to the initial scattering of partonic constituents of the incomingnuclei and the rescattering of the produced partons and hadrons.
Transverse phase space is ideal to study the initial conditions after the collision.
Motivation: =>Estimation of the Bjorken energy density of the produced fireball thru the estimation of ET on an event by event basis to verify if a condition for deconfinement does exist.
=> Study of particle production mechanism
=>Study of Quark-Hadron phase transitions thru fluctuation observables like ET and the ratio of it’s components.
Measurement of Transverse Energy (ET)Raghunath Sahoo: Ph.D. thesis
arXiv:0804.1800 [nucl-ex]
The hadronic transverse energy (EThad) is measured thru the TPC
reconstructed tracks (PID and momentum information).
The electromagnetic transverse energy (ETem) is measured thru the
calorimeter tower hits after correcting for the hadronic contaminations.
Sept 8-12, 2008 ICHIC-Goa School 36
ET Distributions @ 62.4 GeV Au+Au Collisions
Minimum-bias distribution of hadronic transverse energy
Minimum-bias distribution of electromgnetic transverse energy
Sept 8-12, 2008 ICHIC-Goa School 37
Minimum-bias distribution of total transverse energy
62.4 GeV Au+Au CollisionsSTAR Preliminary
Transverse energy distribution fordifferent centrality classes.
62.4 GeV Au+Au Collisions
Raghunath Sahoo
Sept 8-12, 2008 ICHIC-Goa School 38
STAR Preliminary
• The EKRT model (based on final state Gluon saturation) underestimates the final transverse energy.
The excitation function of dET/dy per participant pair from AGS to RHIC.
Raghunath Sahoo
Sept 8-12, 2008 ICHIC-Goa School 40
HBT Intensity Interferometry
Intensity interferometry has an intimate relation with Michelson amplitude interferometryAmplitude interferometry measured from detectors 1 and 2 :
| A1 + A2 |2 = | A1|2 + | A2|2 + ( A1* A2 + A1 A2
*)
The later term in the parenthesis is the called the “fringe visibility” .Averaged over,
<V2> = 2 < | A1|2| A2|2> + <A1*2A2
2> + <A12A2
*2> The first term r.h.s above is just twice the correlation of the
intensities landing in the two detectors.<V2> 2<I1I2>
Robert Hanbury Brown and Richard Twiss
p1
“b” source(x)
r1
r2
x1
x2p2
“a” “L”
The goal of intensity interferometry is to extract the space-time information of the heavy-ion collision source from the momentum spectra which are the only measureable quantities making use of quantum statistical correlations between the pairs of identical particles.
Interference is a phenomenon associated with the superposition of two or more waves. The two-particle correlations arise from the interference of particle wave-functionsand depend on whether the particles are bosons or fermions
Debasish Das Ph.D. thesis
Sept 8-12, 2008 ICHIC-Goa School 41
Probing source geometry through interferometry
2
21
2121 )q(~1
)p(P)p(P)p,p(P
)p,p(C
Measurable!F.T. of pion source
The correlation function is defined as the ratio of the probability for the coincidence of p1 and p2 relative to the probability of observing p1 and p2 separately :
Correlation function constructed experimentally, C2 (q) = A (q) / B (q) (normalized to unity at large q),
A (q) is the pair distribution in momentum difference q = p2 - p1 for pairs of particles from
the same event. B (q) is the corresponding distribution for pairs of particles from different events.
Courtesy of S. Bassp1
“b” source(x)
r1
r2
x1
x2p2
“a” “L”
Sept 8-12, 2008 ICHIC-Goa School 42
Qinv (GeV/c)
C2(
Qin
v)
d+AuR ~ 2 fm
Au+AuR ~ 6 fm
p+pR ~ 1 fm
Source geometry p1
“b” source(x)
r1
r2
x1
x2p2
“a” “L”
Sept 8-12, 2008 ICHIC-Goa School 43
if a pion is emitted, it is more likely to emit anotherpion with very similar momentum which makes the HBT effect
experimentally measuring this enhanced probability: quite challenging
Measuring the Source geometry
Sept 8-12, 2008 ICHIC-Goa School 44
p2
p1
q
R long
Rside
Rout
Rlong – along beam direction
Rout – along “line of sight”
Rside – “line of sight”
Detailed source geometry Debasish Das Ph.D. thesis
Sept 8-12, 2008 ICHIC-Goa School 45
Beam energy dependence of pion HBT
Pion rapidity density is proportional to the freezeout volume => Constant Freezeout Volume (freezeout at a constant density).
STAR Debasish Das Ph.D. thesis
Sept 8-12, 2008 ICHIC-Goa School 46
d
dNm
R
dy
dE
R
chT
TBj
2
31
1)(
2
2
Now finally to Bjorken Energy Density
Sept 8-12, 2008 ICHIC-Goa School 47
Compiled by Raghunath Sahoo
Bjorken Energy Density: Excitation function
Bjorken Energy density increases logarithmically with center of mass energy.
= 1
d
dNm
R
dy
dE
R
chT
TBj
2
31
1)(
2
2
Sept 8-12, 2008 ICHIC-Goa School 48
Rough Estimation for AuAu 10GeV
Bjorken Energy Density – for different centralities
Bjorken Energy density is unique for given centrality and beam energy and can be used as an estimator for different physics topics.
Sept 8-12, 2008 ICHIC-Goa School 49
END OF LECTURE-1
What did we try to learn today:
• Measurement of charged particle multiplicity and rapidity distributions
• Measurement of pT spectra and extraction of effective temperature
• Radial flow and estimation of thermal temperature
• Source sizes from HBT parameters
• Estimation of energy density
• Work in progress: Use of for making an EoS plot
• Work in progress: EoS plot from experimental estimations and
comparison with lattice
SUMMARY