11 heavy ions collisions heavy ions collisions (results and questions) anatoly litvinenko...
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Heavy Ions CollisionsHeavy Ions Collisions(results and questions)(results and questions)
Anatoly Litvinenko
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Outline.Outline.
Ядерная материя при большой плотности энергии Новое фазовое состояние – легко верится
Workshop on Heavy Ions, New York, Nov. 29 - Dec 1, 1974.
The name ”Quark Gluon Plasma” was coined by Eduard Shuryak in 1978.
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The conception of the phase diagram of QCD as a function of time
L. McLerran and N. Samios
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Lattice QCD
GeVTc 0.17=
Frithjof Karsch, arXiv:hep-lat/0106019v2 (2001)
F. Karsch, Lecture Notes in Physics 583 (2002) 209.
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Space-time structure of heavy ions collisions
kinetic freeze-out(no collisions)
Chemical freeze-out(no particles production)
Parton-parton interaction
Initial inelastic collisions
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RRelativistic elativistic HHeavy eavy IIon on CCollider (ollider (RHICRHIC))
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2 rings, 3.8 km circumference.2 rings, 3.8 km circumference.Polarized p and Nucleus up to Au.Polarized p and Nucleus up to Au.
Top energies (each beam):Top energies (each beam):100 GeV/nucleon Au-Au. 250 GeV polarized p-p.100 GeV/nucleon Au-Au. 250 GeV polarized p-p.
NIM, v.499, p. 235-880, (2003)
GeV200SNN
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STAR
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The PHENIX Detector Детектор PHENIX регистрирует различные частицы после столкновения:фотоны, электроны, мюоны и адроны (пионы и протоны).
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The PHOBOS Detector
137000 Silicon Pad Channels
1m
12m Be Beampipe
Spectrometer
Octagon
Vertex
Ring Counters
Paddle Trigger Counter
Cerenkov Counter
DX magnet DX MagnetZDC ZDC
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The BRAHMS Experiment
95°
30°
30°
15°
2.3°
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LHC
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Questions have to be answered
1.Can we achieve high energy density in nuclear-nuclear collisions ?
2.What is the baryon density for hadronic matter created?
3.Whether thermodynamic equilibrium is established?
Related question
Can we make conclusion about this from experiment?
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STAR EVENTShttp://www.star.bnl.gov/
p+p (200 GeV)Central
Au+Au(200 GeV)
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s
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QUESTION I(a)QUESTION I(a)
How much energy is lost by primary hadrons?What is barion density of produсed
hadronic matter?
Can we make some conclusion from experiment?
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Stopping power
Net protons distribution
BRAHMS collaboration PRL 93, 1020301 (2004),
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Stopping power
BRAHMS collaboration PRL 93, 1020301 (2004),
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QUESTION I(b)QUESTION I(b)
Can we have high energy densityin nuclear-nuclear collisions ?
Can we make some conclusion from experiment?
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Energy density and Bjorken equation
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Dependence on centrality of charged hadron density
S.S. Adler et al. , Phys. Rev. C 71, 034908 (2005)
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Dependence on pseudorapidity of charged hadron
Not to be confuse - it is a different distribution
B. Alver et al.Phys. Rev. C 83, 024913 (2011) PHOBOS Coll.
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Dependence on pseudorapidity of charged hadron
The CMS collaboration, J.High Energy Phys 08, p.141 (2011)
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Dependence on pseudorapidity of charged hadron
The CMS collaboration, J.High Energy Phys 08, p.141 (2011)
«LHC multiplicity is two times greater than at RHIC»
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Dependence on centralty of charged hadron
S.S. Adler et al. , Phys. Rev. C 71, 034908 (2005)
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S.S. Adler et al. , Phys. Rev. C 71, 034908 (2005)
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Can we have high energy densityin nuclear-nuclear collisions ?
Can we make some conclusion from experiment?
Yes! For RHIC and LHC energy
QUESTION I(b)QUESTION I(b)
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QUESTION IIQUESTION II
Is equilibrium state of hot and dense hadronic matter achieved?
What is conclusions from experiment?
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QUESTION IIQUESTION II
Is equilibrium state of hot and dense hadronic matter achieved?
The possible observable Particle ratios Particle spectra Collective flows
… ?
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Particle ratio and sParticle ratio and statistical modelstatistical models
These models reproduce the ratios of particle yields with only two (or three ) parameters
One assumes that particles are produced by a thermalized system with temperature T and baryon chemical potential
The number of particles of mass m per unit volume is :
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Particle ratios and statistical model(s)
Peter Braun-Munzinger, Krzysztof Redlich, Johanna StachelarXiv:nucl-th/0304013v1, (2003)«Of particular interest is the extent to which the measured particle yields are showing equilibration.»
Estimation of equlibration time for RHIC and LHC (have to be studied)R. Baier, A.H. Mueller, D. Schiff, and D.T. Son, Phys. Lett. B 502 (2001)51; Nucl. Phys. A698 (2002) 217.
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A. Tawfik ; arXiv:hep-ph/0508244v3 22 Mar 2006
Statistical methods have become an important tool to study the propertiesof the fireball created in high energy heavy ion collisions, where theysucceed admirably in reproducing measured yield ratios.
1. Can this success be taken as evidence that the matter produced in these collisions has reached thermal and chemical equilibrium?
2. Can the temperature and chemical potential values extracted from such statistical model fits be interpreted as the equilibrium properties of the collision matter?
STAR Coll., Nucl. Phys. A 757 (2005) 102
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Particle ratiosParticle ratios
S. S. Adler, et al., Phys. Rev. C69 (2004) 034909
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Particle ratios and sParticle ratios and statistical modelstatistical models
chemical freeze-out
Nucl. Phys. A758, No.1-2, p.184, (2005)
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Particle ratios and sParticle ratios and statistical modelstatistical models
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Particle ratios and sParticle ratios and statistical modelstatistical models
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arXiv:nucl-th/0304013 v1 3 Apr 2003
Peter Braun-Munzinger, Krzysztof Redlichb, Johanna Stachel
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Low energy (NA49)
Katarzyna Grebieszkow for the NA49 and the NA61 CollaborationsACTA PHYSICA POLONICA Vol. B41, No 2,p.427 (2010)
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Particle (hadrons) Particle (hadrons) spectraspectra
kinetic freeze-out
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Particle (hadrons) Particle (hadrons) spectraspectra
R. Stock; «Quark Matter 99 Summary: Hadronic Signals»arXiv:hep-ph/9911408v1 19 Nov 1999
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BorisTomasic, arXiv:nucl-th/0304079 v1 25 Apr 2003
blast-wave model
1. Pions, nucleons and also kaons decouple all quite suddenly from the whole transverse profile of the fireball. For all of them the freeze-out happens at the same proper time, measured in a frame that co-moves longitudinally with the fluid element of the expanding firebal
2. The radial density distribution at the freeze-out is uniform.3. Longitudinal expansion is boost-invariant. 4. In this study, the transverse expansion is parametrized through
rapidity, which depends linearly on the radial coordinate.
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BorisTomasic, arXiv:nucl-th/0304079 v1 25 Apr 2003
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Particle (hadrons) Particle (hadrons) spectraspectra
A Iordanova (for the STAR Collaboration);J. Phys. G35, p.044008, (2008
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Elliptic flowElliptic flow
For big value of elliptic flow you need to save space anisotropy for a long enough timeThe value of elliptic flow is sensitive to the Equation of State (EoS)
Importance of elliptic flowImportance of elliptic flow
1.Gives information about equilibration time2.Gives information about EoS
On the next slides it is shown how ensemble of free streaming particles loses its space eccentricity
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TIME = 0 fm/c, 0.7
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TIME = 1 fm/c, 0.6
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TIME = 2 fm/c, 0.5
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TIME = 3 fm/c, 0.3
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:
elliptic flow hydrodynamicselliptic flow hydrodynamics
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elliptic flow and space eccentricityelliptic flow and space eccentricity
ε/=A 2v 2
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Evidence for the short thermalization time
Good description of elliptic flow by hydrodynamics with initiation conditionjust from geometry of collision
Constant ratio of elliptic lowto the space eccentricity
Fast decreasing of space anisotropy for the free streaming particle
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QUESTION IIQUESTION II
Is equilibrium state of hot and dense hadronic matter achieved?
What is the conclusion about it from experiment?
The strong indication that YES.
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Some designations
sQGP for strongly-interacting Quark-Gluon Plasma
Commonly accepted:QGP, pQGP,wQGP
for weakly-interacting Quark-Gluon Plasma
Observables and hadronic matter properties
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KEKETT – CQN Scaling – CQN ScalingKEKETT – CQN Scaling – CQN Scaling
Phys. Rev. Lett. 98, 162301 (2007)
Mesons
Baryons
Quark-Like Degrees of Freedom EvidentQuark-Like Degrees of Freedom Evident
Roy A. Lacey, Stony Brook; Quark Matter 09, Knoxville, TN March 30 - April 4, 2009
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K. Aamodt et al.(ALICE Collaboration), PRL 105, 252302 (2010)
Elliptic flow – energy Elliptic flow – energy dependancedependance
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JET Quenching
Modification of Jet property in AA collisions, because of partons propagating in colored matter, which lose energy.
One of the possible observable
Was predicted in a lot of works. Some of them (not all) are:
1
0)(Pd
J.D.Bjorken (1982), Fermilab – PUB – 82 – 059 - THY.M.Gyulassy and M.Palmer, Phys.Lett.,B243,432,1990.X.-N.Wang, M.Gyulassy and M.Palmer, Phys.Rev.,D51,3436,1995.R.Baier et al., Phys.Lett.,B243,432,1997.R.Baier et al., Nucl.Phys.,A661,205,1999
Jet: A localized collection of
hadrons which come from a fragmenting parton
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High pT (> ~2.0 GeV/c) hadrons in NN
h
h
h
abc
dParton distribution functions
Hard-scattering cross-section
Fragmentation Function
h
)Q,x(f 2aaa/A )Q,x(f 2
bbb/B cdabd )Q,z(D 2ddd/h
d,c,b,ahXABd
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h
High pT (> ~2.0 GeV/c) hadrons in AA
A
B
h Hard-scattering cross-section
Fragmentation Function
Parton distribution functions
+Numbers of binary collisionsPartonic Energy
Loss
(...)f b/B(...)f a/A cdabd
)Q,z(D 2d
*dd/h
1
0 d
*d
z
z)(Pd
∑→dcba
hXABd,,,
=σ CollN
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Nuclear modification factor
is what we get divided by what we expect.is what we get divided by what we expect.
NN
collAAAA d
NdR
σ><σ
=/
From naive picture
AAR
Suppression of high-pt hadrons. Qualitatively.
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6666
First data in first RHIC RUN
Jet Quenching ! Great!
But (see the next slide)
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Nuclear modifications to hard scattering
Large Cronineffect at SPSand ISRSuppression at RHIC
Is the suppression due to the medium?(initial or final state effect?)
RAA (pT ) d2N AA /dpTdTAAd
2 NN /dpTd
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Au+Au @ sNN
= 200 GeV d+Au @ sNN
= 200 GeV
preliminary
Au+Au @ sNN
= 200 GeV d+Au @ sNN
= 200 GeV
preliminary
Au+Au @ sNN
= 200 GeV d+Au @ sNN
= 200 GeV
preliminary
Au+Au @ sNN
= 200 GeV d+Au @ sNN
= 200 GeV
preliminary
• Nice picture! Isn’t it?
Again Au+Au and d+Au
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The matter is so opaque that even The matter is so opaque that even
a 20 GeV a 20 GeV 00 is stopped is stopped..
• Suppression is very strong (RAA=0.2!) and flat up to 20 GeV/c• Common suppression for 0 and it is at partonic level• > 15 GeV/fm3; dNg/dy > 1100
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.ALICE Collaboration, Physics Letters B 696 (2011) 30.
JET Quenching at LHC
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ALICE Collaboration, Physics Letters B 696 (2011) 30
JET Quenching at LHC
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The matter is so dense that even heavy quarks are stopped
Even heavy quark (charm) suffers substantial energy loss in the matter
The data provides a strong constraint on the energy loss models.
The data suggest large c-quark-medium cross section; evidence for strongly coupled QGP?(3) q_hat = 14 GeV2/fm
(2) q_hat = 4 GeV2/fm
(1) q_hat = 0 GeV2/fm
(4) dNg / dy = 1000
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If there are any other observables for Jet Quenching?
Correlation of trigger particles 4<pT<6.5 GeV withassociated particles 2<pT<pT,trig
Associated particles
Near side jetTrigger particle
Away side jet
Yes! Back to Back Jets correlation.
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In-plane In-plane
Out-of-plane
Out-of-plane
Back to Back Jets correlation.Back to Back Jets correlation.Dependence from reaction plane.Dependence from reaction plane.
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Jet tomography
20-60%
STAR Preliminry
20-60%
Back-to-back suppression depends on the reaction plane orientation
In-plane
Out-plane
energy loss dependence energy loss dependence on the path length!on the path length!
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The matter is so dense that it The matter is so dense that it modifies the shape of jetsmodifies the shape of jets
• The shapes of jets are modified by the matter.– Mach cone?– Cerenkov?
• Can the properties of the matter be measured from the shape?– Sound velocity– Di-electric
constant• Di-jet tomography is
a powerful tool to probe the matter
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Resonances melting (Debye scrinig)
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One more results from lattice QCD
heavy-quark screening mass
r/)rexp(~)r(
In EM plasma it is well known Debye screening
T/1~r/1 D
/J -- suppression
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The matter is so dense that it melts(?) J/ (and regenerates it ?)
CuCu
200 GeV/c
AuAu
200 GeV/c
dAu
200 GeV/c
AuAuee
200 GeV/c
CuCuee
200 GeV/c
J/’s are clearly suppressed beyond the cold nuclear matter effect
The preliminary data are consistent with the predicted suppression + re-generation at the energy density of RHIC collisions.
Can be tested by v2(J/)?
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The matter is so dense that it melts Y.
QM’11
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direct photons
8181
• T0max ~ 500-600 MeV !?
T0ave ~ 300-400 MeV !?
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SummarySummary
o RHIC has produced a strongly interacting,RHIC has produced a strongly interacting, partonic state of dense matterpartonic state of dense matter
/ 15 3fmGeVBj
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8383
SummarySummary
o The matter is so dense that even heavy quarks are stopped
(3) q_hat = 14 GeV2/fm
(2) q_hat = 4 GeV2/fm
(1) q_hat = 0 GeV2/fm
(4) dNg / dy = 1000
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SummarySummary
o The matter is so strongly coupled that even heavy quarks flow
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SummarySummary
o The matter is so dense that it melts(?) J/ (and regenerates it ?)
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SummarySummary
o The matter modifies jets
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SummarySummary
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The matter is hot 8888
The matter may melt but regenerate J/’s
Put the results together
The matter is denseThe matter is strongly coupled
The matter modifies jets
> 15 GeV/fm3
dNg/dy > 1100
Tave = 300 - 400 MeV (?)PHENIX preliminary
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Backup slidesBackup slides
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January 6, 2002 RHIC/INT Winter Workshop 2002 90
Modeling the Source• Interaction region
Assembly of classical boson emitting sources in space-time region
• The source S(x,p) is the probability boson with p is emitted from xDetermines single-particle momentum spectrum
E d3N/dp3 = d4x S(x,p)
Determines the HBT two-particle correlation function C(K,q) C(K,q) ~ 1 + | d4x S(x,K) exp(iq·x) | 2/| d4x S(x,K) |2
where K = ½(p1 + p2) = (KT, KL), q = p1 – p2
The LCMS frame is used (KL = 0)
• In the hydrodynamics-based parameterizations: assume something about the source S(x,p)Gaussian particle density distribution
Linear flow (rapidity or velocity) profile
Instantaneous freeze-out at constant proper time (“sharp”)
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CollN(...)/ aAf (...)/ bBf cdabd
1
0 d
*d
z
z)(Pd )Q,z(D 2
d*dd/h∑
dcba ,,,
(...)/ aAf (...)/ bBf cdabd ),(/2dddh QzD∑
dcba ,,,
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9393
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9494
Why the collisons of heavy nuclei is interesting?
Let us see on the space – time picture of collision
pre-collision QGP (?) and parton production
hadron production
hadron reinteraction
QCD phase diagram
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9595
The QGP in the early universe
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9696
What kind of transition is predicted by lattice QCD
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97
Dependence on pseudorapidity of charged hadron
S.S. Adler et al. , Phys. Rev. C 71, 034908 (2005)
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9898
Theoretical explanation
Comparison to model calculations with and without parton energy loss:
Numerical values range from ~ 0.1 GeV / fm (Bjorken, elastic scattering of partons)~several GeV / fm (BDMPS, non-linear interactions of gluons)
Too many approaches.We need additional data!
2.0~Rand,p~d AuAu8
T
2.0~p/p
Estimation from data
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9999
Initial state effects (test experiment d+Au)
Suppression in central Au+Au due to final-state effects
/h
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100100
Binary scaling. Is it work?
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101101
How about suppression for protons?
pcollccollCP )N/dN/()N/dN(R New
Close to nuclear mod. factor, because no suppression for peripheral coll.
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102102
Jets composition as measured by STAR
Kirill Filimonov, QM’04
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104104
[w/ the real suppression]
( pQCD x Ncoll) / background Vogelsang/CTEQ6
[if there were no suppression]
( pQCD x Ncoll) / ( background x Ncoll)
Au+Au 200 GeV/A: 10% most central collisions
[]measured / []background = measured/background
Preliminary
pT (GeV/c)
Binary scaling. Is it work?
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105105
Theoretical explanation
Comparison to model calculations with and without parton energy loss:
Numerical values range from ~ 0.1 GeV / fm (Bjorken, elastic scattering of partons)~several GeV / fm (BDMPS, non-linear interactions of gluons)
Too many approaches.We need additional data!
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106106
If is there space for Color Glass Condensate or only Cronin Effect?
May be. Look at the BRAMS DATA
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Observables and space time structureObservables and space time structure of of Heavy ion collisionsHeavy ion collisions
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109109
Observables and space time structureObservables and space time structure of of Heavy ion collisionsHeavy ion collisions
Production of hard particles: jets heavy quarks direct photonsCalculable with the tools of perturbative QCD
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110110
Observables and space time structureObservables and space time structure of of Heavy ion collisionsHeavy ion collisions
Production of semi-hard particles: gluons, light quarks relatively small momentum: make up for most of the multilplicity
cGeVpT / 21
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111111
Observables and space time structureObservables and space time structure of of Heavy ion collisionsHeavy ion collisions
Thermalizationexperiment suggest a fast thermalization (remember elliptic flow)but this is still not undestood from QCD
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Observables and space time structureObservables and space time structure of of Heavy ion collisionsHeavy ion collisions
Quark gluon plasma
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Observables and space time structureObservables and space time structure of of Heavy ion collisionsHeavy ion collisions
Hot hadron gas
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Particle ratio and sParticle ratio and statistical modelstatistical models
These models reproduce the ratios of particle yields with only two parameters
One assumes that particles are produced by a thermalized system with temperature T and baryon chemical potential
The number of particles of mass m per unit volume is :
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115115
N/ ratio shows baryons enhanced for pT < 5 GeV/c
One more observable. Particle ratios