Heavy Ion Collisions at RHIC and at the LHC: Theoretical Overview Urs Achim Wiedemann CERN PH-TH
Jan 05, 2016
Heavy Ion Collisions at RHIC and at the LHC:
Theoretical OverviewUrs Achim Wiedemann
CERN PH-TH
From elementary interactions to collective phenomena
How do collective phenomena and macroscopic properties of matter emerge from fundamental interactions ?
1973: asymptotic freedom
QCD = quark model +gauge invariance
Today: mature theory with a precision frontier
• background in search for new physics• TH laboratory for non-abelian gauge theories
QCD much richer than QED:
• non-abelian theory• degrees of freedom change with
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Q2
Open questions• What is the QCD equation of state? How can we test it?
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Tc ≈175 MeV
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εc ≈ (3 − 5) εnuclear mattercold
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0q LqR + q RqL 0 ≈ (250 MeV )3
• What is the origin of mass in the universe?
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T
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μB
CFL2SCHadron Gas
Quark Gluon Plasma
… and more questions…
• Confinement: How does hadronization proceed dynamically?
How is it changed in dense QCD matter?
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LQCDC P ∝θ tr Gμν ˜ G μν[ ]
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θ ≈0
• Why is there no strong CP violation? Or is there at finite temperature?
• What are the properties of matter at the highest temperatures and densities?
Degrees of freedom? Viscosity? Heat Conductivity? Transport of conserved quantum numbers?
• What are the dominant microscopic mechanisms of QCD non-equilibrium dynamics and thermalization?
Parton energy loss? Plasma Instabilities, color chaos?
… and many more …
Question:Why do we need collider energies
to test properties of dense QCD matterwhich arise on typical scales €
sNN = 200GeV [RHIC]
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sNN = 5500GeV [LHC]
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T ≈150 MeV , Qs ≈1− 2 GeV ?
Answer 1: Large quantitative gains
Increasing the center of mass energy implies
Denser initial system, higher initial temperature
Longer lifetime
Bigger spatial extension
Stronger collective phenomena
A large body of experimental data from RHIC supports this argument.
Answer 2: Qualitatively novel access to properties of dense matter
For a detailed experimentation with dense QCD matter, one ideally wants to do DIS on the QGP.
… and we can by using auto-generated probes at high
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sNN
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Q2 >> T ≈150 MeV
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Q2Large allows us to embed well-controlled large- processes (hard probes) in dense nuclear matter.
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sNN
Q: How sensitive are hard probes?
Bjorken’s original estimate and its correction
Bjorken 1982: consider jet in p+p collision, hard parton interacts with underlying event collisional energy loss
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ΔE rad ≈ α sˆ q L2
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dE coll dL ≈10GeV fm
Bjorken conjectured monojet phenomenon in proton-proton
Today we know (th): radiative energy loss dominates
Baier Dokshitzer Mueller Peigne Schiff 1995
• p+p:
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L ≈ 0.5 fm, ΔE rad ≈100 MeV
• A+A:
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L ≈ 5 fm, ΔE rad ≈10 GeV
Negligible !
Monojet phenomenon!
observed at RHIC, see talk by Bill Zajc
(Bjorken realized later that this estimate was numerically erroneous.)
High pT Hadron Spectra
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RAA ( pT ,η ) =dN AA dpT dη
ncoll dN NN dpT dη
Centrality dependence:0-5% 70-90%
L large L small
Centrality dependence: Au+Au vs. d+Au● Final state suppression ● Initial state enhancement
partonic energy
loss
Leading hadron suppression at RHIC:
Abundant yield at collider energies (detailed differential study of experimental signal possible)
+ robust and large signal (medium effect much larger than theoretical uncertainties)
= Basis for controlled experimentation and controlled theoretical interpretation
The medium-modified Final State Parton Shower
Medium characterized bytransport coefficient:
Baier, Dokshitzer, Mueller, Peigne, Schiff (1996); Zakharov (1997); Wiedemann (2000); Gyulassy, Levai, Vitev (2000); Wang ...
Salgado,Wiedemann PRD68:014008 (2003)
● energy loss of leading parton ● pt-broadening of shower €
ˆ q ≡μ 2
λ∝ ndensity
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ωc = ˆ q L2 2€
ωc ω = 32
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ˆ q L
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ωc ω =10
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ωc ω = 3.2
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ωc ω =1
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κ 2 ≡kT
2
ˆ q L
The fragility of leading hadrons
?
• The quenching is anomalously large (I.e. exceeds the perturbative estimate by ~ 5)
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ˆ q • Why is RAA = 0.2 natural ? Surface emission limits sensitivity to
Eskola, Honkanen, Salgado, WiedemannNPA747 (2005) 511, hep-ph/0406319
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ˆ q (τ =1 fm /c) ≥ 5GeV 2
fm≈ 5 ˆ q QCD
pert
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ˆ q How can we understand the size of ?
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ˆ q • defines short-distance behavior of expectation value of two light-like Wilson lines
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Tr W A +(x)W A (y)[ ] ≈ exp1
4ˆ q L (x − y)2 ⎡
⎣ ⎢ ⎤ ⎦ ⎥
o Well-defined but difficult problem in QCD.o Is this calculable from 1st principles in a thermal quantum field theory?
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ˆ q • Are there other classes of measurements sensitive to ?
o to test the microscopic dynamics of parton energy loss on which extraction of is based.o to confirm and further constrain the large value of .
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ˆ q
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ˆ q
How can we better gauge ‘hard probes’?
Where does thisassociated radiationgo to ?
How does this partonthermalize ?
What is the dependence on parton identity ?
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ΔEgluon > ΔEquark, m= 0 > ΔEquark, m>0
Parton energy loss depends on parton identity
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RD h = RAAD RAA
h
• Color charge dependence dominates
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RB h
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ΔEquark,m= 0 > ΔEquark,m>0
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ΔEgluon > ΔEquark
Massless “c,b”Armesto, Dainese, Salgado, Wiedemann, PRD71:054027, 2005
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1
kT2⇒
kT2
kT2 + m 2
E 2 ω2( )
2
• Vacuum and medium radiation is
suppressed due to quark mass Dokshitzer, Kharzeev, PLB 519 (2001) 199
Massive c,b
• Mass dependence dominates
• To test this at the LHC, exploit: light-flavored mesons - gluon parents D - mesons - quark parents (mc~0) B - mesons - quark parents (mb>0)
Jet modifications in dense QCD matter
Armesto, Salgado, Wiedemann, Phys. Rev. Lett. 93 (2004) 242301
• Jets ‘blown with the wind’ Hard partons are not produced in the rest frame comoving with the medium
• ‘Longitudinal Jet heating’: The entire longitudinal jet multiplicity distribution softens due to medium effects. €
dN h dξ
Borghini,Wiedemann, hep-ph/0506218
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ξ =ln ETjet pT
h[ ]
Question:How to relate experimental data
to fundamental properties of dense QCD matter?
Approaches include:Perturbative QCD
Lattice QCDSaturation Physics
String theory…
Approach discussed here
String Theory Calculations of Properties of Matter• AdS/CFT correspondence relates Strong coupling problems Classical Problem in a curved in non-abelian QFT higher-dimensional space
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g2, Nc
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gs,α '= ls2 String coupling and
string tension
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λ ≡g2N T’Hooft coupling
Black hole horizon
Curvature radius
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R2
α '= λ = g2Nc
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TH =r0
π R2= T
• Translation into field theoretic quantities
• Finite T Lattice QCD is difficult to apply too problems involving real-time dynamics (moving QQbar pair, light-like Wilson loops, …)o hydrodynamic properties (Problem of analytical continuation to if lowest Matsubara frequency in imaginary time formalism is .)o ….
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ω → 0
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2πT
Maldacena, 1997
AdS/CFT Calculation of Quenching Parameter
Maldacena (1998)Rey and Lee (1998)
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W F (C)T
≡ exp iS(C)( )
Our (3+1)-dim worldWilson loop C in our world
horizon
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r = r0
: area of string world sheet with boundary C.
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S(C)
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r = Λ
→ ∞
• Result for the quenching parameter
• AdS/CFT Recipe
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W A Clight−like( ) = exp −1
4ˆ q
L−
2L2
⎡
⎣ ⎢
⎤
⎦ ⎥= exp i2S Clight−like( )[ ]
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ˆ q SYM =π 3 / 2Γ 3
4( )Γ 5
4( )λ T 3 ≈ 26.68 α SYM Nc T 3 Liu, Rajagopal, Wiedemann,
Phys. Rev. Lett. 97:182301, 2006
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Nc = 3
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αSYM =1 2
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ˆ q SYM = 4.4 GeV 2
fm for T = 300 MeV
• “Numerology”: relate N=4 SYM to QCD by fixing
Is this comparison meaningful ?
Comment on: Is comparions meaningful?
• conformal
• no asmptotic freedom no confinement
• supersymmetric
• no chiral condensate
• no dynamical quarks, 6 scalar and 4 Weyl fermionic fields in adjoint representation
N=4 SYM theory
Physics near vacuum and at very high energy is very different from that of QCD
At finite temperature: Is comparions meaningful?
• conformal
• no asymptotic freedom no confinement
• supersymmetric (badly broken)
• no chiral condensate
• no dynamical quarks, 6 scalar and 4 Weyl fermionic fields in adjoint representation
N=4 SYM theory at finite T QCD at T ~ few x Tc
• near conformal (lattice)
• not intrinsic properties of QGP at strong coupling
• not present
• not present
• may be taken care of by proper normalization
In solid state physics, materials of different microscopic composition and interaction show similar thermal properties.Here: non-abelian gauge theories of different particle content and symmetries show similar thermal properties above Tc.
Is there a new form of “universality class” at high temperature?
QCD Saturation Physics:QCD at the highest parton densities
Venugopalan McLerran; Jalilian-Marian,Kovner,Leonidov,Weigert; Balitsky; Kovchegov;…
This requires that the action is large
Need weak coupling and strong fields, satisfied at sufficiently small Bjorken x,where hard processes develop over long distance
At highest , there is a qualitatively novel regime of QCD, in which
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sNN
• Parton densities are maximal up to large scales
• Coupling constant is small
• Semi-classical methods apply€
Q2 < Qsat2 ~ (2 − 3GeV )2
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ρ ~ 1 α s
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α s(Qsat2 >> ΛQCD )<<1
Can we test this novel QCD regime in the laboratory?
The kinematical range accessible
• Small x higher initial parton density qualitatively different matter produced at LHC mid-rapidity? tests of saturation phenomena? - bulk observables - pt-spectra in scaling regime - rapidity vs. dependence - …
• Large abundant yield of hard probes precise tests of properties of produced matter - color field strength - collective flow - viscosity - …
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Q2
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sNN
The Next-to-last Slide• This presentation was not comprehensive. I missed to mention: and how they relate to first principle calculations in a QFT:
- collective flow - transport coefficients, relaxation times - electromagnetic probes - spectral functions - rapidity and -dependence - saturated non-linear QCD evolution
• Instead of being comprehensive, I emphasized - how controlled experimentation with dense QCD matter is possible
- how the field makes progess in relating measurements to fundamental properties of matter calculable in QCD.
Abundant yield + robust signal + theory = understanding of hard probes (e.g. jet quenching >> uncertainties)
The RHICness of the LHC
Abundant yield of hard probes + robust signal (medium sensitivity
>> uncertainties)
= detailed understanding of dense QCD matter
• Jets• identified hadron specta• D-,B-mesons• Quarkonia• Photons• Z-boson tags
The probes:
The wide kin. range:
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Q2 ,x, A, luminosity QuickTime™ and aTIFF (LZW) decompressor
are needed to see this picture.