QCD at finite temperature and density on the lattice
Maria Paola Lombardo
INFN, Laboratori Nazionali di Frascati, Italy
Abstract. In the first lecture we briefly summarize the basics of field theory thermodynamics and critical phenomena. We then introduce the lattice gauge field theory approach to QCD at finite temperature and density, which is a non-perturbative scheme allowing first principle calculations using the QCD Lagrangian as a sole input. Some of the general concepts and idea introduced at the beginning are demonstrated by use of simple effective models of QCD. The second lecture is devoted to applications. We emphasize that current methods suffice to study the main phenomena at RHIC and LHC energies, and we discuss the ongoing theoretical efforts devoted to the solution of the sign problem which hampers the simulations of cold and dense matter. We conclude with short overview of the status of the field as of Summer 2008.
References
1. The Proceedings of Quark Matter, the International Conference on Ultrarelativistic Heavy Ion Collisions, usually include reviews on recent lattice results; the pro-ceedings of The International Symposium on Lattice Field Theoryusually include review on more specific aaspects of lattice thermodynamics.
2. M. P. Lombardo, Finite temperature field theory and phase transitions,arXiv:hep-ph/0103141. Lectures given at ICTP Summer School on Astroparticle Physics and Cosmology, Miramare, Trieste, Italy, 12 Jun - 7 Jul 2000. Published in *Trieste 2000, Astroparticle and Cos-mology*
3. F. Karsch,Lattice QCD at high temperature and den-sity, Lect. Notes Phys. 583, 209 (2002) [arXiv:hep-lat/0106019].
4. J. B. Kogut and M. A. Stephanov, The phases of quantum chromodynamics: From confinement to extreme Camb. Monogr. Part. Phys. Nucl. Phys. Cosmol. 21 (2004) 1.
© Owned by the authors, published by EDP Sciences, 2010 DOI:10.1051/epjconf/20100701004
EPJ Web of Conferences 7, 01004 (2010) 7
This is an Open Access article distributed under the terms of the Creative Commons Attribution-Noncommercial License 3.0, which permits unrestricted use, distribution, and reproduction in any noncommercial medium, provided the original work is properly cited.
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
0.0 0.5 1.0
T/0
0.0 0.5 1.0
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
d-dimensional space Imaginary time
and
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
0.4 0.8 1.2
0.8
0.4 0 0.5 1.0 T
m
μ
0.2 0.4 0.6
r=0.7 T=133MeV r=0.53
T=186MeV
r=0.43 T=216MeV 1.5
1.0
0.5
as
0 0.2 0.4 0.6 0.8 1 1.2
0 0.1 0.2 0.3 0.4 0.5
T/T
c
/Tc
q=0
q0
1st 2nd TCP w/o baryons
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
2 pi / 12 2 pi/24 T_c
Chiral transition
mu^2 T_E
Roberge Weiss critical line
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
0.80 0.85 0.90 0.95 1.00 1.05 1.10 1.15
T/TC
10 8 6 4 2 0 2 4 6
d
2M/d
2
S
0.40 0.45 0.50 0.55 0.60 0.65 0.70 0.75 0.80 0.85 0.90
0 50 100 150 200 250 300
frequency
<> for upd=0.0
0.10 0.20 0.30 0.40 0.50 0.60 0
50 100 150 200 250 300
frequency
<> for upd=0.625
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
Glasgow
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6
Pbp
Mu
Real mu (m.f.) Im mu (m.f.) Im mu (simulation)
-0.1 0 0.1 0.2 0.3 0.4 0.5 0.6
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8
Pbp
Mu
0.00 0.10 0.20 0.30
0.35 0.40 0.45 0.50
<L>
Imaginary data Imaginary data fit Analytic continuation Uncertain analytic continuation Real Data
Lattice:8x8x8x4
=2.0 m=0.07
0.00 0.10 0.20 0.30 0.40
0.060 0.070 0.080 0.090 0.100
<
>
Imaginary data Imaginary data fit Analytic continuation Uncertain analytic continuation Lattice:8x8x8x4
=2.0 m=0.07
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
0.2 0.3 0.4 0.5 0.6
0 0.2 0.4 0.6 0.8 1
T/S0
mu/S0
0 200 400 600 800
B/MeV
145 150 155 160 165 170 175 180 185
T/MeV
Nf=2, [3]
N
f=2+1, [1]
Nf=2, [2]
Helmholtz International Summer School
Dense Matter in Heavy Ion Collisions and Astrophysics
JINR Dubna Russia July 14–26 2008
QCD at nite temperature
and density
on the lattice
M.P. Lombardo, INFN Laboratori Nazionali di Frascati
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
HISS Dubna July 2008 MpL-QCD at nite T andμ
LATTICE FIELD THEORY : FIRST PRINCIPLE APPROACH TO THE QCD PHASE DIAGRAM
T
μB
Hadron Gas
CSC
QGP
QGP
PLAN
T μ μ B I Hadron Gas CSC ? Superfluid
1
2
3
4
4
QGP1. Critical line and Critical Point
2. EoS and Critical Behaviour
4. Cold and Dense Matter : QCD−like models 3. Towards FAIR
HISS Dubna July 2008 MpL-QCD at nite T andμ
T μ μ B I Hadron Gas CSC ? Superfluid 1 2 3 4 4 QGP
1.
T
c, THE CRITICAL LINE AND THE CRITICAL POINT
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
T
c
:
RBC-B
IELEFELD
100 150 200 250
140 160 180 200 220 240
T [MeV]
0.75*p4fat3
asqtad
HISS Dubna July 2008 MpL-QCD at nite T andμ
T
c
:
T
cAT
μ
B= 0
:
STATUS AS OF
QM2008
RBC-B
IELEFELD
:
T
c= 190(5)
MeV
W
UPPERTAL
-J
UELICH
:
T
c= 175(5)
MeV (Glue)
T
c= 151(6)
MeV (Fermions)
HISS Dubna July 2008 MpL-QCD at nite T andμ
T
HE
CRITICAL
LINE
IN
THE
μ
B, T
PLANE AT
SMALL
μ
BT
=
T
c−
Kμ
2BK
∝
1
/N
fHISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
Results for Nf=2+1 from gluonic and fermionic susceptibilities
Fodor, Guse, Katz, K ´alm ´an K. Szab ´o, QM2008
HISS Dubna July 2008 MpL-QCD at nite T andμ
HISS Dubna July 2008 MpL-QCD at nite T andμ
C
HALLENGING THE
C
RITICAL
E
NDPOINT OF
QCD
Forcrand-Philipsen : strategy
Scenario I or Scenario II ? To decide, measure slopeKin
m
c(
μ
)
m
c(0)
= 1 +
K
μ
T
2+
...
K >0: Scenario I , critical endpoint at smallμB
K <0: Scenario II, NO critical endpoint at smallμB: favored at QM2006
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
Kogut-Sinclair 2007 : QCD at nite isospin density
NB :μIμBatT TcToublan, Kogut, Sinclair 2004
m
c(
μ
)
m
c(0)
= 1
−
3
.
(1)
μ
IT
2
+
...
Current Results:
• Conrm unusual scenario forNt= 4
• Suggest NO critical endpoint forμB <600M eV • See talk by Philippe de Forcrand
HISS Dubna July 2008 MpL-QCD at nite T andμ
SU(3)L×SU(3)RNJL MODEL
60 80
100 120 140 160 180 100 200 300 400 500 0 100 200 300 400 500 600 700 800 900 1000
B [MeV]
m [MeV]
mK [MeV] B,CEP physical point diagonal B [MeV]
T μ μ B I Hadron Gas CSC ? Superfluid 1 2 3 4 4 QGP
2. EOS AND CRITICAL BEHAVIOUR
HISS Dubna July 2008 MpL-QCD at nite T andμ
LATTICE OBSERVABLES FOR THERMODYNAMICS
Number Density : accessible atimaginary chemical potential.
nu,d(T , μu, μd, mu, md) =∂p(T , μu, μd)
∂μu,d ;p(T , μu, μd) = T
VlnZ(T , μu, μd)
Susceptibilities: accessible atatμ= 0
χju,jd(T) =∂
(ju+jd)p(T , μu, μd)
∂μjuu ∂μjdd
μu=μd=0
.
Test for uctuations.
Taylor coefcients of the excess pressure:
Δp(T , μu, μd)≡p(T , μu, μd)−p(T , μu= 0, μd= 0) =ju,jdχju,jd(T)μ
ju u ju!
μjd d jd!,
containing information about baryon density effects in the EoS.
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
Temperature
Real 2
QGP Hadron Gas Endpoint RW and Chiral
Chiral Transition Roberge Weiss Transition = 0
• In the critical region:
p(T , μ)
=b(T)|t+a(T)(μ2−μ2c)|(2−α)
implying
n(T , μ) =
A(T)μ(μc2−μ2)(2−α)
• High Temperature, away from critical line
Approach to Free Field
n(T , μ)→nSB(T , μ)
HISS Dubna July 2008 MpL-QCD at nite T andμ
HADRON GAS; CRITICAL BEHAVIOUR; SB from SUSCEPTIBILITIES
0 0.5 1 1.5 2
150 200 250 300 350 T [MeV]
<B4>-3<B2>2 <B2>
SB nf=2+1, m=220 MeV
nf=2, m=770 MeV
Resonance gas
1.5
2 <Q4>-3<Q2>2 <Q2>
nf=2+1, m=220 MeV
nf=2, m=770 MeV
Resonance gas 0 0.5 1 1.5 2 2.5 3
50 100 150 200 250 300 350 400 450 T [MeV]
<S4>-3<S2>2 <S2>
SB nf=2+1, m=220 MeV
Resonance gas
CRITICAL BEHAVIOR AND THERMODYNAMICS AT THE ENDPOINT OF THE RW TRANSITION
Critical behavior at imaginaryμ n(μI) =A(T)μI(μc2−μ2I)(2−
α) -0.08 -0.07 -0.06 -0.05 -0.04 -0.03 -0.02 -0.01 0 0.01
0 0.05 0.1 0.15 0.2 0.25 0.3
n
I
Data All data, open critical point >0.15, constrained critical point
Continued to realμ..
n(μ) =A(T)μ(μc2+μ2)(2−α)
nSB(μ) =Aμ+Bμ3)→α= 1
0 0.5 1 1.5 2 2.5 3
0 0.2 0.4 0.6 0.8 1
n(
)
Analytic Continuation
Stephan Boltzmann
D’Elia, Di Renzo, Lombardo, 2007, QM2008
HISS Dubna July 2008 MpL-QCD at nite T andμ
CRITICAL BEHAVIOR, THERMODYNAMICS, QUASIPARTICLE MODELS K ¨ampfer, Bluhm Proposal
amenable to an easy comparison with lattice data.
I. Quasiparticlemodel vs Imaginary Chemical Potential Lattice Data, and analytic continuation to Real Chemical Potential
0 0.5 1 1.5
/ T 0 0.5 1 1.5 2 2.5
n / T
i
3
c
0 0.5 1 1.5
/ T 0 0.5 1 1.5 2 2.5 3 3.5 4
n / T
3
c
K ¨ampfer, Bluhm , 2007, QM2008
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
0.8 1 1.2 1.4 1.6 1.8 2 T/T
0 0.05 0.1
c4Q
c
0.8 1 1.2 1.4 1.6 1.8 2 2.2 T/T 0 0.2 0.4 c Crucial ingredients:
• Explicit dependence of the self-energy parts onμi=μu,dandT
• Implicit dependence via the effective couplingG2(T , μu, μd).
ω2i=k2 +m2i+ Πi, Πi=13
⎛ ⎝T2 +μ
2
i π2
⎞
⎠G2(T , μu, μd).
K ¨ampfer-Bluhm : see Poster
HISS Dubna July 2008 MpL-QCD at nite T andμ
APPROACH TO SB : ANALYTIC RESULTS VS. LATTICE DATA Based on A. Vuorinen, 2004
0.00 0.02 0.04 0.06 0.08 0.10
Μ Tc 0.88 0.90 0.92 0.94 0.96 N NSB
0.00 0.02 0.04 0.06 0.08 0.10
Μ Tc 0.90 0.92 0.94 0.96 0.98 N NSB
T
= 1
.
5
T
c—————————-
T
= 3
.
5
T
c
T
μ
μ
B
I
Hadron Gas
CSC
? Superfluid
1
2
3
4
4
QGP
3. TOWARDS FAIR
HISS Dubna July 2008 MpL-QCD at nite T andμ
STRONG COUPLING
New Results on The Mass Spectrum
Kawamoto, Miura 2007
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
T
phys/Tc= 6T/Tc
( phys
0.5 1/3 0.6 0.4 2 3 0.7 0.8 0.9 5.75 5.62 5.50 5.55 5.70 5.67 5.65 5.80 5.85 1.0 0.95 0.9 0.85 0.8 0.75 0.7 = 0.4
( 2.4 ) ( 3.0 )
0.5 0.6
( 3.6 )
( 4.2 )
( 4.5 )
( 4.8 )
( 5.1 )
( 5.4 )
( 5.7 )
( 6.0 )
5.72
5.60
A B
———–
μ
BResults forNf = 3:
• Identied phase transition • Indentied Ridge in the T,μplane • Studies of diquark in progress Di Pietro, Feo, Seiler, Stamatescu 2008
HISS Dubna July 2008 MpL-QCD at nite T andμ
CANONICAL FORMALISM
ZC(T , N) =
3
2π
2πT
0 d(μI/T)e−N iμI/TZGC(T , iμI) Forcrand and Kratovchila, 2006,2007 Canonical partition a la Hasenfratz-Toussaint:
ZC(B,β)
ZGC(β0=β,μ=iμI0)
=1
2π
π
−π d
μI
T
e−i3B μI
T det(U;iμI)
det(U;iμI0)β0,iμI
0
≡ det(ZCˆ U(U;;B)
iμI0)β0,iμI
0
Results forNf= 4:
• First order line-coexistence region • Criticalμand Critical densities→
0.6 0.8 1 1.2 1.4
0 2 4 6 8 10 12 14 16 0 1 2 3 4 5
/T
Baryon number /T3
1 2
T/Tc = 0.92 /T=1.06(2) Weakly interacting massless gas
0 5 10 15 20 25 30
0 0.5 1 1.5 20 1 2 3 4 5 6 7 8
Baryon number B
/T
3
/T = (F(B)-F(B-1))/3T T/Tc = 0.92
Saddle point approximation
CANONICAL APPROACH II : HISTOGRAMS Proposed by Ejiri,2007
Alternative search for a critical point inNf= 2QCD, large masses
Alexandru, Li, Liu, 2007 :
0 5 10 15
2 3 4 5 6 7 ke Μ T 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10 1.31.41.51.61.7 0 2 4 6 8 10
Β 5.22
Β 5.20
HISS Dubna July 2008 MpL-QCD at nite T andμ
CANONICAL APPROACH III :
Grand Partition Function via a Taylor Expansion. Ejiri, 2007,2008
ZGC(T ,μq)
ZGC(T ,0) ≡
e
NfNtV∞n=1Dn
μq
T
n
(T ,μq=0),
ZC(T ,ρV¯ )
ZGC(T ,0)at large V≈
expVNfNtn∞=1Dnzn0−ρz¯0
e−iα/2
1
V|D(z0)|
(T ,μ=0)
Results forNf= 2:
• Qualitative change atT /Tc0.8 • Indication of First Order Line Ejiri 2008
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
Density of states –ρ– constrained partition function:
ρ(x) = DU g(U)δ(φ−x).
Results forNf = 4
• Signal of two phase transition lines
• Indication for a triple point
Fodor, Katz, Schmidt 2007 90
100 110 120 130 140 150 160 170
0 50 100 150 200 250 300 350 400 q [MeV]
[MeV] multiparameter reweighting
DOS method, am=0.05
DOS method, am=0.03
HISS Dubna July 2008 MpL-QCD at nite T andμ
T μ μ B I Hadron Gas CSC ? Superfluid 1 2 3 4 4 QGP
TWO COLOR QCD
• Symmetry :qq←→qq¯
• Symmetry :μB←→μI • At T=0 μcB=μcI =mπ/2 • Diquark Condensate forμB> μcB • Pion Condensate forμB> μcI • No sign problem
HISS Dubna July 2008 MpL-QCD at nite T andμ
QCD atμI= 0and TWO COLOR QCD atμB= 0 No sign problem, many studies!
• Low Temperature, Fermionic Sector
– Strong coupling analysis [Dagotto, Karsch, Moreo,Wollf, 1986]
– Laboratory for diquark condensation [Alford,Rajagopal and Wilczek; Rapp, Sch ¨afer, Shuryak and Velkovsky, 1998]
– Numerical studies of symmetries and spectrum [Hands, Kogut, Morrison, MpL 1998]
– Lattice studies of diquark condensation [Hands, Kogut, Morrison, Sinclair;1998; Aloisio, Azcoiti, di Carlo, Galante, 1999]
– RMT analysis [Akemann, Splittorff, Toublan, Verbaarschot,2001] – Studies of the Dirac spectrum [Bittner, Markum, Pullirsch, MpL, 2001]
– μc(T= 0) =mπ/2: amenable toχPT analysis.
[Kogut, Stephanov, Toublan, Verbaarschot and Zhitnitsky, 2001; Kogut, Toublan, Sinclair 2002]
– EoS and Gluon Condensate fromχPT [Metlitsky,Toublan,Zhitnisky, 2005,2006]
– Model studies of the vector sector [Lenaghan, Sannino, Splittorff 2002]
– Vector spectroscopy on the lattice [Alles, D’Elia, Pepe, MpL, 2001; Muroya,Nakamura,Nonaka, 2003]
– Test Bed for Imaginaryμ[Cea, Cosmai, Giudice, D’Elia, Papa, 2006, 2007]
• High T , Gluon Sector niteμtransition from hadron gas to QGP, similar to the T=0 transition
– Critical Line [Kogut, Sinclair, 2003-2008]
– Topological Susceptibility [ Alles, D’Elia, Pepe, MpL 2002] – Polyakov Loop [Muroya,Nakamura, 2004; Alles, D’Elia, MpL 2006] – Order Parameter for Conement [D’Elia Conradi 2007] – Critical Line [Forcrand, Stephanov, Wenger, 2007]
• Low T : Chiral Symmetry , Connement, BEC Phase
– Connement/Deconnenement,Screening [Hands, Kim, Skullerud 2006–2008] – Glueballs spectrum, screening [Lombardo, Paciello, Petrarca, Taglienti, 2007] – BEC Phase, interface BEC/QGP [Forcrand, Stephanov, Wenger, 2007]
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
4.4 4.5 4.6
0 1 2 3 4
I/T
1 1.5 2 2.5
0 1 2 3 4 5
I/T 0.7 0.6 0.5 T/T c BEC
m/T
Binder cumulant
Forcrand, Stephanov, Wenger, 2007
HISS Dubna July 2008 MpL-QCD at nite T andμ
GLUONIC OBSERVABLES IN THE BEC PHASE of QC2D
0++Glueball : lighter in the BEC phase
Susceptibility:χ=< P2>−< P >2peaks atμc
Normal Phase
mπ/mρ m++0 /mρ
BEC AND CONFINEMENT: deconnement deep in the BEC phase
0.2 0.4 0.6 0.8 1
0 0.2 0.4
<qq>/2 4<L>
Hands, Kim, Skullerud 2006,2007
HISS Dubna July 2008 MpL-QCD at nite T andμ
DECONFINEMENT IN THE BEC PHASE – BEC/BCS crossover
0.2 0.3 0.4 0.5 0.6 0.7 0.8
0 0.5 1 1.5 2 2.5 3
nq/nSB
pII/pSB
0.2 0.3 0.4 0.5 0.6 0.7 0.8
0 5 10 15 20
q/SB nq/nSB p/pSB
Hands, Kim, Skullerud 2008; preliminary, courtesy S. Hands
HISS Dubna July 2008 MpL-QCD at nite T andμ
Dense Matter In Heavy Ion Collisions and Astrophysics (DM2008)
From SmallNc= 2to
Large
N
c: Proposed Phase Diagram
McLerran, Pisarski, 2007
HISS Dubna July 2008 MpL-QCD at nite T andμ
QCD AT FINITE TEMPERATURE AND DENSITY : SUMMARY
Tcknown within 20 % .
Fate of the critical endpoint of QCD???
Smallμ: Mature calculations. Critical line towards continuum Mass spectrum depends onμB
Critical line at lower temperature, largerμ’bends down’ First evidences of a triple point in the T,μBplane
Cold Phases studied atμI= 0/ QC2D atμB = 0
Examples of interesting patterns connement/chiral symmetry.
Critical region needs exact dynamics, models do not sufce