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Deconfinement transition from “perturbationtheory”
M. Pelaez, U. Reinosa, J. Serreau, M. Tissier, A. Tresmontant,N. Wschebor
Ilha bela, September 2015
Deconfinement transition ...
Introduction
Yang-Mills theory, gauge-fixed in the Landau gauge with theFaddeev-Popov procedure, is described by a set of massless fields:Gluons (Aa
µ), ghosts (ca and ca) and a Lagrange multiplyer (ha)
L =1
4(F a
µν)2 + ∂µc
a(Dµc)a + ha∂µA
aµ
However, lattice simulations see unambiguously a gluon propagatorthat saturates at low momentum.
Deconfinement transition ...
However...
Gluon propagator is massive! (Sternbeck et al ’07)!
0.001 0.01 0.1 1 10 100
q2[GeV
2]
0
5
10
15
20
D(q
2 )
L=64, 14 confsL=72, 20 confsL=80, 25 confs
Gluon propagatorL = 64, 72, 80, SA
The origin of the mass could:
result from solving Dyson-Schwinger equations;
be a consequence of a gluon condensate;
be related to Gribov ambiguity;
none of those...Deconfinement transition ...
Phenomenological model
The mass generation is a difficult issue. Once we are convinced itexists, how much physics can we understand?Introduce a mass for the gluon by hand in the (gauge-fixed)Lagrangian:
L =1
4(F a
µν)2 + ∂µc
a(Dµc)a + ha∂µA
aµ +
1
2m2
(
Aaµ
)2
(Here, we make the assumption that no extra field is needed)This is one particular representative of the Curci-Ferrari lagrangian.
Deconfinement transition ...
Overview
Motivate the interest of this phenomenological model.
General arguments;Systematic comparison with Lattice correlation functions.
Applications to finite temperature physics
in the quenched approximation;with dynamic quarks, with and without chemical potential.
Deconfinement transition ...
Nice properties of the model I
UV (p ≫ m) properties are unaffected by the gluon mass.
In particular, the theory is renormalizable to all orders (DeBoer et al). (gluon mass softly breaks the BRST symmetry)
the (running) gluon mass tends to zero in the ultraviolet(m(µ) ∝ gα(µ) with α > 0).
Feynman rules are identical to usual ones, except for themassive gluon propagator:
〈AµAν〉0(p) =(
δµν −pµpν
p2
)
1
p2 +m2
perturbation calculations are easy to perform.
Low momentum physics regularized by the gluon mass.
Deconfinement transition ...
Infrared behavior
At very low momenta, gluons are frozen. Ghost loop dominates.
ΓAaµA
bν∼ δab(δµν)p
d−2
ΓAaµA
bνA
cρ∼ −f abc(ipµδνρ + · · · )pd−4
in d = 4, leads to log divergences, hard to see...in d = 3, gluon propag cte + |p|, 3-gluon vertex changes sign,consistent with lattice data.Interaction between ghosts is mediated by heavy gluons (seealso Weber). Effective interaction is suppressed by somepositive power of p at low momentum.
Par
amet
er e
xpan
sion
0
0.2
0.4
0.6
0.8
1
1.2
1.4
1.6
0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
µ (GeV)
Deconfinement transition ...
Ghost and gluon propagators
Need to compute 4 Feynman diagrams
Define 〈AµAν〉(p) =(
δµν − pµpνp2
)
G (p) 〈cc〉(p) = 1p2F (p).
Introduce 4 renormalization parameters and you get (s = p2/m2.):
G−1(p)/m2 = s + 1 +g2N
384π2s{
111s−1 − 2s−2 + (2− s2) log s
+ (4s−1 + 1)3/2(
s2 − 20s + 12)
log
(√4 + s −√
s√4 + s +
√s
)
+ 2(s−1 + 1)3(
s2 − 10s + 1)
log(1 + s)− (s → µ2/m2)}
,
F−1(p) = 1 +g2N
64π2
{
− s log s + (s + 1)3s−2 log(s + 1)− s−1 − (s → µ2/m2)}
,
Deconfinement transition ...
Comparison with lattice data
For SU(2) (Cucchieri, Mendes ’08)
0
0.5
1
1.5
2
2.5
3
3.5
4
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2
G(p
)
p (GeV)F
(p)
p (GeV)
0
0.5
1
1.5
2
2.5
3
3.5
4
4.5
0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2
Deconfinement transition ...
Renormalization-group flow
From renormalization factors, deduce a set of coupled β functionsfor g and m:
In the UV (µ≫ m) βg ≃ − g3N16π2
113
In the IR (µ≪ m) βg ≃ + g3N16π2
16
For SU(3) (Bogolubsky ’09, Dudal ’10)
p G
(p)
2
p (GeV)
0
0.5
1
1.5
2
2.5
0 1 2 3 4 5 6 7 8
F(p
)
p (GeV)
0
2
4
6
8
10
12
14
0 1 2 3 4 5 6 7 8
Deconfinement transition ...
Other correlation functions
By the same technique, we have computed (all tensorialcomponents) and compared with lattice data, when available:
3 gluon vertex and ghost-gluon vertex;quark propagator;quark-gluon vertex;
Agreement (Maximal error of 15-20%) in the quenchedapproximation.
In unquenched calculations (Skullerud et al), still ok, but lessprecise, because the quark-gluon vertex is larger (typically thedouble of the ghost-gluon vertex).
1-loop compares badly to lattice for the quark renormalizationfactor and for one of the structure tensors of the quark-gluonvertex (λ2).
Deconfinement transition ...
Quark mass
The quark mass is enhanced in the infrared. But no chiralsymmetry breaking.
0 1 2 3 4 5
0.05
0.10
0.15
0.20
0.25
0.30
p HGeVL
MHpLHG
eVL
Deconfinement transition ...
Quark-gluon vertex
0 1 2 3 4 5 6
0.6
0.8
1.0
1.2
1.4
1.6
1.8
2.0
p HGeVL
Λ1H
pL
Deconfinement transition ...
The phase diagram of QCD I
In heavy ion collisions, and core of neutron stars, matterreaches extreme conditions, with temperatures of the order of∼ 1012 K, densities of ∼ 1018 kg/m3.
Typical values for strong interactions. In strong interactionsunits: T ∼ 1 GeV, ρ ≃ 1 GeV/fm3.
In the quenched approximation (no dynamic quarks), latticesimulations clearly show a phase transition at a temperature∼ 250 MeV, which is in the nonperturbative regime.
Extension to finite chemical potential is intricate because theaction is not real anymore.
Deconfinement transition ...
Phase diagram of Yang-Mills II
To study the theory at finite temperature, compactify thetime direction, with periodicity β = 1/T .
There exist gauge transformations A → AU such that AU isperiodic, although U itself is not: U(β, x) = z U(0, x) with z
an element of the centre (for SU(N), z = e imπ/NI with
m ∈ {0, · · · ,N − 1}).Some quantities are invariant under the centre (such as F 2
µν).Other vary, such as the Polyakov loop
ℓ ∝ Tr Pe ig∫ β
0 A0(τ)dτ
〈ℓ〉 = exp(−βFq) where Fq is the free energy of a quark.
If the centre symmetry is realized, 〈ℓ〉 = 0, Fq = ∞, confinedphase.If the centre is spontaneously broken, 〈ℓ〉 6= 0, Fq finite,deconfined phase.
Deconfinement transition ...
Phase diagram of Yang-Mills III
To encode the centre symmetry, convenient to
decompose the gluon field in a background A and afluctuating a field: A = A+ a (we choose A constant,temporal, in the Cartan subalgebra);
introduce the Landau-de Witt gauge ∂µaµ + gf abc Abµa
cµ = 0;
choose A such that 〈a〉 = 0.
This last condition is fulfilled by minimizing some potential V (A).Center transformations act on A!At leading order in g , the SU(2) potential reads (r3 = βgA3)
V = T 4
(
3
2Fmβ(r3) +
1
2F0(r3)− 1F0(r3)
)
+O(g2)
Fm(r) =
∫
q
log(1 + e−2√
m2+q2 − 2e−√
m2+q2 cos(r))
The Polyakov loop:
〈ℓ〉 = cos(r3/2) +O(g2)
Deconfinement transition ...
Phase diagram of Yang-Mills IV
At high temperatures (red), V → +1F0(r3). (Weiss potential)At low temperatures (blue), V → −1
2F0(βgA).
−0.8
−0.4
0
0.4
0 π/2
VSU(2)(r)
πr
0.08
0.12
0.04
0
−0.040
VSU(2)(r)
π/2 π
r
r = π is invariant under center transformations and corresponds to〈ℓ〉 = 0.The leading order approximation captures the good physics!
Deconfinement transition ...
Pressure I
0.1 0.2 0.3
0.01
0
0
0.001
0 0.2 0.4T 1lcT (GeV)
p (GeV−4)
T 2lc
Deconfinement transition ...
Pressure II
0
0.1
0.2
0.3
0.1 0.2 0.3 0.4
p/T 4
T (GeV) T 1lc T 2l
c
π2
120
Deconfinement transition ...
Phase diagram for SU(3) I
Two fields in the Cartan subalgebra: r3 and r8.
0
r3
2π−2π
0
−4π 4π
r8
4π√3
− 4π√3
Calculation of the potential and Polyakov loop generalizes easily.
Deconfinement transition ...
Phase diagram for SU(3) II
Leads to first order transition
2.8 3 3.2 3.4 3.6 3.8
V
r3
Deconfinement transition ...
Finite chemical potential
Add the quarks lagrangien density, with chemical potential:
∑
f
ψf ( /D +Mf + µγ0)ψf
Explicitely break centre symmetry.
Contributes to the potential as:
Vf (µ) = − T
π2
∫
∞
0dq q2
{[
log[1 + e−β(√
q2+M2f+µ)
]
+ (µ→ −µ)}
+O(g2)
Deconfinement transition ...
Vanishing chemical potential, SU(3)
Consider 2 +1 quarks (only for large mass because we don’tcontrol chiral limit). Columbia plot:
1 0.9 0.8 0.8
0.9
1
Crossover
1st order
1− e−Msm
1− e−Mum
Deconfinement transition ...
Imaginary chemical potential, SU(3)
The action and potential V are real, so lattice simulations canbe performed.
It is symmetric under a simultaneous transformation of thebackground field and of the chemical potential (Roberge,Weiss). µ/T = iπ/3 plays a particular role:
We retrieve the properties obtained in Lattice approaches (deForcrand, Philipsen), in particular at the tricritical point.
Deconfinement transition ...
small quark mass
0.38
0.36
0.34
0.32
µi/Tπ/3 2π/30
T/m
Deconfinement transition ...
intermediate quark mass
0.36
0.340
µi/Tπ/3 2π/3
T/m
Deconfinement transition ...
large quark mass
0.36
0.3480 π/3 2π/3
µi/T
T/m
Deconfinement transition ...
Real chemical potential
For real background fields, the potential is complex!
To be consistent, need to choose r3 real and r8 imaginary (Seealso Nishimura 2014). Then the potential is then real.
0.8
0.9
1
0.8 0.9 1
1− e−Ms
m
1− e−Mu
m
2
1
0 0.36 0.38
T/m
Fq/m
Fq/m
Deconfinement transition ...
Conclusions
Curci-Ferrari seems to capture many “nonperturbative”properties of QCD within “perturbation theory”.
This would mean that the major nonperturbative ingredient isthe gluon mass.
We have a nice model to study low-energy properties of QCD.Tested in several situations.
Propagators in the Landau-de Witt gauge.Chiral symmetry breaking?Polyakov loop in other representations?Analytic structure of the correlation functions?Wilson loop?Two-loop calculations for the propagators?Transport coefficients?...
Can we generate the mass from first principles (relation withproblems with disorder in stat. phys.)?
Can we build a physical subspace?
Deconfinement transition ...