The Functional Renormalization Group...The Functional Renormalization Group Andrea Coser SISSA -...
Transcript of The Functional Renormalization Group...The Functional Renormalization Group Andrea Coser SISSA -...
The Functional Renormalization Group
Andrea Coser
SISSA - ISAS
Introduction to the Functional RG
14/09/2012
Outline Universality Wilson RG The EAA method A computation
Outline
1 Critical phenomena and universalityCritical exponentsThe scaling hypothesis
2 The Wilson approach to RenormalizationThe RG flowThe RG flow: around the Fixed Point
3 Functional RG: the EAA methodThe Effective Average ActionThe cutoff functionThe exact RG equation
4 Computation of critical exponents in the O(N) model
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Critical phenomena and universality
Phase transitions:
• magnetic system, liquid-gas transition
• non-analyticity of the thermodynamicpotential
• first or second order
P
T
Pc
Tc
solid
gas
liquidC
Second order phase transition −→ different symmetries in the two phases−→ order parameter−→ critical phenomena
Universality:
some properties near the critical point appear to be the same for very differentphysical systems
the behavior is rather independent of the microscopical details (interactionsbetween particles)
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Critical exponents
Critical Exponents:
Definitions: near the critical point (t = (T − Tc)/Tc)
• specific heat: C ∼ |t|−α
• order parameter (B = 0): m ∼ |t|β
• susceptibility: χ ∼ |t|−γ
• order parameter (t = 0): m ∼ |h|1δ
• correlation function: G(r , t) =G±(r/ξ(t))
rd−2+η
• correlation length: ξ ∼ |t|−ν
Scaling relations (experimentally verified):
γ = ν (2− η) Fisher
β =1
2(2− α− γ) Rushbrooke
γ = β (δ − 1) Widom
α = 2− νd Josephson
0.10.005 0.01
reduced temperature
0.02 0.05 0.1
0.2
0.3
0.4
0.5
0.6
ma
gn
eti
zati
on
15
Figure: magnetization in nickelit is found β = 0.358
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Critical exponents
Example: gas-liquid coexistence region
−→ critical points are very different
−→ reduced quantities lie on the same curve: universality → β = 1/3
00.55
0.60
0.65
0.70
0.75
0.80
0.85
0.90
0.95
1.00
0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6 1.8 2.0 2.2 2.4 2.6
ρ/ρc
T/T
c
Ne
A
Kr
Xe
N2
O2
CO
CH4
13
Figure: Guggenheim, J. Chem. Phys. 13, 1945
Tc (C) Pc (atm)
Ne -228.7 26.9Ar 1122.3 48Kr -63.8 54.3Xe 16.6 58N2 -147 33.5O2 -118.4 50.1CO -140 34.5CH4 -82.1 45.8
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The scaling hypothesis
Scaling hypothesis: at the critical point the correlation lengthis the only characteristic length of the system
Consequences: free energy: f (t, h) ∼t∼0h∼0
|t|2−αF±(
h
|t|∆
)
1 similar scaling laws for the otherquantities
2 scaling relations among exponents
m(t, h) = |t|2−α−∆M±(h/|t|∆
) β = 2− α−∆
∆ = βδ
χ(t, h) = |t|2−α−2∆χ±(h/|t|∆
)−γ = 2− α− 2∆
f (t, 0) ∼ ξ−d ∼ |t|νd νd = 2− α
χ =
∫dd r G(r , t) γ = ν(2− η)
−0.2 0 0.2
80
Cp (
J/m
ole
K)
100
120
T − Tλ (µK)
68
Figure: specific heat at the superfluidtransition in 4He
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The Wilson approach to Renormalization
Critical point ξ →∞:
• fluctuations on all wavelengths
• ξ a ∼ Λ−1: short distance details are washed out
Idea: build an effective theory for the long distance degrees of freedom
Implementation: Coarse graining + rescaling −→ RG transformation
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The Wilson approach to Renormalization
Critical point ξ →∞:
• fluctuations on all wavelengths
• ξ a ∼ Λ−1: short distance details are washed out
Idea: build an effective theory for the long distance degrees of freedom
Implementation: Coarse graining + rescaling −→ RG transformation
Z =∑σi
e−H(σi,~K) =∑σB
∑σi∈B
e−H(σi,~K) ≡∑σB
e−H(σB,~K ′)
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The Wilson approach to Renormalization
Critical point ξ →∞:
• fluctuations on all wavelengths
• ξ a ∼ Λ−1: short distance details are washed out
Idea: build an effective theory for the long distance degrees of freedom
Implementation: Coarse graining + rescaling −→ RG transformation
Z =
∫ Λ
Dφ(p) e−H[φ,~K ] =
∫ Λ/s
Dφ<
[∫ Λ
Λ/sDφ> e−H[φ<,φ>,~K ]
]=
∫ Λ
Dφ′(p′) e−H[φ′,~K ′]
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Coarse graining + rescaling −→ RG transformation
Effects of RG transformation:
• probe the system at different scales
• flow in parameter space ~K → ~K ′ = ~T(~K , s
)(∞-dimensional)
−→ flow in the space of theories
• dimensionless correlation length: ξ =ξ
a
a→ s a ⇒ ξ′ =ξ
s
ξ when s : the coarse grained system is less critical
ξ ∼ |T − Tc |−ν −→ t increases
• ξ =∞ ⇒ ξ′ =∞ −→ the system is still critical
critical surface: set of points with ξ =∞ −→ co-dimension 1
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The RG flow
Fixed point:
~K∗ = ~T(~K∗, s
)
Hypothesis:~Kc in a domain of the critical surface:the flow converges to the fixed point
→ all the theories in the basin of attraction belong to the same universality class
~K0 near the critical surface:the flow get close to ~K∗ and then leave
−→ universality
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The RG flow
Fixed point:
~K∗ = ~T(~K∗, s
)
Hypothesis:~Kc in a domain of the critical surface:the flow converges to the fixed point
→ all the theories in the basin of attraction belong to the same universality class
~K0 near the critical surface:the flow get close to ~K∗ and then leave
−→ universality
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The RG flow: around the Fixed Point
Infinitesimal RG transformation −→ beta function∂~Ks
∂ ln s=∂~T
∂s
∣∣∣∣~Ks ,1
≡ ~β(~Ks)
Linearization around the FP: δ~Ks = ~Ks − ~K∗
sd~Ks
ds=
d~β
ds
∣∣∣∣~K∗︸ ︷︷ ︸
stabilitymatrixMij
·δ~Ks +O(δ~K 2
s
)
• scaling directions: eigenvectors of M −→ M~φi = λi~φi
• scaling fields: projection of δ~Ks on ~φi vi (s) =∑α
δKs α φαi
→ not mixed by RG transformations: sdvids
(s) = λivi (s) ⇒ vi (s) ∝ sλi
(a) λi > 0: relevant coupling −→ temperature
(b) λi < 0: irrelevant coupling
(c) λi = 0: marginal coupling
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The RG flow: around the Fixed Point
RG transformation for the free energy: f (~K)→ s−d f (~K ′)
f (t, h, v2, . . . ) = s−d f (sλt t, sλhh, sλ3v2, . . . )
choosing s = |t|−1/λt we get
scaling relations:
f (t, h) = |t|dλt f
(±1,
h
|t|λh/λt, 0, . . .
)= |t|
dλt F±
(h
|t|λh/λt, 0, . . .
)
we can compute
critical exponents:
2− α =d
λt∆ =
λh
λt
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Functional RG: the EAA method
The Effective Action formalism:
• partition function −→ generator of correlation functions
Z [J] =⟨eJφ⟩
=
∫Dφ e−H[φ]+
∫x J(x)φ(x) 〈φ(x1)φ(x2)〉 =
δ2Z [J]
δJ(x1)δJ(x2)
∣∣∣∣J=0
• connected correlation generating function
W [J] = log⟨eJφ⟩
〈φ(x1)φ(x2)〉c =δ2W [J]
δJ(x1)δJ(x2)
∣∣∣∣J=0
• Effective action (Gibbs free energy)
Legendre transform:ϕJ ≡ 〈φ〉J ⇒ Jϕ = J[ϕ]
Γ[ϕ] = Jϕϕ−W [Jϕ]
(i) function of ϕ, which has a physical interpretation
(ii) generates 1PI graphs
(iii)
(δΓ
δϕδϕ
)−1
x1 x2
=δW
δJ(x1)δJ(x2)
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Functional RG: the EAA method
The Effective Action formalism:
• partition function −→ generator of correlation functions
Z [J] =⟨eJφ⟩
=
∫Dφ e−H[φ]+
∫x J(x)φ(x) 〈φ(x1)φ(x2)〉 =
δ2Z [J]
δJ(x1)δJ(x2)
∣∣∣∣J=0
• connected correlation generating function
W [J] = log⟨eJφ⟩
〈φ(x1)φ(x2)〉c =δ2W [J]
δJ(x1)δJ(x2)
∣∣∣∣J=0
• Effective action (Gibbs free energy)
Legendre transform:ϕJ ≡ 〈φ〉J ⇒ Jϕ = J[ϕ]
Γ[ϕ] = Jϕϕ−W [Jϕ]
(i) function of ϕ, which has a physical interpretation
(ii) generates 1PI graphs
(iii)
(δΓ
δϕδϕ
)−1
x1 x2
=δW
δJ(x1)δJ(x2)
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The Effective Average Action
Effective Average Action Γk[ϕ]:
Gibbs free energy of the rapid modes that have been integrated out
k ≤ p ≤ ΛΛ : UV cutoff of the original theory
k : IR cutoff → running parameter
RG flow−−−−→
One parameter family of functionals:
1 k = Λ ⇒ original Hamiltonian: Γk=Λ[ϕ] = H[ϕ]
2 k = 0 ⇒ full Gibbs free energy: Γk=0[ϕ] = Γ[ϕ]
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The cutoff function
Implementation:
decouple the slow mode giving them a large mass→ cutoff function Rk(q2)
Zk [J] =
∫Dφ exp
(−H[φ]−∆Hk [φ] +
∫Jφ
)∆Hk [φ] =
1
2
∫q
Rk(q2)φqφ−q
(a) k = 0 → Rk=0(q2) = 0 ∀q
(b) k = Λ → Rk=Λ(q2) = Λ2 ∀q
(c) 0 < k < Λ → Rk(q2 > k2) ' 0
Rk(q2 < k2) ' k2
k2
q2
k2
Rk(q2)
k2
q2
______
eq
2/k
2
-1(k
2-q
2)θ(k
2-q
2)
Cutoff function Rk(q2)
−→ Γk [ϕ] + Wk [J] =
∫Jϕ−
1
2
∫qRk (q2)ϕqϕ−q
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The cutoff function
Implementation:
decouple the slow mode giving them a large mass→ cutoff function Rk(q2)
Zk [J] =
∫Dφ exp
(−H[φ]−∆Hk [φ] +
∫Jφ
)∆Hk [φ] =
1
2
∫q
Rk(q2)φqφ−q
(a) k = 0 → Rk=0(q2) = 0 ∀q
(b) k = Λ → Rk=Λ(q2) = Λ2 ∀q
(c) 0 < k < Λ → Rk(q2 > k2) ' 0
Rk(q2 < k2) ' k2
k2
q2
k2
Rk(q2)
k2
q2
______
eq
2/k
2
-1(k
2-q
2)θ(k
2-q
2)
Cutoff function Rk(q2)
−→ Γk [ϕ] + Wk [J] =
∫Jϕ−
1
2
∫qRk (q2)ϕqϕ−q
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The exact RG equation
Exact RG equation for the EAA:
∂kΓk [ϕ] =1
2
∫q
∂kRk(q2)(
Γ(2)k [ϕ] +Rk
)−1
q,−q
Rk (q, q′) =
(2π)dδ(q + q′)Rk (q2)
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The exact RG equation
Exact RG equation for the EAA:
∂kΓk [ϕ] =1
2
∫q
∂kRk(q2)(
Γ(2)k [ϕ] +Rk
)−1
q,−q
Rk (q, q′) =
(2π)dδ(q + q′)Rk (q2)
Properties:
• integral equation
• differential equation
• non-linear equation
• IR finite
• UV finite
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The exact RG equation
Exact RG equation for the EAA:
∂kΓk [ϕ] =1
2
∫q
∂kRk(q2)(
Γ(2)k [ϕ] +Rk
)−1
q,−q
Rk (q, q′) =
(2π)dδ(q + q′)Rk (q2)
Properties:
• integral equation
• differential equation
• non-linear equation
• IR finite
• UV finite
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The exact RG equation
Exact RG equation for the EAA:
∂kΓk [ϕ] =1
2
∫q
∂kRk(q2)(
Γ(2)k [ϕ] +Rk
)−1
q,−q
Rk (q, q′) =
(2π)dδ(q + q′)Rk (q2)
Properties:
• integral equation
• differential equation
• non-linear equation
• IR finite
• UV finite
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The exact RG equation
Exact RG equation for the EAA:
∂kΓk [ϕ] =1
2
∫q
∂kRk(q2)(
Γ(2)k [ϕ] +Rk
)−1
q,−q
Rk (q, q′) =
(2π)dδ(q + q′)Rk (q2)
Properties:
• integral equation
• differential equation
• non-linear equation
• IR finite
• UV finite
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The exact RG equation
Exact RG equation for the EAA:
∂kΓk [ϕ] =1
2
∫q
∂kRk(q2)(
Γ(2)k [ϕ] +Rk
)−1
q,−q
Rk (q, q′) =
(2π)dδ(q + q′)Rk (q2)
Properties:
• integral equation
• differential equation
• non-linear equation
• IR finite
• UV finite
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The exact RG equation
Exact RG equation for the EAA:
∂kΓk [ϕ] =1
2
∫q
∂kRk(q2)(
Γ(2)k [ϕ] +Rk
)−1
q,−q
Rk (q, q′) =
(2π)dδ(q + q′)Rk (q2)
Approximation schemes:• vertex expansion:
Γk [ϕ] =∞∑n=0
1
n!
∫x1,...,xn
Γ(n)k x1,...,xn
[ϕ] (ϕ− ϕ)x1. . . (ϕ− ϕ)xn
tower of coupled functional equations
with some Ansatz for Γk (truncation) → tower of beta-functions
• derivative expansion:
Γk [ϕ] =
∫x
[1
2Zk (ϕ) (∂ϕ)2 + Uk (ϕ) + higher derivative terms
]effective potential: Uk(ϕunif) ≡
1
ΩΓk [ϕ = ϕunif]
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Computation of critical exponents in the O(N) model
Example: O(N)-model
Ansatz for the EAA:
Γk [~ϕ] =
∫x
[1
2∂µϕa∂
µϕa +m2
k
2ϕaϕa +
λk
4!(ϕaϕa)2
], a = 1, . . . ,N
• Local Potential Approximation (LPA)
• Zk = 1 =⇒ ηk ≡ −k∂k lnZk = 0
• truncation of Uk(ϕ) up to ϕ4 : Uk(ϕ) = m2kρ+
λk
3!ρ2, ρ =
1
2ϕaϕa
Flow equation for the Effective Potential:
∂tUk(ρ) =1
2
∫q
∂tRk(q)
(1
q2 + Rk(q) + U ′k + 2ρU ′′k+
N − 1
q2 + Rk(q) + U ′k
)m2
k = U ′k(ρ)|ρ=0 λk = 3U ′′k (ρ)|ρ=0
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dimensionless variables: m2k = m2
kk−2 and λk = λkk
d−4
y ≡ q2
k2Rk(q2) ≡ k2 y r(y)
Flow equations:
∂tm2k = −2m2
k +λk
3
N + 2
(4π)dΓ(d2
) ∫ ∞0
dy yd2
+1 r ′(y)
[y(1 + r(y)) + m2k ]
2
∂t λ = (d − 4)λk −2
3λ2k
N + 8
(4π)dΓ(d2
) ∫ ∞0
dy yd2
+1 r ′(y)
[y(1 + r(y)) + m2k ]
3
Choose a cutoff function:
Rk(z) = (k2 − z)θ(k2 − z) , ⇒ r(y) =1− y
yθ(1− y)
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∂tm2k = βm2 (m2
k , λk)
= −2m2k −
N + 2
3cd
λk
[1 + m2k ]
2
∂t λk = βλ(m2k , λk)
= (d − 4)λk +2
3(N + 8)cd
λ2k
[1 + m2k ]
3
→ beta functions are non-perturbative
-2.0 -1.5 -1.0 -0.5 0.0 0.5 1.0
-0.5
0.0
0.5
1.0
1.5
2.0
m k2
Λ
k
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∂tm2k = βm2 (m2
k , λk)
= −2m2k −
N + 2
3cd
λk
[1 + m2k ]
2
∂t λk = βλ(m2k , λk)
= (d − 4)λk +2
3(N + 8)cd
λ2k
[1 + m2k ]
3
→ beta functions are non-perturbative
G
WF
-2.0 -1.5 -1.0 -0.5 0.0 0.5 1.0
-0.5
0.0
0.5
1.0
1.5
2.0
m k2
Λ
k
Fixed points:
m2∗ = − (4− d)(N + 2)
8(N + 5)− d(N + 2)
λ∗ =96
cd
(4− d)(N + 8)2
[8(N + 5)− d(N + 2)]3
• d < 4: two Fixed Points
• d = 4: only the Gaussian FP
• d > 4: spurious FP
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Stability matrix:
Mij =
(∂m2βm2 ∂λβm2
∂m2βλ ∂λβλ
)∣∣∣∣∗
Eigenvalues:
Λ± =1
2
(TrM±
√(TrM)2 − 4 detM
)ΛWF± = − 1
N + 8
3(N + 4)− d(N + 5)
±√
3
2d2 (N2 + 10N + 22)− 6d (2N2 + 21N + 52) + (5N + 28)2
Exponent ν:
ν = − 1
ΛWF−
'd→4−
1
2+
N + 2
4(N + 8)(4− d) +O((4− d)2)
• same result of of theε-expansion (at first order)
• the result is valid for any d
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Stability matrix:
Mij =
(∂m2βm2 ∂λβm2
∂m2βλ ∂λβλ
)∣∣∣∣∗
Eigenvalues:
Λ± =1
2
(TrM±
√(TrM)2 − 4 detM
)ΛWF± = − 1
N + 8
3(N + 4)− d(N + 5)
±√
3
2d2 (N2 + 10N + 22)− 6d (2N2 + 21N + 52) + (5N + 28)2
Exponent ν:
ν = − 1
ΛWF−
'd→4−
1
2+
N + 2
4(N + 8)(4− d) +O((4− d)2)
• same result of of theε-expansion (at first order)
• the result is valid for any d
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Ising (N = 1) massless case (m2k = 0): λk =
(k
Λ
)d−4 λΛ
1 +6ud λΛ
4− d
[(k
Λ
)d−4
− 1
]
d=3:
λk =Λ
k
λΛ
1 + 6u3λΛ
(Λk − 1
) −−−−→k→0
Λ fixed
1
6u3
• k → 0: IR fixed point
• Λ→∞: asymptotic freedom
Π2
0.0 0.5 1.0 1.5 2.0
k
L
2
4
6
8
10
Λ
k
d=4:
λk =λΛ
1− 6u4λΛ log kΛ
−−−−→k→0
Λ fixed
0
• k → 0: triviality
• Λ→∞: Landau pole
1 2 3 4 5
k
L
- 5
0
5
Λ
k
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Ising (N = 1) massless case (m2k = 0): λk =
(k
Λ
)d−4 λΛ
1 +6ud λΛ
4− d
[(k
Λ
)d−4
− 1
]d=3:
λk =Λ
k
λΛ
1 + 6u3λΛ
(Λk − 1
) −−−−→k→0
Λ fixed
1
6u3
• k → 0: IR fixed point
• Λ→∞: asymptotic freedom
Π2
0.0 0.5 1.0 1.5 2.0
k
L
2
4
6
8
10
Λ
k
d=4:
λk =λΛ
1− 6u4λΛ log kΛ
−−−−→k→0
Λ fixed
0
• k → 0: triviality
• Λ→∞: Landau pole
1 2 3 4 5
k
L
- 5
0
5
Λ
k
The Functional Renormalization Group SISSA-ISAS 20 / 22
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Ising (N = 1) massless case (m2k = 0): λk =
(k
Λ
)d−4 λΛ
1 +6ud λΛ
4− d
[(k
Λ
)d−4
− 1
]d=3:
λk =Λ
k
λΛ
1 + 6u3λΛ
(Λk − 1
) −−−−→k→0
Λ fixed
1
6u3
• k → 0: IR fixed point
• Λ→∞: asymptotic freedom
Π2
0.0 0.5 1.0 1.5 2.0
k
L
2
4
6
8
10
Λ
k
d=4:
λk =λΛ
1− 6u4λΛ log kΛ
−−−−→k→0
Λ fixed
0
• k → 0: triviality
• Λ→∞: Landau pole
1 2 3 4 5
k
L
- 5
0
5
Λ
k
The Functional Renormalization Group SISSA-ISAS 20 / 22
Conclusions References
Conclusions
Summary
• RG explains universality −→ flow to a FP
• RG explains critical behavior −→ critical exponents
• EAA: computational framework −→ approximation schemes
• it is possible to compute universal quantities −→ exponents ν, η
Why Functional RG?
• clearer picture (with respect to perturbative RG)
• recover known results (ε-expansion, loop expansion, . . . )
• new approximation schemes: possibility to go beyond perturbation theory
• computation valid for any dimension d
The Functional Renormalization Group SISSA-ISAS 21 / 22
Conclusions References
References
K. Huang, “Statistical Mechanics”, 1987, Wiley
I. Herbut, “A modern approach to Critical Phenomena”, 2007, CambridgeUniversity Press
B. Delamotte, “An introduction to the nonperturbative renormalizationgroup”, 2007, arXiv:cond-mat/0702365v1
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