Title: Asymptotic slavery and transport anomalies in the cuprates
1Asymptotic slavery and transport anomalies in the
cuprates
- Thanks to
- Claudio Chamon, Boston Univ.
- Ting-Pong Choy, UIUC
- D. Galanakis, UIUC
- T. Stanescu, UIUC (Rutgers)
2 2 electrons on 2 sites ?
2 electrons on 2 sites ( ) ?
E
n e r g y
DEU
QUIZWhat is the Ground state? (lowest energy
state)
3Possibilities
,
a.)
gt
,
gt
gt
low energy
,
,
b.)
-
, gt
,
gt
c.)
(high energy)
0, gt
d.)
, 0gt
e.) bd
high low energy
f.) cd
4Answer
,
gt - , gt
Mottness
5Cuprate phase diagram
SG
6asymptotic
slavery
Scaling (single length scale)
Renormalization
Mottness
Effective Theory
7Anomalous Normal State Puzzles
Fermi liquid
2.) Pseudogap
8Batlogg, et. al., 1990
Straight line
9How Wide is theT-linear Region?
Not very
Raffy, et. al., 2001
10Ando, et. al. 2004
11(No Transcript)
12Why T-linear Resistivity?
13Leading explanation
Quantum criticality
14Quantum criticality
- Zero-temperature (quantum fluctuations)
Temporal Correlations Diverge
Spatial correlations diverge
dynamical exponent
15Quantum critical
T
order
disorder
16Quantum Critical modes
Carry the current
17Phase diagram of High-T_c materials
18Is this correct?
19General Result
- One critical length scale
- Charges are critical
- Charges are neither created nor annihilated
(charge conservation)
20Vector potential
current
21scaling
22conductivity
23Charge conservation
24General result
T-linear resistivity
(d3 for cuprates)
Impossible?
Claudio Chamon
25Drude Conductivity
new energy scale
Not of scaling form Except for z-1
26Van der Marel, et. al. Nature 2004
27Scaling hypothesis
28 One-parameter Scaling breaks down
29Big picture
- Quantum criticality is irrelevant?
- Fermions are not critical?
- But ARPES, optical conductivity
Singular boson scattering Is an irrelvant
perturbation for fermions
30Valla et. al., Science, v. 285, p. 2110
31New direction
(UV-IR mixing)
all energy scales are mixed
Asymptotic slavery
32Mott Problem (NiO)
Insulator ???????
Hotel Model (N rooms N guests)
33Mott insulator
U
N
N
PES
IPES
UV-IR Mixing
gt2x
N-1
N-1
2
PES
IPES
34Perturbation Theory
m0
0
m1
Heff
0
m2
Not Fock Space
35What fails when the high energy scale is removed?
Spectral function
Single occupancy
double
UV-IR mixing
LHB
UHB
36Sum rule
Pauli Priniciple
(in general)
Projected Models
(t-J model)
37When is this failure important?
Half-filling
Particle-hole symmetry
Projected Models work!
38What about away from half-filling?
No symmetry
Projected Models
Breakdown of Pauli Principle
39Why?
40Exclusion Statistics(Haldane)
?d?-?? g???N?
Particle number
Available states
metric
Free fermions
)
(
1 0 0 1
g
? d"0
41What about t-J model (projected models?
No double occupancy
)
(
1 1 1 1
g
? d"-1
exclusons
42Mind the Pseudogap
43pseudogap
44(No Transcript)
45Ting-Pong Choy and P2
Hubbard Model
46pseudogap
Low to High energy Spectral weight
transfer
1.)UV-IR mixing 2.) orthogonality catastrophe QP
weight0 3.) Insulating state at T0
47Ando, et. al.
48(No Transcript)
49Pseudogap (intrinsic effect)
Hole doping
magnetic polaron
Orthogonality catastrophe
No overlap with antiferromagnetic regions
50T-J model
Rosch, Wolfle, 2004
Metallic Not insulator
51summary
- Projected models Hubbard model
No Pauli principle
Pauli Principle
Z/ J/t
No QP. Z0
(Kane, Lee, Read, Prokofiev, 2001, Sorella)
Sorella, us, others
52U! 1
L! 1
Do not commute
53Predictions
- Insulator in clean limit
- The dynamical exponent is negative
- Local magnetism in pseudogap state (x)
- Cuprates are asymptotically slaved
54(No Transcript)
552nd Puzzle
Breakdown of perturbation theory
56insulator
57Non-perturbative physics xgt0