theoretical study of high temperature superconductivity · 1.origin of the superconductivity •...
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1 National Institute of Advanced Industrial Scienceand Technology (AIST)2 Hakodate National College of Technology
Theoretical Study ofHigh Temperature Superconductivity
T. Yanagisawa1, M. Miyazaki2, K. Yamaji1
1. Introduction2. Superconductivity3. High Temperature Superconductivity4. Hubbard Model5. Variational Monte Carlo method6. Stripes in high-Tc cuprates7. Spin-orbit coupling and Lattice distortion8. Summary
Outline
1. IntroductionKey words: Physics from U (Coulomb interactions)
•A possibility of superconductivity Superconductivity from U
•Competition of AF and SC
•Incommensurate state Stripes and SC Compete and Collaborate
•Stripes in the lightly-doped region
•Singular Spectral function
0
100
200
300
T(K)
Concentration x in Ln2-x
MxCuO
4-y
SC
AFAF
SC
Hole dopedElectron doped
0.3 0.2 0.1 0 0.1 0.2 0.3 0.4
Pseudo-gap
Stripes
1. Origin of the superconductivity• Symmetry of Cooper pairs• Mechanism of attractive interaction
Coulomb interaction U, Exchange interaction J
2. Physics of Anomalous Metallic behavior• Inhomogeneous electronic states: stripe• Pseudogap phenomena• Structural transition LTO, LTT
Purpose of Theoretical study
2. Superconductivity
Temperature K
1911Kamerlingh Onnes Elements that become superconducting
Superconductive at low temperatures
Superconductive under pressure
Resis
tivity
Characteristics of Superconductivity
Electrical Resistivity
Meissner effect
Metal Semiconductor Superconductor
Exclusion of a magneticfield from a superconductor
3. High Temperature Superconductors
0
20
40
60
80
100
120
140
160
1920 1940 1960 1980 2000
Tran
sitio
n te
mpe
ratu
re (
K)
Year
PbHg
NbNbN
V3Si
Nb3Sn
Nb-Al-Ge
Nb3Ge
K3C
60
MgB2
La2-x
BaxCuO
4
La2-x
SrxCuO
4
YBa2Cu
3O
7
Bi2Sr
2Ca
2Cu
3O
y
Tl2Ba
2Ca
2Cu
3O
y
HgBa2Ca
2Cu
3O
y
HgBa2Ca
2Cu
3O
y(Under Pressure)
TlBaCaCuO
Liquid N2
Liquid H2
Critical Temperature
La2CuO4 YBa2Cu3O7
Phase Diagrams
Phase diagram of HTSC
Electron densityHole density
超伝導
反強磁性
Tc
TN
AF
Superconducting
Carrier density
T
Anomalous metal
Two-Dimensional Plane
Characteristics
• Two dimensional• Low spin 1/2• O level is very closed to Cu level.
Cu
O
dx2-y2
εd
εd+Udεp
Doped hole
px
Model of HTSC
Temperature dependence of Resistivity
H. Takagi et al. T. Ito et al.
Specific Heat
Loram et al., Phys. Rev. Lett. 71, 1740 (1993)
Loram et al., Physica C162-164, 498 (1989)
LSCO
Nuclear Magnetic Resonance
Yasuoka et al., Physica B199 (1994)278
YBa2Cu4O8 Tc= 81K
Tc
χ
The decrease of 1/TT1 above Tcsuggests the existence of the pseuo-gap.
In the conventional case
4. Hubbard Model
Itinerant Electrons
↑ ↑↓ ↓Atoms
Electrons
Mott insulatorsMnO, FeO, CoO, Mn3O4, Fe3O4,NiO, CuO
Insulators due to the Coulomb interaction
(Note: Antiferromagnets such as MnO and NiO are not Mott insulators
in the strict sense.)
On-site Coulomb Interaction
↑
Coulomb interaction
↑
ε0
ε0+U
U >> t Insulator
↑
↑t
+U
↑ ↑
Gap in the Hubbard ModelHartree-Fock theory (Half-filling)
AF Gap Δ = Um Δ ~ t e-2πt/U d = 1, 3 ~ t e-2π(t/U)1/2 d = 2
1D Hubbard modelU << t U >>t
Hubbard gap Δ U(16 / π ) tUe− π / (2U )
Spin-wave velocity 2vs/π = J
�
(4 t /π )(1−U /4πt) 4t2/U
Δε
k0
vsk~U
~1/U
vs
Δ
Cu-O2 Model and Hubbard Model
Cu-O2 model(d-p model)
t-J model Hubbard model
tpd << Ud-(εp−εd)tpd << εp−εdεp−εd << Ud
U >> t
εp−εd ~ 0(tpd)
Zhang-Rice singlet Mixed state of d and p
H = −t (ciσ+
ij σ∑ c jσ + h.c.) + J Si
ij∑ ⋅ Sj H = −t (ciσ
+
ij σ∑ c jσ + h.c.) +U ni↑
i∑ ni↓
5. Variational Monte Carlo methodWe evaluate the expectation values using the Monte Carlo method.
Gutzwiller function
�
ψG = PGψ 0
�
PG = 1− (1− g)n j↑n j↓( )j∏
�
ψ 0 : trial wave function Fermi sea, AF state, or BCS state
Gutzwiller operator
�
0 ≤ g ≤ 1
Control the on-site correlation in terms of g
weight g weight 1Coulomb +U
Variational Monte Carlo Method
Normal state
�
ψ 0 Slater determinant
Wave numbers: k1, k2, …, kn Coordinatepositions:j1, j2, …, jn
�
det D↑ =eik1 j1eik1 j2 L eik1 jn
Leikn j1eikh j2 L eik n jn
�
ψ 0 = all∑ ψ l
�
ψ l :particles in the real space
Weight of this state
�
al = det D↑ det D↓
Slater determinant
The large number of particle configurations → Monte Carlo method
Monte Carlo algorithm
Expectation value
�
ψQψ = ammn∑ an ψ mQψ n =
am2
al2
l∑m
∑ anam
ψ mQψ nn∑
�
ψ m
�
Pm =am2
al2
l∑
�
ψQψ =1M
anam
ψ mQψ nn∑⎛ ⎝ ⎜
⎞ ⎠ ⎟
m∑
�
m = 1,L ,M
Metropolis法 ψ j → ψ n
R = an2 / aj
2≥ ξ , adopt
�
ψn
< ξ ψ jξ: random numbers 0 ≤ ξ <1
The appearance rate of is proportional to in M.C. steps,
Ifagain
ψ CdS = PG (ukk∏ + vkck↑
+ c− k↓+ ) 0
Gutzwiller Projection PG
To control the on-site strongcorrelation
Weight g Weight 1Coulomb +U Parameter 0<g<1
Equivalent to
RVB state (Anderson)
Superconducting state
k -k
SC Condensation energy
ΔESC = Ωn − Ωs = (Sn0
T c
∫ − Ss )dT
= (Cs0
T c
∫ − Cn )dT
Loram et al. PRL 71, 1740 (‘93)
T
C/T
SC Condensation energy ~ 0.2 meV
optimally doped YBCO
Entropybalance
Superconducting condensation energy
Evaluations in the superconducting state
-0.738
-0.736
-0.734
-0.732
-0.730
0 0.05 0.1 0.15
E g /N s
Δ
0
0.001
0.002
0.003
0.004
0 0.005 0.01
ΔE/N
1/Na
Variational Monte Carlo method10x10 Hubbard model U= 8
YBCO
Econd ~ 0.2meV
SC condensation E
T. Nakanishi et al. JPSJ 66, 294 (1997)
K. Yamaji et al., Physica C304, 225 (1998) T. Yanagisawa et al., Phys. Rev. B67, 132408 (2003)
Condensation energyEcond ~ 0.00038tdp = 0.56 meV/site
δ = 0.333tpp= 0.2
SC order parameter
2D d-p model 6x6 and 8x8
Hole density
Condensation Energy for d-p model
T.Yanagisawa et al., PRB64, 184509 (‘01)
Superconductivity and Antiferromagnetism
0
0.002
0.004
0.006
0.008
0.01
0.012
0.014
0.016
-0.4 -0.3 -0.2 -0.1 0 0.1 0.2
SDW(U=6,L=10)SDW(U=6,L=12)SC(U=6,L=10)SC(U=6,L=12)
E cond
t'
Fig. 1
0
0.0002
0.0004
0.0006
0.0008
0.001
0.0012
0 0.002 0.004 0.006 0.008 0.01
Fig. 2SC Econd (ρ ~.84, U=5, t'=−.05)
E cond
1/Ns
Size dependence ofSize dependence ofSC condensation energySC condensation energy
CompetitionCompetition
Pure d-wave SC
0.41meV
Experiments 0.26 meV/site 0.17~0.26 (critical field Hc) (C/T)
AFSC
t’
6. Stripes in high-Tc cuprates
M.Fujita et al. Phys. Rev.B65,064505(‘02) S.Wakimoto et al. PRB61, 3699(‘00)
• Vertical stripes for x > 0.05• Diagonal stripes for x < 0.05
SC+Stripes Coexist
Vertical
Diagonal
Neutron scatteringAF coexists with SC?
T.Y. et al., J.Phys.C14,21(‘02)
Vertical Stripes in the under-doped region
-10
-8.0
-6.0
-4.0
-2.0
0.0
0.2 0.25 0.3 0.35 0.4 0.45 0.5E/N
tpp
Stripes
Commensurate AF
Vertical stripes: 8 lattice periodicity (Tranquada)
x = 1/8Charge rich
Chargepoor
3-band HubbardVMCCharge
rich
8 lattice period
Stripes and Superconductivity
Hij↑ + Fij
Fji* − H
ji↓
⎛
⎝ ⎜
⎞
⎠ ⎟ ujλ
vjλ
⎛
⎝ ⎜
⎞
⎠ ⎟ = Eλ ui
λ
viλ
⎛
⎝ ⎜
⎞
⎠ ⎟
αλ = uiλ a
i↑+ vi
λai↓+
αλ = uiλ a
i↑+ vi
λai↓+
ψ SC = PGPN eαλ
λ∏ αλ
+ | 0 ∝ PG (U−1V)ij ai↑+ aj↓
+
ij∑
⎛
⎝ ⎜ ⎞
⎠ ⎟ N e / 2
|0
Bogoliubov-de Gennes eq.
Wave functionVλj = vj
λ U( )λj = u jλ
↑
↑↓
SC coexists with stripes (AF) Compete and Collaborate
Nano-scale SC
LaLa2-x2-xSrSrxxNiONiO44LaLa2-x2-xSrSrxxCuOCuO44LaLa2-x-y2-x-yNdNdyySrSrxxCuOCuO44
Diagonal stripes are observed for
Diagonal stripes in lightly doped region
0
100
200
300
T(K)
Concentration x in Ln2-x
MxCuO
4-y
SC
AFAF
SC
Hole dopedElectron doped
0.3 0.2 0.1 0 0.1 0.2 0.3 0.4
δ can be explained by 2DHubbard model.
δ = x
Verticalstripes
Diagonal stripes
Incommensurability: Comparison with Experiments
U=8.0 t’= -0.2
LTT,LTO,LTLO,HTT
M.Fujita et al. Phys. Rev.B65,064505(‘02)
Structural transitions: Lattice distortions
Stripes: suggested by Incommensurability
N.Ichikawa et al. PRL85, 1738(‘00)
LTO
LTT
HTT
Hole density
T
LTLO
δ~x
Stripes and Structural transition
1. Anisotropy of the transfer integrals Anisotropic electronic state vertical stripes Diagonal stripes x<0.05 2. Spin-Orbit Coupling induced from lattice distortions 3. Electron-phonon interaction
LTO
LTT
HTT
Hole density
T
LTLO
vertical
What happens under lattice distortions?
0.015
0.02
0.025
0.03
0.035
0.04
0.045
0.75 0.8 0.85 0.9 0.95 1 1.05 1.1
Δ(En-Ecoexist
) / Ns
Δ, (En-Ecoexist) / Ns
β
LTT structural transitions stabilize stripes.• = ty / tx
• X
• Y
One-band Hubbard model (Miyazaki)
Anisotropy of the transfer integrals in LTT phase
tx
LTLO LTTLTTLTLO
LTO
LTT
HTT
Hole density
T
M. K. Crawford et. al.
tx
ty
LTLO
Mixed phase ofMixed phase ofLTT and LTLOLTT and LTLO
Stripes // tilt axisStripes // tilt axis
Hole richdomain
Hole poordomain
Stabilize stripes
Possible Stripe Structure 1
tx
LTT HTTHTTLTT
LTO
LTT
HTT
Hole density
T
M. K. Crawford et. al.
tx
ty
LTLO
Mixed phase of LTT and HTTMixed phase of LTT and HTTStripes perpendicular to tilt axisStripes perpendicular to tilt axis
Stable H. OyanagiA. Bianconi
Charge poorCharge rich
-0.1
0
0.1
0.2
0 0.02 0.04 0.06 0.08 0.1
LTT-HTTParallel //stripesPerpendicular
Δ E/N
u
Oscillation of tilt angles
Possible Stripe Structure 2
HSO = ξ(r)L ⋅ S
dxz(r)↑|HSO|d yz(r)↑ = −i2ξ
dyz(r)↑|HSO|d xz(r)↑ =i2ξ
px(x − a / 2, y)↑|Hdp|d xz(r)↑ = −t xze−ik x / 2⋅a
py(x, y− a / 2)↑|Hdp|dyz (r)↑ = −tyze−iky / 2⋅a
Effective iξ term for p-p transfer
Friedel et al., J.Phys.Chem.Solids 25, 781 (1964)Spin-Orbit Coupling induced by the Lattice distortion
Five orbitals × (↑↓):(dx2-y2, dxz, dyz, px, py)
dx 2 − y 2 (r)↑|HSO|d yz(r)↓ =i2ξ
dx 2 − y 2 (r)↑|HSO|d xz(r)↓ =12ξ txz, tyz ≠0 ~ tilt angle
Q1
CuOxygen
Q2
Tilting
7. Spin-orbit coupling and Lattice distortion
Hkin = − (t ij +ijσ∑ icσθij )diσ
+ djσ(Bonesteal et al.,PRL68,2684(‘92))
One-band effective model
(π/2,π/2)
d-p model
Zone boundary
K.Yamaji, JPSJ 57 (1988) 2745. T.Y. et al., JPSJ 74 (2005) 835.
ξ = 0.4
-8
-6
-4
-2
0
2
4
6
8φ = π/100φ = 3π/100Ek=-2(coskx+cosky)
Ek
k(0,0) (π,0) (π,π) (0,0)
Dispersion in the presence of spin-orbit coupling
φ
φ
φ
−φ
−φ
φ
φ
φ
Excitation: Dirac fermionLinear dispersion
Fermi point (half-filling)
Small Fermi surface
Ek
E(kx ,ky) = ±eiφ / 4eikx + e− iφ / 4eik y
+eiφ / 4e−ik x + e−iφ / 4e−ik y
φ
Inhomogeneous d-density wave
Flux state
Flux statePseudo-gap
Gσ (r, r' ,iω) =ϕσm(r)ϕσm
* (r' )iω − Eσmm
∑
Hϕσm(r) = Eσmϕσm(r)
Nσ (k,ε ) = −1πImGσ (k,ε + iδ )
Density of states
Eigenfunction ϕσm(r)
An origin of pseudo-gap
LTO
LTT
HTT
Hole density
T
LTLO
0
0.2
0.4
0.6
0.8
1
0 0.2 0.4 0.6 0.8 1
φ = 0φ = π/100φ = 3π/100
N(ω
)
ω/ t
Pseudo-gap in the density of states
φ
φ
φ
−φ
−φ
φ
φ
φ
φ
Φ = 4φDiagonal Stripe & d-density wave
Diagonal stripes with Spin-orbit coupling
-0.575
-0.57
-0.565
-0.56
-0.555
-0.55
0 0.02 0.04 0.06 0.08E/N
φ/π
Diagonal
Vertical
Uniformx = 0.03Spin-orbit coupling stabilizes
the diagonal stripes.VMC
bond-centersite-center
Spin-orbit coupling induces flux.
T.Y. et al., JMMM 272 (2004) 183.
d-density waveiΔQY(k) = ck+Qσ
+ ckσ Q = (π ,π )Y (k) = cos(kx) − cos(ky) φ
φ
φ
−φ
−φ
φ
φ
φ
φ
−φ
−φ
−φ
−φ
φ
φ
φ
−φ
−φ
φ
φ
φ
φ
−φ
−φ
−φ
−φ
Inhomogeneous density wave
Stripe
iΔQY(k) = ck+Qσ+ ckσ
Δ lQsσ = ck+lQsσ+ ckσ
k∑
Qs =(π+2πδ,π) verticalQs =(π+2πδ,π+2πδ) diagonal
Nayak, Phys. Rev. B62, 4880 (‘00)Chakravarty et al., PRB63, 094503 (‘01)
d-symmetry
incommensurate
d-density wave
300
200
100
00.300.250.200.150.100.050.00
0
0.001
0.002
0.003
0.004
0 0.005 0.01
ΔE/N
1/Na
ψ CdS = PG (ukk∏ + vkck↑
+ c− k↓+ ) 0
Theoretical estimate ofSC condensation energy
Agreement with Exp.
Econd ~ 0.2meV
IncommensurabilityNeutron scatterings
overdopedunderdoped
YBCO
8. SummaryHTSC and Correlated Electrons
BCS-Gutzwiller functionVariational Monte Carlo study of