Phase fluctuation in AF order and its effect on the pseudo...
Transcript of Phase fluctuation in AF order and its effect on the pseudo...
Phase fluctuation in AF order and its effect on the pseudo-gap in
electron doped cuprates
Chang Young Kim Yonsei University
Outline
1. Review
2. ARPES results
3. Spin-fermion model
4. AF phase fluctuation model
5. Conclusion
What interacts with electronsin HTSCs?
k
k'
?
Lattices, spins, etc
k
k' -k
-k'
Cooper pair
Information in spectral functionsElectron-phonon coupling
Ashcroft, Mermin “Solid State Physics”T. Valla, Science, 1999
“kink”
‘kink’ in the spectral function
Controversies in h-doped HTSCs
- Similar energy scalesSuperconducting gap, Pseudo gap, Phonons, Magnetic resonance mode
Q=(0.5,0.5)
H. He et al. PRL (2001)
Strong kink in Bi2212
A. Gromko et al., PRB
Energy scales in e-doped HTSCs
High E kink (~500 meV)
Low E kink (~50 meV)Pseudo gap ( ~ 100 meV)
Magnetic resonance mode (~10 meV?)Superconducting gap (~3 meV)
B. Moritz et al., NJP
Spin resonance mode?
S. Wilson, Nature 442, 59 (2006)
Phonons in e-doped HTSCs
Nodal
Anti-nodal
Isotropic e-phonon coupling ( S. R. Park, PRL 101, 117006 (2008) )
Wish to look at pseudo-gap
High E kink (~500 meV)
Low E kink (~50 meV)Pseudo gap ( ~ 100 meV)
Spin resonance mode (~10 meV?)Superconducting gap (~3 meV)
N. P. Armitage
PRL (2001)Binding energy(eV)
• Spectral weight suppression near EF at the intersection of AF Billiouin Zone Boundary (AFBZ) and the underlying FS
• Coupling to a bosonicmode localized at Q=(π,π)?
kx
ky
Pseudo-gap effect
PG in electron doped cuprates
Static 2 x 2 order
(π, π) scattering from 2 x 2 order?
AFBZ
EF
Original Fermi surface
(π,0)
(π,π)
Γ
Band StructureAFBZ
2Vπ,π
EF
Reconstructed Fermi surface
EF
2Vπ,π
Inter-band transition
( π,0 )
Bind
ing
Ener
gy (e
V)EF
0.1
0.2
2Vππ
(π/2, π/2)
σ 1(Ω
-1 c
m-1
)
00
2
4
Photon Energy (eV)0.5
onset
x103
1.0
220K140K70K10K
300K
(0,π) (π,0)
EF
2Vππ
(π/2,π/2)
Bind
ing
Ener
gy
Momentum
Energy (eV)0 2 4 86 10 12 14
0.2
0.4
0.6
0.8
1.0
Refl
ecti
vity
DOS
0-2-4
-8-6
2 Energy (eV)
visible pwh
copper
S. R. ParkPRB 2007
Overshooting problemBi
ndin
g En
ergy
(eV)
EF
0.1
0.2
0.3
0.4
k parallel to (0,0)-(p,p) (1.41p/a)(π,0.3π)(π,0)
a)dcb
a (π,π)
Γ
S. R. Park et al., PRB® (2007)
(π,π)
Γ
H. Matsui et al., PRL (2005)
0.50.4 0.6
d)
0.4 0.5 0.6
c)
0.4 0.5 0.6
b)SCCO(x=0.15)
NCCO(x=0.13)AFBZ
2Vπ,π
EF
EF spectral weight at hot spot
kx (p/a)
k y(p
/a)
1-1
a)
b)1
B.E.
(eV)
0.0
0.2
0.4
PGa)
Momentum
B.E.
(eV)
0.0
0.2
0.4
Momentum
b)
Inte
nsit
y (a
rb.)
0.4 0.3 0.0Binding energy (eV)
0.2 0.1
NCCO
AF LRO
Hot spot
Hot spot
FS, Tem.=10KNd1.85Ce0.15CuO4
Two problems:1. Band overshoots across AFZB
2. Ef Spectral weight @ hot spot
In addition:
What is the origin of scattering?(Spin-fermion, localized moments, …)
Effect of short range order?Te
mpe
ratu
re (K
)
Cerium concentration, x
100
200
300
400
500
00 0.5 1.0 1.5
ξ/a2
400
50
5
10
20
100
200
Nd2-xCxCuO4
AF correlation length by INS
Cu
AF long range order
E. M. Motoyama et al., nature (2007)
2ξ
How to control the ordering length?
Rare earth element dependent AF: muon spin relaxation
2.0Time (ms)
0.0 0.5 1.0 1.5A
sym
met
ry
Nd2-xCexCuO4 T=10K
x=0.0
x=0.10
x=0.14
x=0.16
Doping concentration0.0 0.0
50.10 0.15 0.2
0
AFMSCTe
mpe
ratu
re (k
)
0
100
200
300Nd2-xCexCuO4
Time (ms)0 1 2 3 4
Asy
mm
etry
Sm1.95Ce0.05CuO4120K
110K
75K
100K
75K
Sm1.80Ce0.20CuO4
G. M. Luke et al., PRB, 1990 T. Sasakawa, unpublished
heavier rare-earth element, stronger AF
static AF cover all SC dome in SCCO
SCAFM
0.0 0.05 0.10 0.15 0.200
0.25
100
200
Doping concentration
Sm2-xCexCuO4
Tem
pera
ture
(k)
Pr1-xLaCexCuO4
Doping concentration0.0 0.10 0.2
0
Tem
pera
ture
(k)
100
200
M. Fujita et al., PRB, 2003
Samples
Nd1.85Ce0.15CuO4(Tc=23K)
Sm1.90Ce0.10CuO4(Tc=0K)
Sm1.85Ce0.15CuO4(Tc=17K)
Sm1.82Ce0.18CuO4(Tc=9K)
Eu1.85Ce0.15CuO4(Tc=0K)
Gd1.85Ce0.15CuO4(Tc=0K)
Rn2-xCexCuO4
Floating zone
SSRL, Stanford, USAB.L. 5-4 high resolution ARPES
ARPES Optical
Yonsei Univ.
Experiments
• ARPES experiments: Stanford Synchrotron Radiation Lab.
• Energy resolution : 15 meV
• Temperature : 15K
Rare-earth elements dependent
kx (p/a) 1 1
SCCO ECCO GCCO
kx (p/a) kx (p/a)0 1
k y(p
/a)
1 90
80
70
60
50
40
30
Nd Sm Eu GdIn
tens
ity(
arb.
)Ln1.85Ce0.15CuO4
Integrated Intensity from
-0.1 to EF
.0
.1
.2
.3
.4 NCCO SCCOECCO
SCCO
NCCO
Bin
ding
ene
rgy
(eV
)
0.00.10.20.3Binding Energy (eV)
Momentum ( (1/2,1/2) → (1,0) )
Tem. Dep. Spectral weight
kx (π/a)
k y(π
/a)
1-1
1FS, Tem.=10K
kx (π/a)
k y(π
/a)
1
1
-1
FS, Tem.=280K
A(k,w)/F.D.
105
95
10 30 80 130 180 230 280
Inte
nsit
y (a
rb.)
Temperature (K)
Integrated intensity from -0.1 to EF~1/correlation length(ξ)
Tem
pera
ture
(K)
Cerium concentration, x
100
200
300
400
500
00 0.5 1.0 1.5
ξ/a2
400
50
5
10
20
100200
Nd2-xCxCuO4
Intensity (arb. units)
0.00.10.20.3
10K80K130K180K230K280K
Previously also seen in NCCOH. Matsui et al., PRB (2007)
Doping dep. spectral weight
Sm2-xCexCuO4
0.00.10.20.3Binding Energy (eV)
0.10
0.15
0.18
Doping, temperature, rare earth dependences all show that:
1. Overall, gap size does not change much
2. Gap is filled up as AF ordering length
decreases
⇒Similar to pseudo-gap in hole doped & reminiscence of phase fluctuation.
Spin-fermion model
Coupling to spin excitations
χ”
U = 1.59 eV
ξ=4a
ξ=16
a
0.00.10.20.30.4
Binding Energy (eV)
0.00.10.20.3
Electron doped case
(0.5, 0.5)
Ene
rgy
(eV
)
0.1
0.3
0.0
0.2
Imχ(ω)
q=(0.5, 0.5)
FS Dispersion
Momentum
Wilson et al., PRL 96, 157001 (2006)
kx (p/a) 1
SCCO
0
k y(p
/a)
1
Optical conductivity
Experiment Simulation
σ1 (arb. unit)σ 1(Ω
-1 c
m-1
)
0
2
4
Photon Energy (eV)
x103
0.0
220K140K70K10K
300K
0.2 0.4 0.0 0.2 0.4
ξ=32aξ=16a
ξ=8a
ξ=4a
ξ=2a
AF phase fluctuation model
(“Yet another spin-fermion model”,A. Chubukov)
Subject to potential from AF order
mi = local magnetic momentSi = electron spinλ = coupling constant
<= AF phase fluctuation
with
and
Finally:
with∗ ξ = ordering length
AF phase fluctuation effect(averaging over different Q’s)
Γ (π,0)
(π,π)
Q0
∼1/ξ
Q0+δ
∼1/ξ
Γ (π,0)
(π,π)
Q0+δ
∼1/ξ
Γ (π,0)
(π,π)
Q0+δ
∼1/ξ
Γ (π,0
(π,π)
ξ~8a ξ~4a ξ~2aξ~16aξ~32a
0.0
0.1
0.2
0.3
0.4
1 2 1 2 1 2 1 2 1 2
1
2
1
2
1
2
1
2
1
2
Bind
ing
Ener
gy (e
V)
EF
0.1
0.2
0.3
0.4
0.50.4 0.6
c)
0.4 0.5 0.6
b)
cb
(π,π)
Γ
a
0.4 0.5 0.6
a)
Bind
ing
Ener
gy (e
V)
EF
0.1
0.2
0.3
0.4
a) b) c)
k parallel to (0,0)-(π,π) (1.41π/a)
Momentum
Sm1.85Ce0.15CuO4
Short Range Order(SRO) , ξ~4a Long Range order
Electron-AF SRO coupling
0.0
0.1
0.2
0.3
0.4Bind
ing
ener
gy (e
V)Momentum
Gap filling and EF weightBi
ndin
g En
ergy
(eV) EF
0.1
0.2
0.3
0.4Momentum Momentum Momentum Momentum Momentum
Fermi surfaceξ~8aξ~16aξ~32a ξ~4a ξ~2a
Binding Energy (eV)
A(k
,w)
Spectral weight near EF
ξ~32a, 16a
ξ~4aξ~2a
ξ~8aξ~16aξ~32a ξ~4a ξ~2a
-0.30 -0.25 -0.20 -0.15 -0.10 -0.05 0.00
ξ~8a
Optical conductivity
Experiment Simulation
σ1 (arb. unit)σ 1(Ω
-1 c
m-1
)
0
2
4
Photon Energy (eV)
x103
0.0 0.2 0.4
ξ=32aξ=16aξ=8aξ=4aξ=2a
0.0
220K140K70K10K
300K
0.2 0.4
The model….
1. Not spin-boson but phase gradient ( φ) couples to electron.
2. Tc can be estimated based within the model.
3. The parameter λm can be obtained by fitting exp data.
Summary
1. Correlation between pseudo-gap behavior and AF ordering
2. Pseudo-gap does not close but fills up as AF ordering decreases
3. ARPES spectral function and optical conductivity are well explained within AF phase fluctuation model
Quasi-particle dynamics intopological insulator Bi2Se3
S. R. Park, W. S. Jung, Chul Kim, D. J. Song, C. Kim, S. Kimura, K. D. Lee and N. Hur
Importance
1. Long lifetime of surface metallic states due to helical spin structure
2. Protected surface metallic states• No Fermi surface instability
: TI
: normal
FS of surface state and spin structure
Γ
Dissipationless nano-device and spinstronics
Long lifetime?- ARPES studies
ARPES for lifetime measurement
22 ),(Im)),(Re(),(Im1),(
ωωεωω
πω
kkkkA
k Σ+Σ−−Σ
=
Spectral function
energy
AR
PES
inte
nsity
FWHM:2ImΣ ~ 1/τ
ARPES on TI “Bi2Se3”Crystal structure Surface states
Y. Xia et al., Nat. Phys. (2009)H. Zhang et al., Nat. Phys. (2009)
Bulk
Our ARPES data (15 K, 8eV P. E.)
Γ
Fermi surface
0.3
0.2
0.1
0.0
Bin
ding
ene
rgy
(eV
)
-0.1 0.0 0.1Momentum (Å-1)
Experimental Fermi level
K
H. Zhang et al., Nat. Phys. (2009)
• Transport measurements as a bulksensitive tool also report metallicbehavior
Bulk
Bulk
Time dependence
-0.1 0.0 0.1Momentum (Å-1)
-0.1 0.0 0.1 -0.1 0.0 0.1
0.3
0.2
0.1
0.0
Bin
ding
ene
rgy
(eV
)
0.4
0.5
8 eV 10 eV 17 eV
Momentum (Å-1)
0.3
0.2
0.1
0.0
Bin
ding
ene
rgy
(eV
)0.4
0.5
~ 0.1eV
Fresh surface 4 days later
Surface (electron) doping effect with time
8eV
10
15
17
19
21
0.2 0.1 0.0Binding energy (eV)
0.3-0.1 0.0 0.1Momentum (Å-1)
-0.1 0.0 0.1 -0.1 0.0 0.1
0.3
0.2
0.1
0.0
Bin
ding
ene
rgy
(eV
)
0.4
0.5
8 eV 10 eV 17 eV EDCs @Γ
• Bulk states taken with 8 eV are suppressed due to kz-selection rule.• B. E. of bulk conduction band (EBB) ~ 0.1eV
After 4days
After 4days
Photon energy dependence
Life time : kink in ImΣ at ~EBB
ImΣ
(meV
)
0.25 0.20 0.15 0.10 0.05
60
50
40
70
Binding energy (eV)
Fresh surface (EBB ~ 0.1 eV)
0.0
4 days later (EBB ~ 0.2 eV)
ImΣ
EF
EBB
e-h pair phonon impurity
Scattering channels
EF impurity
e
h
• Kink in ImΣ at around EBB is originated from scatteringdue to phonon or impurity
Surface electron lifetime
• Scattering to bulk states due to impurity is the mainscattering channel for TM states.
0.25 0.20 0.15 0.10 0.05Binding energy (eV)
0.0
60
50
40
30
20
10
0
ImΣ
(meV
)
total
e-h pairphonon + impurity
P. E. 8eV, 15KFresh surface
Mob
ile e
lect
rons
τ=40 fs
)(02.0)/(105)(1040 515 msmsl gm μυτ =⋅×⋅=×= −
. To appear in PRB(R)
Summary
Experimental observation• Kink in scattering rate at around bulk
conduction band bottom
Interpretation• Strong scattering between surface and
bulk electrons due to electron-phonon coupling or impurity near EF
• Carrier life time in TM states hardly affected by adsorbate created disorder potential