utilizing the short wavelength of x-ray to study low-energy local excitations q-dependence of the...
TRANSCRIPT
Utilizing the short wavelength of X-ray to study low-energy local excitations
q-dependence of the spectral weights and dispersions
Wei Ku (BNL & SUNY Stony Brook)
Acknowledgement
Ben Larson & Jon Tischler (ORNL)
Chi-Cheng Lee & Hung-Chung Hsueh (BNL & Tamkang U. Taiwan)
Ken Finkelstein (CHESS, Cornell)
Paul Zschack (UNICAT-APS & UIUC)
Oscar Restrepo & Adolfo Eguiluz (UT-Knoxville & ORNL)
Peter Abbamonte, James P. Reed & Serban Smadici (UIUC)
Chen-Lin Yeh (BNL & Tamkang U. Taiwan)
Tim Graber (U. of Chicago)
Abhay Shukla (Universit ´e Pierre et Marie Curie)
Jean-Pascal Rueff (Synchrotron SOLIEL)
sq , 1
VS
q , 2Im
G G
q
G ,
Non-Resonant Inelastic X-Ray Scattering (NIXS)
[hkl]
sample
Detector
Spherically BentAnalyzer Crystal
q
UNI-CAT ID-337.59 keVE ~ 1.1 eVIo ~ 5•1012 Hz
UNI-CAT ID-33CHESS C-LineE ~ 0.3 eVIo ~ 1011 Hz
100
100
100110
110
110
111
IXS Measurement Directions
Sq , 2V Im
G ,
G
q
G ,
Absolute Response CalculationsAbsolute IXS Measurements
New in-gap features at large q! What are these excitation? Strong angular dependence? (100) != (111) Difference between NiO & CoO?
25
20
15
10
5
0s(
q,
)
(eV
-1n
m-3
)302520151050
²E (eV)
CoO (1.1 eV Res.)
(111) (100)
2.0 A-1
7.0 A-1
25
20
15
10
5
0
s(q
,
) (e
V-1
nm
-3)
302520151050
²E (eV)
NiO (1.1 eV Res.)
(111) (100)
2.0 A-1
7.0 A-1
Strong Within-Mott-Gap Excitations at Large q
NiO CoO
q = 2/Å q = 2/Å
q = 7/Aq = 7/A
Charge Excitations in NoO and CoOSmall momentum transfer cases
Linear response within time-dependent density functional theory LDA+U approximation greatly improves the gap and line shape Work well at small q in absolute unit
0 10 20 30 40Energy (eV)
0.0
0.2
0.4
0.6
0.8
1.0
-Imv
0 5 10 15Energy (eV)
0.0
0.2
0.4
0.6 expLDALDA+U
NiO, q ~ 0.7 /Å
Charge Excitations in NoO at Large q
Large q excitations local d-d excitation (dipole forbidden) Strong angular dependence and nodal directions ?
0.014
0.012
0.010
0.008
0.006
0.004
0.002
0.000
s(q,
) (
eV
-1 Å
-3)
161412108642
²E (eV)
NiO (111) and (100)
q(111) = 3.5 A-1 (Meas.)
q(100) = 3.5 A-1 (Meas.)
q(100) = 3.5 A-1 (0.35 eV Res.)
q(111) = 3.5 A-1 (0.35 eV Res.)
q(111) = 3.5 A-1 (Calc.)
q(100) = 3.5 A-1 (Calc.)
B. Larson et. al, Phys. Rev. Lett. 99, 026401 (2007)
25
20
15
10
5
0
s(q
,)
(eV
-1n
m-3
)
302520151050²E (eV)
CoO (1.1 eV Res.)
(111) (100) 2.0 A
-1
7.0 A-1
25
20
15
10
5
0
s(q
,)
(eV
-1n
m-3
)
302520151050²E (eV)
NiO (1.1 eV Res.)
(111) (100) 2.0 A
-1
7.0 A-1
25
20
15
10
5
0
s(q
,)
(eV
-1n
m-3
)
302520151050²E (eV)
CoO LSDA+U = 8 eV
2.0 A-1
(111) 1.9 A
-1 (100) 7.0 A
-1 (111)
7.0 A-1
(100)
25
20
15
10
5
0
s(q
,)
(eV
-1n
m-3
)
302520151050²E (eV)
NiO LSDA+U = 8 eV
2.0 A-1
(111) 2.0 A
-1 (100)
7.0 A-1
(111)
7.1 A-1
(100)
Large-q only excitations local d-d excitation (dipole forbidden) Strong local interaction needed for correct energy How about the strong angular dependence and nodal directions ?
Linear Response & LDA+U Approximation
L
L
L
Time dependent density functional theory with LDA+U approximation:
local Fockp-h attraction
local Hartree
Hartreelong-range screening
d.c. LDAxcf w
1 21 1 2 2 , ; 1 2 1 2 ,; ; ;m m mn m n n n
mnm n
t t M L t t t t M
x xx x 1 *, 1 1m m m mM x x x
C.-C. Lee, H.-C. Hsueh, and Wei Ku, to be published
Real-Space Picture of Local Excitons
d x 5
eg x 2
t2g x 3
eg x 2
a1g x 1
e’g x 2
2 21 3ge z r 2 22 3ge x y
1 1 3 1 3 2ge yz zx xy
1 : 2ga yz zx xy
2 1 3 1 3 2ge yz zx xy
F of NiO
F of CoO
ˆ
1
ˆ
1
, ; 1,1 ;1 ,1;1 1 1 1i ie ew L w
q x q xq q
L
Energy-resolvedWannier orbitals
X-ray sees this
particle
hole
EF
e’g
eg
Local Excitations in NoO and CoOPoint group symmetry and new selection rules
Local point group symmetry nodal directions new selection rules
Anisotropy of Local Excitations
Nodal direction point group symmetry Lack of [100] node in CoO weak symmetry breaking
B. Larson et. al, Phys. Rev. Lett. 99, 026401 (2007)
Local Excitations in NoO and CoOSensitive probe of weak symmetry breaking
Lost of nodal directions : extremely sensitive to weak symmetry breaking Visualization of symmetry breaking via Wannier functions
NiO CoO
NiO CoO
CoO NiO
Formation of Frenkel Excitons in Local Picture
p1 h1
p1 h1
same pairp-h attraction
+
p1 h1
p1 h1
Hybridization of Frenkel Excitons in Wannier basis
local Fock
+
p1 h1
p2 h2
local Hartree
+
p1 h1
p1 h1
Tightly-Bound Excitons in Charge Transfer Insulators:case study of LiF
P. Abbamonte et. al., to be published
Tightly bound exciton
Charge transfer insulator
p-h in different atoms
Frenkel or Wannier exciton ?
Inelastic X-ray scattering
Structured spectral weight
Clear dispersion at large q !
observe fs dynamics
20
15
10
5
0
-5
-10
½ x
y z
x
yz
½ ½
Excitons in LiF as a Frenkel Exciton in a “Super Atom”
q = 0~1.5 Intensity divided by 2.60 1 2 3 4
161412
10
x
y
z
3 3 5
x
yz
½
Matrix Element and Structure in q-space
real-space
q-space
Effective Two-Particle Hopping
1 21 1 2 2 , ; 1 2 1 2 ,; ; ;m m mn m n n n
mnm n
t t M L t t t t M
x xx x 1 *, 1 1m m m mM x x x
C-L Yeh, H.-C. Hsueh, and Wei Ku, to be published
Define effective two particle kinetic kernel T vialocal
local
Propagation of exciton L L
L
L
local
local
T gives hopping of p-h pair in real space dispersion in q-space
Effective Two-Particle Hopping in LiF
C-L Yeh, H.-C. Hsueh, and Wei Ku, to be published
T() is complex and strongly -dependent to fully account for1. Landau continuum2. Lower mobility with stronger p-h binding
Re{T()} Im{T()}
(0,.5,.5) (0,.5,.5)
(0,0,1) (0,0,1)
within the continuum fast decay
NN hopping dominant cos() like dispersion
Time Evaluation of Charge Fluctuation in LiF
at the source of perturbation well defined averaged frequency steady decay in time
t ( fs )
Lph
,hp (
R, t
) *
4(0, 0, 0) * 22Lph,hp ( q , )
(
eV)
q (reciprocal lattice unit)
Propagation of Frenkel Excitons
(0, 0.5, 0.5) * 0.72
(0, 1, 1) * 1.42
(0, 1.5, 1.5) * 2.12
t ( fs )
Lph
,hp (
R, t
) (
scal
ed b
y R
2 )
along the (011) “direct” path efficient propagation steady group velocity
t ( fs )
Lph
,hp (
R, t
) (
scal
ed b
y R
2 )(0, 0, 1) * 12
(0, 0, 2) * 22
along the (001) “indirect” path velocity decreases interference due to multiple scattering
Propagation of Frenkel Excitons
Non-resonant IXS measurement vs. theory in absolute unit Non-resonant inelastic scattering at large q
sub-atomic spatial resolution beyond dipole selection Strong anisotropy & nodal directions of spectral weight at large q
direct access to spatial distribution of underlying orbital local point group symmetry new selection rules Clearer signature of dispersion at large q
propagation of excitations in space and time good (space, time) resolution: ( a0, fs )
Theory of local dynamics based on 1st-principles Wannier function real-space picture of local excitons and their propagation visualization of particle holes pairs and their nodal directions suitable for charge-transfer & more itinerant systems applicable for exciton decay near surfaces and in nano-systems Potential applications in correlated materials (orbiton, polaron, phason …)
Conclusion
The Correspondence is Less Direct With Resonant Emission X-ray Spectroscopy (REXS) And Cluster Calculations
REXS Observes A Range of Gap Excitations In NiO and CoO
0.05
0.04
0.03
0.02
0.01
0.00
s(q,
)
( e
V -
1 Å
-3)
3.5eV3.02.52.01.5²E (eV)
NiO
q = 7 (Å-1
)
Along (001) Along (111)
~1.3 eV
IXS
0.025
0.020
0.015
0.010
0.005
0.000
s(q,
)
(eV
-1 Å
-3)
3.0eV2.52.01.51.00.5
E (eV)
CoO<111>
q = 7 A-1
~1.4 eV
IXS
IXS Peak Positions
REXS
Butorin et al., PRB 54, 4405 (1996)
The Non-Resonant X-Ray Scattering Observations Are Similar to Spin-Polarized Resonant-Exchange Electron Scattering In NiO and CoO
Fromme et al., PRB 75, 693 (1995)
NiOC-SPEELS
0.05
0.04
0.03
0.02
0.01
0.00
s(q,
)
( e
V -
1 Å
-3)
3.5eV3.02.52.01.5²E (eV)
NiO
q = 7 (Å-1
)
Along (001) Along (111)
~1.3 eV
IXS
0.025
0.020
0.015
0.010
0.005
0.000
s(q,
)
(e
V -
1 Å
-3)
3.0eV2.52.01.51.00.5
E (eV)
CoO<111>
q = 7 A-1
~1.4 eV
IXS