exciton effect of the resonance window of swnts · exciton effect of the resonance window of swnts...
TRANSCRIPT
Exciton effect of the resonance
window of SWNTs
1Department of Physics, Tohoku University, Sendai, Japan2Department of Mechanical Engineering, University of Tokyo, Tokyo, Japan
J. S. Park1, K. Sato2, R. Saito1
The 2nd GCOE International Symposium
• No destructive, No contact Measurement
– Room Temperature at Ambient Pressure
– Quick (1min)
• Standard tool for Nano-Technology
Raman Spectroscopy of CNTM. S. Dresselhaus, et.al. Physics Reports, 409, 47-99, (2005)
Background
One dimensional structure
Chiral vector (n,m) determines physical properties of CNT.
Metallic and semiconducting electronic structure
Carbon nanotube
Raman Spectroscopy
1nm
1m
(5,5)
Metallic Semiconducting
EFEF
(9,0) (10,0)
Ch
T
Ch=na1+ma2= (n,m)
na1ma2
As-grown purified
CoMoCAT SWNTsSDS + SWNTs
Population (P) =IEXP(RBM)
ICAL(RBM)
S:M=1.2:1 S:M=2.4:1
If consider the calculated RBM intensity,
S:M=11:1
A. Jorio et al., PRB (2005)
Motivation: Population of SWNTs with RRS
Population by summation of experimental RBM intensity
(n,m) dependent P(IEXP/ICAL)
M
S
M
S
Precise nanotubes population
Calculation of precise Raman cross-section
Exciton-phonon matrix, excition-optical matrix, (Resonance width)Jiang, et.al. PRB (2007) Park, et.al. PRB (2006)
M
G+G-
G-
S-SWNT
M-SWNT
G+
[cm-1] G+ G-
S-SWNTs 1590 1570
M-SWNTs 1590 1550
Kohn anomaly effect in
Metallic SWNTsS.D.M. Brown et al., Phys. Rev. B63, 155414 (2001)
A. Jorio et al., Phys. Rev. B65, 155412 (2002)
Chirality dependence of
the experimental G band
Z. Yu, et al. J. Phys. Chem. B,
105, 6831 (2001)
Outline of this presentation
1. Raman spectra of single wall carbon nanotubes
- Radial Breathing Mode and G band
- Kohn anomaly effect of metallic-SWNTs
2. Exciton effect of Raman resonance window- Introduction of previous calculation
- Exciton-phonon scattering process
Intra-valley scattering
Inter-valley scattering (in future work)
3. Summary
Calculation of Raman spectra (RBM, G)
Raman Intensity I(, EL)
phonon
energy K ELk
j
a
b
resonance
window
Laser
energy
ex-ph
matrix
optical
matrixoptical
matrix
K. Sasaki, et al. Phys. Rev. B 77, 245441 (2008)
ex
Original
frequencyFrequency shift
2
Kohn anomaly
effect for metallic tube
Raman spectra = Raman intensity + Spectral width (const.)
G band Raman spectra
ELaser = E11Low
TOLO
LO
J. S. Park, et al. Phys. Rev. B 80, 081402 (2009)
TO
LO
M-SWNT ELaser = E22S-SWNT
k11
10 Mel-ph
(15,0)TO
k11
10 Mel-ph
(15,0)LO
Mel-phk
Chiral angle dependence of KA for G band
Zigzag Armchair
Why TO becomes hard for zigzag NT?
Q dependent el-ph interaction
LO:
TO:
Chiral
K. Ishikawa and T. Ando, J. Phys. Soc. Jpn. 75, 84713 (2006).
T. Ando, J. Phys. Soc. Jpn. 77, 14707 (2008).
K. Sasaki, R. Saito, et al. Phys. Rev. B, 77, 245441 (2008)
TOLO
TO
LO LO
EF>0
EF<0
(11,8)
Gate voltage dependence of G band Raman spectraJ. S. Park, et al. Phys. Rev. B 80, 081402 (2009)
Metallic RBM Raman spectra
ELaser = E11Low
Ex-ph matrix elements &
Resonance windows
Zigzag
Armchair
(15,0)
(10,10)
(13,4)
(11,8)
(12,6)
(14,2)
q=0
RBM
A
Z
k22
10 Mel-ph
(10,8)
S1
k22
10 Mel-ph
(10,9)
S2
S1 Type
S2 Type
Chiral angle dependence of ex-ph interaction
semiconducting
S1 Type S2 Typemod(2n+m,3)=1 mod(2n+m,3)=2
S1
S2
Experimental 2D RBM Raman plot
ii
Resonance
window
EL=Eii EL Eph
ab
i
valence
band
conduction
band
Resonance
point
ħ
ħ
ħ
el-ph AD1 AD2
additional effect
(ex. el-op scattering)
Resonance window
- Inverse lifetime of a
photo-excited electron
Resonance Raman window
MIT
Experimental resonance window
Brazil
Calculated values
(S1) > (S2) in the diameter (>0.9nm) range
Resonance window for S-SWNTs
For 0.6 < dt < 1.5nm
S1 type
S2 type
semiconducting
(8,0), (7,2), (9,1), and (11,0) SWNTs
: small value compared to other S1 tubes
Diameter and chirality
dependence
0.9 nm
S1 Type
S2 Type
mod(2n+m,3)=1
mod(2n+m,3)=2
Comparison with the experiment
Semiconducting SWNTs
Correlation
Ex
pe
rim
en
t
Calculation
Experiment(Brazil)
EX 15 meV
S1 Type
S2 Type
Experiment (MIT)
F=38(S)
F=30(M)
E33S
E11ML
E22S
Calculation
Exciton-phonon scattering processes
Intra-valley scattering
k
kq
kq1
k
kq
kq2
Bright
exciton
Bright
exciton Bright
excitonDark
exciton
Intervalley Scattering
A exciton
ehK
KK
E exciton
e
h
K
KK
not vertical transition
A- : bright exciton
A+, E and E*: dark excitons
RBM and LO phonon
LO
RBM
TO
S1
S2
Open circle : el-ph
Filled circle : ex-ph
TO phonon
Ex-ph Intra-valley scattering
Exciton-phonon
interactionElectron-phonon
interaction
Mel-phk
k
Mex-ph
Why ex-ph is smaller than el-ph?
Mel-ph
Constant for k
k
Mel-ph
Mex-ph
Not constant for k
Exciton-phonon interaction
Summary
1. Chirality dependence of RBM and G band Raman intensity
RBM : Zigzag > Armchair
G : only one peak appears in Zigzag CNT.
2. Resonance window
exciton-phonon Intravalley scattering
: Bright exciton (A-)
exciton-phonon Intervalley scattering
: Bright(A-) and Dark (E or E*) exciton
3. Ex-ph interaction < el-ph interaction
- Localization of exciton
- El-ph interaction dependence on k.
Gate voltage dependence of metallic RBM Raman spectra
(12,0) (9,6) (8,8)
EF=0.6eV
EF=0.6eV
Ram
an inte
nsity, a. u.
200180160140
Raman shift, cm -1
0 V
-0.5 V
0.5 V
-1.5 V
1.5 V
-1.0 V
1.0 V
EXP
Sasaki-san
Jiang-san
RBM for (10,10)
Goff = 6.4 eV
Gon = 3.0 eV
Resonance window- Inverse lifetime of a photo-excited electron (uncertainty principle)
EL=Eii EL Eph
ab
i
valence
band
conduction
band
Resonance
window
ii
Raman excitation profile
Resonance
point
ħ : relaxation time of transition
from an initial k state to all possible
final k states
ħ
ħ
ex-ph AD1 AD2
additional effect
(ex. ex-op scattering)
Fermi Golden rule
ex
Symmetry of Excitons
A
Bright and dark exciton
A- : bright exciton
A+, E and E*: dark excitons
J. Jiang et al. Phys. Rev. B75 035405 and 035407(2007)
E exciton
e
h
K
KK
C2
ehK
KK eh
K
KK
ehK
KK
00exciton dipole transition matrix
Eigen states are irreducible representation
for C2 rotation (odd or even).
not vertical transition
A+ even A- odd
oddodd
A exciton
ehK
KK
Resonance window for intravalley scattering
Type I
Type II
O Ec2-c1
Eph < Ec2-c1
c2
c1
Resonance
Exciton-phonon interaction
Exciton-phonon scattering processes
Intravalley scattering (2) Intervalley scattering(2)phonon(6)=24
1. Intravalley scattering
O Ec2-c1
Eph < Ec2-c1
c2
c1
Resonance
2. Intervalley scattering
kk+q
Ram
an inte
nsity, a. u.
200180160140
Raman shift, cm -1
0 V
-0.5 V
0.5 V
-1.5 V
1.5 V
-1.0 V
1.0 V
Gate dependent resonance Raman excitation profile
M. Kalbac et al, unpublished.
Ra
ma
n in
ten
sity,
a.u
.
-1.5 -1.0 -0.5 0.0 0.5 1.0 1.5
Electrode potential, V vs. Ag/Ag+
2.067 eV
2.084 eV
2.120 eV
2.138 eV
2.102 eV
M
Ram
an in
tensi
ty,
a.
u.
-1.5 -1.0 -0.5 0.0 0.5 1.0 1.5
Electrode potential, V vs. Ag/Ag+
1.653 eV
1.687 eV
1.699 eV
1.710 eV
1.722 eV
1.734 eV
1.746 eV
1.676 eV
Ram
an in
tensi
ty, a. u.
200150
Raman shift, cm -1
16001500
x10
S
A- : bright exciton
A+, E, E*: dark excitons
E exciton
e
h
K
KKA++A- exciton
ehK
KKeh
K
KK
A+-A- exciton
E* exciton
e
h
K
KK
inter-valley
scattering
(fast!)
D-band, G’-band
exciton-phonon interaction
- breaking symmetry -
EF dependence of the G band
Raman spectra for metallic tubes
LO
softeningTO
noshiftLO
softening
TO
hardening
LO
softening
Armchair – TO mode not shift
Chiral tube – both TO and LO shift
Zigzag – LO softening
EL
j
a
b
G band Raman scattering process
a point
: resonance point
ab process
: el-ph scattering
Original
frequencyFrequency shift
2
Kohn anomaly
effect for metallic tube
What is the Kohn Anomaly
Hard
Soft
Low energy el-hole pair – TO hardening
High energy el-hole pair – LO softening
El-ph matrix for the el-hole pair creation
F : Fermi velocity
: Pauli matrix
g: el-ph coupling constant
A: Deformation-induced gage field
u: Relative displacement vector
El-hole pair
energy
K. Sasaki, et al. Phys. Rev. B 77, 245441 (2008)
El-ph matrix elements for Raman scattering processK. Sasaki, et al. Phys. Rev. B 77, 245441 (2008)
Armchair (=30)
QR(k)
QR(k)
Calculation of Raman spectra (RBM, G)
G band Raman spectra = Intensity Spectral width
1. Raman Intensity I(, EL)
phonon
energy
K ELk
j
a
b
resonance
window
Laser
energy
ex-ph
matrix
optical
matrixoptical
matrix
2. Spectral width
Phonon energy
Original
frequency
Correction frequency
Including el-ph coupling
Spectral
width
Electron-hole pair creation matrix
by el-ph interaction
electron
energy
hole
energy
Fermi distribution function
Spectral width is given by the decay length .
K. Sasaki, et al. Phys. Rev. B 77, 245441 (2008)
Kohn anomaly effect
ex