excitonic aharonov-bohm effect in type-ii quantum...
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Excitonic Aharonov-Bohm Effect in Type-II Quantum Dots
Igor L Kuskovsky Department of Physics
Queens College of CUNY, Queens, NY 11367
Acknowledgements
B. Roy (QC) H. Ji (QC) S. Dhomkar (QC) M. C. Tamargo (CCNY) D. Smirnov (NHMFL) Y. Kim (NHMFL) J. Ludwig (NHMFL)
L. Mourokh (QC) A. O. Govorov (Ohio U.) F. Peeters (U. Antwerp) M. Tadic (U. Belgrade) I. C. Noyan (Columbia U) U. Manna (Columbia U)
Aharonov-Bohm Effect Classical electrodynamics: the vector potential, A, is
considered a mere mathematical auxiliary -- convenient for calculations, but having no direct physical meaning
Quantum mechanics: the potential(s) play a more significant role, for the Hamiltonian is expressed in terms of ϕ and A, not E and B: Nevertheless, it was taken for granted that there could be no
electromagnetic influences in regions where E and B are zero
In 1959 Aharonov and Bohm showed that the vector potential can affect the quantum behavior of a charged particle even in regions where electromagnetic field is zero (a magnetic flux exists, while no effects of the classical Lorentz force are present)
Aharonov-Bohm Effect
Consider an electron on a circular orbit with and without presence of a Solenoid (the bound Aharonov-Bohm Effect) Solenoid lifts two-fold (direction of rotation) degeneracy The energy of a [positive] particle moving along the current of the
solenoid (l > 0) is lowered The energy now depends on the magnetic filed inside the solenoid,
although the magnetic filed at the particle’s location is ZERO
2
2
2
2
22
2
2
0 0 ... ,2 ,1 ,0 ,
Φ−==
≠Φ=Φ±±==
hqll
ill
lmR
EmR
lE
le
φψ
Aharonov-Bohm Effect
Excitonic-AB Effect in Magneto-PL
As the flux increases, |L| changes from 0 to 1, 2, 3 …
Two important outcomes: Energy Oscillation(s) (“known”) PL Intensity Oscillation(s) - due
to selection rules Multiple Oscillation in strong
confinement or weak coupling A single ‘peak’ in strong coupling
regime
• The Excitonic [“Optical”] AB Effect refers to manifestation of the Aharonov-Bohm phase in the optical emission of polarized excitons [“dipoles“] – overall neutral quasi-particle
• Quantum Rings and Type-II Quantum Dots
e.g., Kalameitsev, et al., JETP Lett. 68, 669 (1998); Govorov, et al., PRB RC 66, 081309 (2002); Janssens, et al., PRB 67, 235325 (2003)
BRRR he 0)(2 −=∆Φ π
he llL +=
2
020
2
0 2
Φ
∆Φ++= L
MREE excexc
2/)(0 he RRR +=
20
22 )(R
RmRmM hhee +=
Excitonic-AB Effect in Magneto-PL The 1st transition of the electron orbital number to non-zero
value occurs at the magnetic field BAB for which,
0 1 2 3 4 5
Excit
on En
ergy (
arb. u
nits)
Φ/Φ0
le = 0 le = -1 le = -2
20
AB20
Φ=BRπ
meV 5.0~8
2
20
2
2
020
2
0
MRE
LMR
EE
exc
excexc
=∆
Φ
∆Φ++=
Excitonic-AB Effect in Magneto-PL
The ground sate for a QR,
No transition to dark states is expected without external fields, e.g., electric field*
Romer and Raikh, PRB 62 7045 (2000); *Fischer, et al., PRL 102, 096405 (2009)
ΦΦ
+−∝∆ −e πργπ 2
0
00 2cos1
Type-II Heterosturctures In Type-II heterostructures,
the charge carriers are spatially separated
• In QDs: one type of carriers is confined within the QD whereas the other is attracted via the Coulomb interaction, creating spatially indirect (type-II) exciton • Electrical dipole across interface is formed
In ideal type-II QDs the ‘barrier’ carrier would locate above-below the QD
Kuskovsky, et al., PRB 76, 035342 (2007)
Blue = Highest Electron Density
Type-II Quantum Dots: Examples
2.2 2.3 2.4 2.5 2.6 2.7 2.8
10-4 10-3 10-2 10-1 100
2.4
2.5
2.6
2.7
2.8
2.9
3.0
3.1
T = 10K
Blue band Green band 1 Green band 2 Linear fit I1/3
ex
PL P
eak
posi
tion
(eV)
Excitation Intensity (arb. units)
Iex = 0.0001Imax
Inte
nsity
(arb
. uni
ts)
Energy (eV)
Blue band Green band 1 Green band 2
Iex = 0.1Imax
• cw PL – Emission energy shifts
to higher values with increasing excitation
Roy et al., Eur. Phys. J. B, 86, 31 (2013)
Type-II Quantum Dots: Examples
0 50 100 150 200 250
0.01
0.1
1
10
0 100 200 300
0.01
0.1
1
PL In
tens
ity (a
rb.u
.)
Time (ns)
calculated Iexc
1
Iexc2
Iexc3
Iexc1 >Iexc
2 >Iexc3
PL In
tens
ity (a
rb.u
.)
Time (ns)
• Time-resolved PL – Long-lived due to weak
overlap of the carriers’ wave functions
– Dependent on Iex, for overlap of the wave functions depends on the concentration of photo-generated carriers
Gu et al., PRB 71, 045340 (2005); Shuvayev et al., PRB 79, 115307 (2009)
Type-II Exciton Lifetimes and Binding Energies from Temperature Dependent TRPL
0 0
1 1 1[1 exp( / )] exp( / )b B a Br nr
C k T k Tε ετ τ τ
= − − + −
0.0 0.2 0.4 0.6 0.8 1.0 1.2
0.010
0.015
0.020
0.025
0.030
1/
τ (ns
-1)
Sample C2.34 eV
1/kBT (meV-1)
~130 K
Yi, et al., PRB 71, 045340 (2005); Ji, et al., J. Electr. Mat. 42, 3297 (2013)
Ionization/Re-capture
Type-II Exciton Lifetimes and Binding Energies from Temperature Dependent TRPL
0 0
1 1 1[1 exp( / )] exp( / )b B a Br nr
C k T k Tε ετ τ τ
= − − + −
Sample Photon Energy
(eV)
Exciton Binding Energy (meV)
𝝉𝒓𝟎 (ns)
Activation Energy (meV)
𝝉𝒏𝒓𝟎 (ns)
A 2.48 6.20 64.7 90.7 0.10
B 2.48 7.34 91.9 103.0 0.15 2.36 7.44 93.1 111.1 0.18
C 2.34 11.30 99.9 83.1 1.37
Yi, et al., PRB 71, 045340 (2005); Ji, et al., J. Electr. Mat. 42, 3297 (2013)
Disk-like Type-II QDs in Magnetic Field
Blue = Highest Electron Density M
agne
tic F
ield
No AB Effect
Kuskovsky, et al., PRB 76, 035342 (2007)
Single Type-II QD: Strain The AB effect was observed is
InP/GaAs QDs (Ribeiro, et al., PRL, 92, 126402 (2004))
However, no oscillations were observed by de Godoy, et al., in the same system (PRB 73, 033309 (2006))
Madureira, et al., APL 90, 212105 (2007) showed that the ability to observe it depends on the growth conditions and specifics of the system
Single Type-II QD: Strain The AB effect was observed is
InP/GaAs QDs (Ribeiro, et al., PRL, 92, 126402 (2004))
However, no oscillations were observed by de Godoy, et al., in the same system (PRB 73, 033309 (2006))
Madureira, et al., APL 90, 212105 (2007) showed that the ability to observe it depends on the growth conditions and specifics of the system
Stacked Type-II QDs
Blue = Highest Electron Density
No AB Effect Possible • Red = Highest Electron (Hole) Density at
0 T (upper) and 6 T (lower)
AB effect is Possible
Mag
netic
Fie
ld
Samples MEE-MBE Shutter Sequence
Schematic of the Samples
Kuskovsky, et al., PRB 63 155205 (2001);PRB 76, 035342 (2007)
n = 1 or 3
Example: ZnMgTe/ZnSe
Manna et al, JAP 111, 033516 (2012)
• XRD simulations showed • A minimal amount of Te (< 1%)
inside the spacer • ~ 32% of Mg inside the QDs
Quantum Dots Form Stacks, which results in “averaging” out QDs size variations
Strain cannot be completely ruled out
Qualitative Model
Kuskovsky, et al., PRB 76, 035342 (2007); Dhomkar, et al., APL 103, 181905 (2013); Manna, et al., JAP 111, 033516 (2012); Ji et al., (2014) - unpublished
-0.50 -0.45 -0.40 -0.35 -0.30 -0.25 -0.20
-0.03
0.00
0.03
q x(A-1)
SL(-1)SL(-2)
10-5 10-4 10-3 10-2 10-1 100103
104
105
106
107
108
109
Slope = 1.02
Int.
PL In
tens
ity (a
rb. u
nits
)
Excitation Intensity (arb. units)
D47T = 9.0 K
The AB Signature in PL Intensity
2.1 2.2 2.3 2.4 2.5
D47, 1.5 NDFT =5.4 K
6.00 T 4.00 T 2.00 T 1.39 T 0.65 T 0.00 T
Inte
nsity
(arb
. uni
ts)
Photon Energy (eV)-6 -4 -2 0 2 4 6
2450
2500
2550
2600
2650D47, 1.5 NDFT =5.4 K
Int.
Inte
nsity
(arb
. uni
ts)
Magnetic Field (T)
• The AB peak is only observed in Faraday Configuration, as expected • The AB signature is ‘masked’ at high excitation intensities
The AB Signature in PL Intensity
• The AB peak is only observed in Faraday Configuration, as expected • The AB signature is ‘masked’ at high excitation intensities
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5
D47, 1.5 NDFT =5.4 K
Int.
Inte
nsity
(arb
. uni
ts)
Magnetic Field (T)
4.7%
BAB ~1.40 T
AB Signature in Intensity of Polarized PL
-20 -10 0 10
0.4 0.8 1.2 1.6 2.0 2.4
Inte
grat
ed In
tens
ity (a
rb. u
nits
)
Magentic Field (Tesla)
D47, T = 1.9 K
Inte
grat
ed In
tens
ity (a
rb. u
nits
)
Magentic Field (Tesla)
~1.37 T
~15.2%
The AB ‘peak’ appears only in one polarization Largest reported
magnitude Possibly was masked by
some background emission
AB Signature in Energy of Polarized PL
-15 -10 -5 0 5 10 152.28
2.29
2.30
2.31
2.32
2.33
2.34
2.35
2.36
Ener
gy (e
V)
Magnetic Field (T)
0.9000
0.9167
0.9333
0.9500
0.9667
0.9833
1.000D47T = 0.36K
The AB energy peak also become evident in polarized PL
meV 5.0~8
2
20
2
2
020
2
0
MRE
LMR
EE
exc
excexc
=∆
Φ
∆Φ++=
The AB Signature in PL Intensity
Magnetic field of the 1st angular momentum transition increases with decreasing Te concentration
Attribute to ‘size’ of QDs
Correlating with PL at zero magnetic field, allows to estimate QD density*, binding energy of excitons*, as well as the in-plane size of type-II exciton** 0 1 2 3 4
0.3
0.6
0.9
1.2
1.5
1.8
~ 1.85 T
~ 1.90 T
~ 2.08 T
~ 1.42 T
~ 1.88 T~ 1.88 T
Norm
. Int
. Int
ensi
ty (a
rb. u
nits
)
Magnetic Field (T)
~ 2.06 T
Kuskovsky, et al., PRB 76, 035342 (2007); *Ji et al., – unpublished; **Roy et al., APL 100, 213114 (2012)
‘Spectral Analysis’
• ‘Double peak’ in the AB oscillation points to at least two different QD stacks, with corresponding type-II exciton sizes of 18.2 & 17.9 nm
• TRPL at B = 0 also confirms two distinct decays in these spectral regions.
• There is a non-monotonic change in the AB oscillation magnitude
0.00.20.40.60.81.0
2.0
2.1
2.2
2.3 2.4 2.5 2.6 2.7 2.8
2.0
2.5
3.0
3.5
Nor
m. P
L (a
rb. u
nits)
a)
B AB (T
)
b)
Peak
Cou
nts (
%)
Energy (eV)
c)
Roy, et al., APL, 100, 213114 (2012); PRB, 86, 165310 (2012); *ErJPB 86:31, 1 (2014)
‘Spectral Analysis’
• ‘Double peak’ in the AB oscillation points to at least two different QD stacks, with corresponding type-II exciton sizes of 18.2 & 17.9 nm
• TRPL at B = 0 also confirms two distinct decays in these spectral regions.
• There is a non-monotonic change in the AB oscillation magnitude
0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0
~2.15 T~1.98 T
D50 2.465 eV 2.520 eV 2.641 eV
PL
Inte
nsity
(arb
. uni
ts)
Magentic Field (T)
~2.15 T
~1.98 T
Roy, et al., APL, 100, 213114 (2012); PRB, 86, 165310 (2012); *ErJPB 86:31, 1 (2014)
0 50 100 150
0.01
0.1
1
Nor
mal
ized
Inte
nsity
(arb
. uni
ts)
Time(ns)
2.43 eV 2.48 eV 2.53 eV 2.58 eV 2.63 eV 2.69 eV 2.75 eV
Sample B T= 9K
Type-II QDs in Single-Cycle Samples
0 5 10 15 20
T = 4.2K
Inte
grat
ed P
L In
tens
ity (a
rb. u
nits
)B (T)
~2.1T
• Samples that did not exhibit “type-II behavior” at low temperatures at zero magnetic field
Kuskovsky, et al., Supperlattices & Microstruct., 47, 87-92 (2010)
Type-II QDs in Single-Cycle Samples The QD related PL appears at elevated
temperatures, and behaves the same as that observed for samples grown with three Zn-Se-Te cycles
Kuskovsky, et al., Supperlattices & Microstruct., 47, 87-92 (2010)
Built-in Electric Field?
Was proposed by Fischer et al., [PRL 102, 096405 (2009)] as caused by an in-plane electric field
Samples with low amount of Te exhibit relatively narrow AB ‘peak’, which indicates a presence of built-in electric fields
Roy, et al., PRB, 86, 165310 (2012)
Decoherence of the AB Excitons
Attempt to use excitonic AB effect to study quantum decoherence
It is inherently a contactless approach Decoherence of the AB excitons
should be of the same nature as that of AB oscillations observed in transport
0 1 2 3 4
Int.
Inte
nsity
(arb
. uni
ts)
Magnetic Field (T)
Tem
pera
ture
0.3
1 -
27.1
K
0 1 2 3 4
Int.
Inte
nsity
(arb
. uni
ts)
Magnetic Field (T)
T = 27.1 K
Decoherence of the AB Excitons
∆𝐼𝐴𝐴 ∝ 𝑒𝑒𝑒 − 𝐿𝐿𝐷(𝑇)
Assuming Ballistic regime, 𝐿𝐷(𝑇) ∝ 𝜏𝐷(𝑇)
∆𝐼𝐴𝐴 ∝ 𝑒𝑒𝑒 − 𝜏𝜏𝐷(𝑇)
At high temperatures, phonon mediated decoherence dominates, and
𝜏𝐷−1(𝑇) ∝ 𝑇3
0 7000 14000 21000 28000
2
3
4
5 10 15 20 25 300
15
30
45
60
T3 (K3)
Ln(Integarted Peak PL) Linear Fit C
Ln(In
tega
rted
Pea
k P
L)
Peak AB counts Fit to v*exp[-BT3]
Inte
grat
ed P
eak
T (K)
Decoherence of the AB Excitons
1 10
1
10
1 2 3
7.5
7.8
8.1
AB
Mag
nitu
de R
(%)
Temperature (K)
AB M
agni
tude
R (%
)
Temperature (K)
1 100
2
4
6
8
τ-1D~T3
AB M
agni
tude
R (%
)
Temperature (K)
y = Cexp[-αT-β T3]
C = 8.1; α = 0.04 K-1; β = 9.2×10-5 K-3
τ-1D~T
∆𝐼𝐴𝐴 ∝ 𝑒𝑒𝑒 − 𝜏
𝜏𝐷(𝑇)
Phonon mediated decoherence
𝜏𝐷−1(𝑇) ∝ 𝑇3 Below 1÷3 K, carrier-
carrier scattering or thermal averaging dominate, so that we assume
𝜏𝐷−1(𝑇) ∝ 𝑇
Summary Polarized 2D excitons are perfect
objects to study Aharonov-Bohm effect of neutral quasi-particles
Stacked type-II QDs are among the best systems for such experiments as QD size variations are averaged out
We did observed strong AB signal in PL intensity of in stacked sub-monolayer ZnTe/ZnSe type-II QDs
Multiple sets of QDs can be detected and size of exciton is measured with sub-nanometer precision
In some samples, the observed ‘peaks’ are narrow, suggesting presence of in-plane electric fields
We have attempted to measure decoherence using contactless techniques
More detailed studies required to verify a non-monotonic behavior at
very low temperatures understand polarized magneto-PL