AASHTO-PCI-ASBI Segmental Box Girder Standards for Span-by ...
Clustering Effects in Ga(AsBi) - University of Michigan › ~mctp › SciPrgPgs › events › 2011...
Transcript of Clustering Effects in Ga(AsBi) - University of Michigan › ~mctp › SciPrgPgs › events › 2011...
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Sebastian Imhof 07/15/2010Technische Universität Chemnitz, Germany
Clustering Effects in Ga(AsBi)
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Motivation: S-Shape
Imhof et al., Appl. Phys. Lett. 96, 131115 (2010)
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Outline
● Photoluminescence in disorderd semiconductors
● Kinetic Monte-Carlo simulation● Experimental results● Two scale approach for Ga(AsBi)● Conclusion and outlook
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Disorder Model
E
Mobility edge
● Localized states randomly distributed in space
● Energies given by a certain distribution function
● N0: Area density of
localized states
X
Exciton
● α: Exciton localization radius
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Hopping of Excitons
● Excitons can move among localized states
E
X
Mobility edge
● Motion of excitons independent in the case of low densities
● Excitons can decay radiatively
X
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Hopping of Excitons
● Hopping transition given by Miller-Abrahams Indices
Mobility edge
E
X ● Excitons can decaywith life time
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Hopping of Excitons
● Hopping transition given by Miller-Abrahams Indices
Mobility edge
E
X ● Excitons can decaywith life time
● Decay rate of exciton on ith site:
● Dynamic of exciton:
● Spectra depend on three parameters:
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Explanation of the S-Shape
E2
1
3
12
3
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Kinetic Monte-Carlo Simulation
1.Calculate energies and positions of localized states
2.Choose start position of exciton randomly
3.Calculate hopping rates
4.Decide whether exciton decays or performs a hop● Decay: save the energy and restart with a new
exciton● Hopping transition: Go to step 3
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Ga(AsBi) Sample Properties
● Thickness ~30nm● Bi content: 4% - 5%● Substrate: GaAs● MBE-grown
Grown by:D. BeatonUniv. of British Columbia, Kanada
X. LuArizona State University, USA
T. TiedjeUniv. of Victoria, Kanada
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Experimental results I
● Band gap from linear absorption spectrum around 1.2 eV
● Gaussian shaped density of states at low energy tail
Stokes-Shift
Experiments done byA. Chernikov, K. Kolata, N. Köster, M. Koch, S. ChatterjeePhilipps University Marburg, Germany
Imhof et al., Appl. Phys. Lett. 96, 131115 (2010)
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Experimental results II
● Zero-temperature Stokes-shift excitation power dependent
● Maximal Stokes-shift around 110 K
● Finite Stokes-shift at high temperatures
● Disorder effects still present at high temperatures
Imhof et al., Appl. Phys. Lett. 96, 131115 (2010)
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Experimental results III
● Very broad PL spectra,FWHM at T=0 around 70meV
● FWHM has maximum at 140 K
● Sign of exponential DOS
● PL linewidth at T=0 excitation power independent
Imhof et al., Appl. Phys. Lett. 96, 131115 (2010)
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Summary: Experimental results
● Gaussian shaped low energy tail of linear absorption spectra
● Sign of Gaussian DOS
● Disorder effects still present at high temperatures
● Inconsistent with energy scale of 11 meV
● Maximum Stokes-shift at T=110 K and maximum FWHM at T=140 K
● Sign of exponential DOS with energy scale of 11 meV
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Two energy scales
● Alloy disorder of Bi only affects the valence band
E
CB
VB
● Gaussian distribution
● Additional Bi-Cluster sites beyond the valence band● Exponential
distribution
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Experiment-Theory ComparisonStokes-Shift
TheoryExperiment
Imhof et al., Appl. Phys. Lett. 96, 131115 (2010)
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Experiment-Theory ComparisonFWHM
Experiment Theory
Imhof et al., Appl. Phys. Lett. 96, 131115 (2010)
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Conclusion and Outlook
● Experimental spectra show both, Gaussian and exponential behavior of DOS
● Spectra can be fitted using the approach of two energy scales
● Next steps:● Time dependent photoluminescence spectra● Analysis of systematic sample series
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Acknowledgements
C. Wagner and A. ThränhardtChemnitz Technical University, Germany
A. Chernikov, K. Kolata, N. Köster, M. Koch, S. Chatterjee and S.W. KochPhilipps University Marburg, Germany
X. Lu and S. JohnsonArizona State University, USA
D. BeatonUniversity of British Columbia, Kanada
T. TiedjeUniversity of Victoria, Kanada
O. RubelLakehead University, Kanada
Further Details:Imhof et al., Appl. Phys. Lett. 96, 131115 (2010)