Upload
heather-osborne
View
227
Download
2
Tags:
Embed Size (px)
Citation preview
Effects of supersaturation on the crystal structure of gold seeded III–V nanowires
1Jonas Johansson, 2Lisa S. Karlsson, 1Kimberly A. Dick, 1Jessica Eriksson, 1Brent A. Wacaser, 1Knut Deppert, and 1Lars Samuelson
1Solid State Physics and the Nanometer Structure Consortium, Lund University, Sweden
2National Centre for High Resolution Electron Microscopy (nCHREM) / Polymer & Materials Chemistry, Lund University, Sweden
Introduction• High density of planar defects in III-V
nanowires with zinc blende structure. This can be tuned by growth conditions.* **
• Can we radically change the crystalline properties of gold seeded III–V nanowires by growth at different conditions:– Pulsed growth– Altered seed particle
• Can we find growth conditions that let us grow pure zinc blende or wurtzite wires?
• Can we also find a sharper condition for wurtzite formation in zinc blende nanowires than what has recently been proposed?***
*J Johansson et al, Nat Mater, 5 574 (2006): GaP at 440, 470, and 500°C
**H Joyce et al, Nano Lett, 7 921 (2007): GaAs at 450-390°C
***F Glas et al, Phys Rev Lett, 99 146101 (2007): ΔGWZ < ΔGZB
Stacking sequences
Zinc blende: ABC…
Wurtzite: AB…
fault plane
(twinning)
fault plane
fault plane
(wurtziteformation)
zinc blende
Experimental
• Growth of GaP(111)B nanowires on GaP(111)B substrates in MOVPE at 470°C.
• Growth seeded by aerosol fabricated gold particles, 40 nm diameter.
• Precursors: TMG and PH3.
• In contaminated or clean (In free) susceptor.• Pulsed growth or continuous growth.
• Pulsed growth:– TMG: 10 s ON, 1 min OFF– 20 pulses
– PH3 always ON
• HR TEM for structural characterization
Nanowire growth resultsPulsed growthIn background
Continuous growthIn background
Continuous growthIn free background
Extended zinc blende (ZB) segmentsAverage: 20 MLMaximum: 200 ML
Short ZB segments (lamellar twinning)Average: 3.5 ML
Wurtzite (WZ) segmentsAverage: 3.5 MLMaximum: 21 ML
Composition of the seed alloy particle• EDS measurements of the Ga and In concentrations in the gold alloy particle
• Two different growth terminations• Cooling down in
– H2: Ga concentration during growth, C– PH3 + H2: Ga concentration at eqiulibrium, Ceq
• Conclusion: higher supersaturation during In free growth– In background: C/Ceq ≈ 1–3 – In free: C/Ceq ≈ ~10
In background In free background
H2 PH3 H2 PH3
In (at-%) 20 – 30 20 – 30 0 – 5 0 – 5
Ga (at-%) 0 0 20 – 26 0Detection limit ≈ 3 at-% (0 means less than 3 at-%)
Growth at different supersaturationsPulsed growthIn background
Continuous growthIn background
Continuous growthIn free background
Extended zinc blende (ZB) segments
Short ZB segments (lamellar twinning)
Extended wurtzite (WZ) segments
low Supersaturation (, C/Ceq) high
Nucleation description• Two assumptions for the nucleation model:
– (i) Layer-by-layer growth, monocenter nucleation at wire edge
– (ii) Poissonian nucleation
• Justifications– (i) Perfect atomic planes in
the wires (no grain boundaries),very low P solubility in Au
– (ii)
2
exp1 s
sf
ms = 4.2 ML
2D nucleation model
rrrG 22
22
0 for ordinary planet for fault plane
Step energy eih 2
eqc
B
C
C
s
Tkln
0 rG
Finding the nucleation barrier for ordinary and fault plane nucleation
2
2*G f
ffG
2
2* f
Nucleation barrier
r
ΔG(r)
ΔG*
r*
rrrG 22
22
Possibility for wurtzite formation?• Fault plane nucleation is favoured:*
• Can happen if Γf < Γ– Inner step energies same: γi
f = γi
– Edge step energies differ: γef < γe
• Rewrite ΔG-inequality:
– Not much data… If step energies follow surface energies, for ZnSf ≈ 0.6–0.7 (WZ σav = 0.57 J/m2, ZB σav = 0.86 J/m2)**
• Is this relation sufficient for the wurtzite structure to form?
** GG f
**H Zhang et al, J Phys Chem B, 107 13051 (2003) *F Glas et al, PRL, 99 146101 (2007)
fft
114
2 2
1 efef
Nucleation probabilities
• Nucleation rates:
• Fault plane nucleation probability
TkGJ B*exp
TkGJ Bff*exp
f
ff JJ
Jp
Poissonian nucleation
• Can we relate the fault plane nucleation probability, pf, to segment thicknesses?
• Poissonian nucleation: the (geometric) probability distribution of nucleating exactly k fault planes, that is a k ML thick WZ segment, before an ordinary nucleus forms
• The average WZ segment thickness (the average value of k)
,2,1,0,1 kpp fkf
f
fWZ p
ps
1
Interpretation of growth results
swz = 3.5, pf = 0.78
sZB = 3.5, pf = 0.22
sZB = 20, pf = 0.05
Pulsing
Continuous
In-free
Condition for WZ formation revisited
• Fault plane nucleation is favoured when
• Does this mean that WZ formation will occur?
• This is a matter of definition…
• By combining the equations for pf and swz, we can pose a stronger condition for WZ formation:
** GG f
** ln GsTkG WZBf