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Gold-free GaAs/GaAsSb heterostructure nanowires grown on

silicon

Citation for published version (APA):

Plissard, S. R., Dick, K. A., Wallart, X., & Caroff, P. (2010). Gold-free GaAs/GaAsSb heterostructure nanowires grown on silicon. Applied Physics Letters, 96(12), 1-3. [121901]. https://doi.org/10.1063/1.3367746

DOI:

10.1063/1.3367746

Document status and date: Published: 01/01/2010

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Gold-free GaAs/GaAsSb heterostructure nanowires grown on silicon

S. Plissard, K. A. Dick, X. Wallart, and P. Caroff

Citation: Appl. Phys. Lett. 96, 121901 (2010); doi: 10.1063/1.3367746 View online: http://dx.doi.org/10.1063/1.3367746

View Table of Contents: http://apl.aip.org/resource/1/APPLAB/v96/i12

Published by the American Institute of Physics.

Additional information on Appl. Phys. Lett.

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Gold-free GaAs/GaAsSb heterostructure nanowires grown on silicon

S. Plissard,1,a兲 K. A. Dick,2,3X. Wallart,1and P. Caroff1

1Institut d’Electronique, de Microélectronique et de Nanotechnologie, UMR CNRS 8520, Avenue Poincaré,

B.P. 60069, 59652 Villeneuve d’Ascq, France

2Solid State Physics, Lund University, Box 118, S-22100 Lund, Sweden

3Polymer and Materials Chemistry, Lund University, Box 124, S-22100 Lund, Sweden

共Received 9 February 2010; accepted 27 February 2010; published online 22 March 2010兲 Growth of GaAs/GaAsSb heterostructure nanowires on silicon without the need for gold seed particles is presented. A high vertical yield of GaAs nanowires is first obtained, and then GaAsxSb1-x

segments are successfully grown axially in these nanowires. GaAsSb can also be integrated as a shell around the GaAs core. Finally, two GaAsSb segments are grown inside a GaAs nanowire and passivated using an AlxGa1-xAs shell. It is found that no stacking faults or twin planes occur in the GaAsSb segments. © 2010 American Institute of Physics.关doi:10.1063/1.3367746兴

Lattice-mismatched III-V semiconductor heterostruc-tures are important for optoelectronic, nanoelectronic, and energy applications. Their integration on the advantageous Si platform is still facing major challenges, because of large lattice mismatches, polar/nonpolar growth, and differences in thermal expansion coefficients. Nanowires共NWs兲 have been considered as good candidates to overcome some of these issues and to facilitate the growth of III-V heterostructures at the nanoscale on silicon, thanks to the efficient strain relax-ation at their free borders.1 However, gold, the most used seed particle for NW growth, is known to create detrimental midgap defects in silicon and should therefore be avoided in Si-compatible technological processes. Recently, the Fukui group2 and Paek et al.3 reported direct growth on silicon, respectively, of InAs catalyst-free NWs arrays by metal-organic vapor-phase epitaxy 共MOVPE兲, and self-catalyzed GaAs NWs by molecular beam epitaxy共MBE兲, thus opening a viable route for silicon integration of III-V devices.4One of the most interesting materials for telecommunication or en-ergy applications is GaAsxSb1-x, as its wavelength can be

tuned between 0.9 and 1.8 ␮m, and it allows type II band alignments with standard arsenide semiconductors.5 This possibility to extend band gap engineering to type II band alignments, which is interesting for separation of holes and electrons,6 could find applications in future solar cell de-signs. Gold-free growth of Sb-containing heterostructures has never been reported up to now by use of standard epitaxy systems.

In this paper, we present a study of axial and core-shell gold-free GaAs/GaAsSb NW heterostructures grown on na-tive oxide-covered Si共111兲 substrates by gas source molecu-lar beam epitaxy. Arsenic共As2兲 is obtained by thermal

crack-ing of arsine gas共AsH3兲, a standard effusion cell is used for

gallium and a valved-cracker cell is used for antimony共Sb2兲.

Growth rate and V/III ratios are calibrated using reflection high energy electron diffraction specular intensity oscilla-tions. Lightly n-doped Siltronix Si共111兲 substrates were loaded without any treatment in the MBE reactor, and the native oxide thickness was evaluated to be 10⫾1 Å by angle-resolved x-ray photoemission spectroscopy共XPS兲. The

growth temperature was set at 630 or 650 ° C for all samples, using a As/Ga ratio of 1.5 共As pressure: 5.10−6 torr兲, at a two-dimensional 共2D兲 equivalent GaAs growth rate of 1 ML/s. The morphology was studied by a Zeiss Supra scan-ning electron microscope 共SEM兲 at 10 kV. Crystal structure characterization was performed using a JEOL-3000F field emission transmission electron microscope 共TEM兲 operated at 300 kV in conventional TEM共CTEM兲 mode and in high-angle annular dark field 共HAADF兲-scanning TEM 共STEM兲 mode. TEM images were recorded along the具1¯10典 zone axis 共cubic notation兲 and compositions were determined using x-ray energy dispersive spectroscopy 共EDS兲 operated in HAADF-STEM mode. The distribution of the present ele-ments was studied by linescans and point composition spec-tra. The EDS linescans illustrate the heterostructure material changes qualitatively, whereas quantitative point scan analy-sis is used to extract precise compositions. In the following, all compositions are mean ones, and are given in atomic percents 共at. %兲. All presented TEM and EDS data was as-sessed to be representative of the whole NW samples by analyzing five to ten different NWs for each growth condi-tion.

Figure1共a兲shows a SEM image共at 30° tilt angle兲 of the typical GaAs NWs used in this study as a base/stem for the Sb-containing heterostructure NWs. The diameter of these hexagonally shaped NWs was typically in the range of 60– 100 nm, and their length was found to be about 1 ␮m long for a growth time of 5 min. Most NWs grow in the 具111典 direction perpendicular to the substrate, without measurable tapering. Some “bulk” material共i.e., GaAs crystallites form-ing a discontinuous layer兲 is present between the NWs, and

a兲Author to whom correspondence should be addressed. Electronic mail: sebastien.plissard@free.fr.

(a) (b) (c)

200 nm

400 nm 200 nm

FIG. 1. SEM views at 30° tilt angle of gold-free NWs grown on silicon.共a兲 GaAs NWs used as a base/stem of this study.共b兲 Core-shell GaAs/GaAsSb heterostructure.共c兲 Axial GaAsSb segment inserted in a GaAs NW.

APPLIED PHYSICS LETTERS 96, 121901共2010兲

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visible in Fig. 1共a兲. The composition of the nanoparticles measured by EDS is above 99.5 at. % gallium. It shows, in agreement with similar studies by other groups,3,7 that the liquid gallium droplet is, in our case, the seed particle re-sponsible for the enhancement of axial growth rate in the 具111典 direction leading to NW growth, in contrast to selective-area mechanisms reported by the Fukui group in the case of MOVPE grown NW arrays.8

Having established controlled parameters for gold-free GaAs NW growth on silicon, it is now possible to grow more advanced structures, like core-shell关Fig.1共b兲兴 or axial 关Fig.

1共c兲兴 heterostructures. In the first case, the growth of the NW is interrupted after the GaAs core, and by maintaining the arsenic flux on for 2 min with a closed Ga shutter, the gal-lium droplet is transformed into GaAs NW material, termi-nating axial NW growth.9Then, a GaAsSb shell is created by opening simultaneously the Ga and Sb sources at the same temperature. Cross-sectional EDS analysis on these samples 共not shown兲 indicates a GaAsSb shell, which seems fairly uniform although some samples present heterogeneous shell facets 关Fig. 1共b兲兴. EDS point analysis suggests the shell thickness to be around 5 nm, with Sb content around 11 at. %.

In the second case 关Fig. 1共c兲兴, a GaAsSb segment is grown axially during the GaAs NW growth by using a very high nominal antimony flux共equivalent to 3.5 ML/s兲 to par-tially overcome the re-evaporation rate for this element, at the high growth temperature used. Two samples were grown, one at 630 ° C 共shown in Fig.2兲, and one at 650 °C 共only

described in the text兲, in order to tune the antimony compo-sition of the GaAsSb segment. Low magnification HAADF-STEM image of this segment is shown in Figs.2共a兲and2共b兲

illustrates an EDS linescan profile along the length of the NW. A GaAsSb segment, 270 nm in length, is easily recog-nized when following the antimony signal in Fig. 2共b兲. Quantitative EDS point analysis of wires from this sample indicates a Sb content of 15 at. %. Low antimony traces 共around 2 at. %兲 are also detected in the GaAs segment be-low the GaAsSb one, which suggests that a very thin GaAsSb shell forms in parallel to the dominant axial GaAsSb segment growth. A complementary growth of the same structure at 650 ° C confirms the temperature

sensitiv-ity of the Sb incorporation with a measured Sb composition in the segment around 12 at. %. The reduced average Sb content may be related to the higher competing evaporation of Sb at the higher temperature.

Having achieved single heterostructures, the following stage was to develop more complex structures. For that pur-pose, two GaAsSb segments were grown inside GaAs NWs, and then an AlGaAs shell was grown all-around. Growth time for these materials were 4 min 共GaAs兲, 1 min 共GaAsSb兲, 30 s 共GaAs兲, 1 min 共GaAsSb兲, and 2 min 共GaAs兲. Finally a 1 min AlGaAs shell was grown to passivate the whole structure against nonradiative recombination pro-cesses induced at the GaAs surface.3

Figures3共a兲and3共b兲show the SEM and TEM images of these NWs, along with a three-dimensional simple schematic of the nominal structure. Very interestingly, strain fields are visible in the TEM image only in the regions of the GaAsSb segments, allowing easy identification of these segments at low resolution. The appearance of strain fields can be ex-plained by the following: an AlGaAs shell is approximately lattice-matched to GaAs for any aluminum content. How-ever, if GaAsSb is elastically relaxed共one of the key advan-tages of NWs兲,10 then only the GaAsSb/AlGaAs interfaces will be strained because of the AlGaAs shell covering the whole NW. A cross-sectional EDS linescan over a GaAsSb segment in one of these NWs is shown in Fig. 3共c兲. A ⬃85 nm GaAsSb core can be observed with a ⬃25 nm Al-GaAs shell all-around. Quantitative EDS point analysis indi-0 5 10 15 20 25 30 35 40 45 50 0 100 200 300 400

In

tensity

(arb.un.

)

Length (nm)

Sb As

(a)

(b)

100 nm

FIG. 2. 共Color online兲 Characterization of an axial GaAsSb segment in a GaAs NW grown at 630 ° C.共a兲 HAADF STEM measurement of a GaAs wire with a⬃270 nm long segment. 共b兲 EDS linescan measurement of the wire in共a兲, qualitatively illustrating the Sb and As composition.

0 5 10 15 20 25 30 35 40 0 50 100 150 100 nm GaAs GaAsSb GaAsSb GaAs GaAs GaAs AlGaAs 50 nm (a) GaAsSb Al Sb Ga As Length (nm) Intensity (arb.un.) (c) (b)

FIG. 3. 共Color online兲 共a兲 SEM and 共b兲 TEM images of GaAs NWs con-taining with 2 GaAsSb axial segments, and coated by an AlGaAs shell. The TEM image is taken along the具1¯10典 zone axis. A schematic of the structure is also given.共c兲 Cross-sectional EDS measurement across a segment in a NW, showing the GaAsxSb1-xcore and the AlxGa1-xAs shell.

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cated Sb composition in the segments around 17 at. % 共similar to the single axial heterostructure兲, and Al composi-tion around 27 at. %. The antimony composicomposi-tions of the two segments are very similar and the aluminum composition of the shell is in good agreement with the 2D layer growth calibrations. As previously discussed for the single hetero-structure sample, antimony traces are measured in the first two GaAs sections, while the top on the NW does not exhibit detectable antimony.

Finally, the crystal structure of these NWs was studied by high resolution TEM共HRTEM兲. The first GaAs segment typically exhibits stacking faults and wurtzite phase, as is often observed in gold-nucleated GaAs NWs.11On the con-trary, the GaAsSb segments exhibit perfect twin-free zinc blende phase. Figure4 shows an HRTEM image of the two GaAsSb segments separated by GaAs. The crystal phase is also characterized in the fast Fourier transform共FFT兲 images added as insets. The control of phase purity in III-V NWs is a very active research area, as most of these naturally show polytypism.12 We note that our results are in perfect agree-ment with previously studied gold-seeded GaSb or GaAsSb NWs,13–15 although the growth mechanism, growth condi-tions, and substrate used are completely different. In view of these studies and of the present work, it is clear that this effect should be linked to the presence of antimony, indepen-dent of the nature of the seed particle droplet, and could be linked to its well known surfactant properties.16Another in-teresting point is shown in Fig.4, which shows the transition zone from the first 共bottom兲 GaAsSb segment 共right兲 to GaAs middle segment and second 共top兲 GaAsSb segment. Both GaAsSb segments are perfect zinc blende but the

middle GaAs segment has a wurtzite crystal structure. The transition from GaAsSb to GaAs on the right hand side shows some stacking faults, whereas the transition from GaAs to GaAsSb on the left hand side is abrupt. This could be due to Sb traces remaining in the particle after the switch-ing sequence to GaAs is done.

In summary, we have reported successful growth of gold-free axial and lateral GaAs/GaAsSb heterostructure NWs on silicon. Single GaAs/GaAsSb heterostructures were first shown. A 5 nm thick GaAs0.78Sb0.22shell around a GaAs core and a⬃270 nm GaAs0.70Sb0.30axial segment were then

separately engineered. Finally, a complex structure com-posed of two axial GaAs0.76Sb0.34segments in a GaAs NW,

passivated with an Al0.54Ga0.46As shell, was detailed. The GaAsSb segments exhibit a perfect zinc blende structure, linked to the presence of antimony, while the GaAs contains significant wurtzite structure under the investigated growth conditions. The possibility to grow strained passivating Al-GaAs shells is very promising for future microphotolumines-cence studies of strained type II band-alignments in Sb-containing III-V NW heterostructures.

The authors would like to acknowledge A. Addad, S. Godey, C. Coinon, and J.-L. Codron, respectively, for TEM characterizations, XPS analysis, and help with MBE work. Part of this work was funded by the Swedish Foundation for Strategic Research 共SSF兲, the Swedish Research Council 共VR兲, and the Knut and Alice Wallenberg Foundation.

1K. L. Kavanagh,Semicond. Sci. Technol. 25, 024006共2010兲.

2K. Tomioka, J. Motohisa, S. Hara, and T. Fukui, Nano Lett. 8, 3475 共2008兲.

3J. H. Paek, T. Nishiwaki, M. Yamaguchi, and N. Sawaki, Phys. Status

Solidi C 6, 1436共2009兲.

4W. Wei, X. Bao, C. Soci, Y. Ding, Z. Wang, and D. Wang,Nano Lett. 9, 2926共2009兲.

5D. L. Dheeraj, G. Patriarche, H. Zhou, T. B. Hoang, A. F. Moses, S. Grønsberg, A. T. J. van Helvoort, B. O. Fimland, and H. Weman,Nano Lett. 8, 4459共2008兲.

6M. E. Pistol and C. Pryor,Phys. Rev. B 80, 035316共2009兲.

7C. Colombo, D. Spirkoska, M. Frimmer, G. Abstreiter, and A. Fontcuberta i Morral,Phys. Rev. B 77, 155326共2008兲.

8K. Ikejiri, J. Noborisaka, S. Hara, J. Motohisa, and T. Fukui, J. Cryst.

Growth 298, 616共2007兲.

9A. Fontcuberta i Morral, D. Spiroska, J. Arbiol, M. Heigoldt, J. R. Morante, and G. Abstreiter,Small 4, 899共2008兲.

10F. Glas,Phys. Rev. B 74, 121302共2006兲.

11F. Glas, J.-C. Harmand, and G. Patriarche, Phys. Rev. Lett. 99, 146101 共2007兲.

12K. A. Dick, P. Caroff, J. Bolinsson, M. E. Messing, J. Johansson, K. Deppert, L. R. Wallenberg, and L. Samuelson,Semicond. Sci. Technol.

25, 024009共2010兲.

13Y. N. Guo, J. Zou, M. Paladugu, and H. Wang, Appl. Phys. Lett. 89, 231917共2006兲.

14M. Jeppsson, K. A. Dick, J. B. Wagner, P. Caroff, K. Deppert, L. Samuel-son, and L.-E. WernersSamuel-son,J. Cryst. Growth 310, 4115共2008兲.

15D. L. Dheeraj, G. Patriarche, L. Largeau, H. L. Zhou, A. T. J. van Helvoort, F. Glas, J. C. Harmand, B. O. Fimland, and H. Weman,

Nanotechnology 19, 275605共2008兲.

16P. Nimmatoori, Q. Zhang, E. C. Dickey, and J. M. Redwing,

Nanotech-nology 20, 025607共2009兲. 50 nm ZB WZ ZB GaAsSb GaAsSb GaAs Growth Direction [111] _ _ [111] _ _ _ [002] _ [0002] _ [1101] _ _

FIG. 4. HRTEM image of the axial GaAsSb/GaAs/GaAsSb heterostructure shown in Fig.3, taken in the具1¯10典 zone axis. Inset FFTs are given for each material, indicating the cubic 共zinc blende兲 structure of the GaAsSb and hexagonal共wurtzite兲 structure of the GaAs in the center. Stacking faults are visible at the GaAsSb-GaAs interface but the switch back to GaAsSb is abrupt.

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