# Interaction and Cooperative Nucleation of InAsSbP Quantum Dots and Pits on InAs(100) Substrate

- Karen M Gambaryan
^{1}Email author

**Received: **19 November 2009

**Accepted: **9 December 2009

**Published: **24 December 2009

## Abstract

An example of InAsSbP quaternary quantum dots (QDs), pits and dots–pits cooperative structures’ growth on InAs(100) substrates by liquid phase epitaxy (LPE) is reported. The interaction and surface morphology of the dots–pits combinations are investigated by the high-resolution scanning electron microscope. Bimodal growth mechanism for the both QDs and pits nucleation is observed. Cooperative structures consist of the QDs banded by pits, as well as the “large” pits banded by the quantum wires are detected. The composition of the islands and the pits edges is found to be quaternary, enriched by antimony and phosphorus, respectively. This repartition is caused by dissociation of the wetting layer, followed by migration (surface diffusion) of the Sb and P atoms in opposite directions. The “small” QDs average density ranges from 0.8 to 2 × 10^{9} cm^{−2}, with heights and widths dimensions from 2 to 20 nm and 5 to 45 nm, respectively. The average density of the “small” pits is equal to (6–10) × 10^{9} cm^{−2} with dimensions of 5–40 nm in width and depth. Lifshits–Slezov-like distribution for the amount and surface density of both “small” QDs and pits versus their average diameter is experimentally detected. A displacement of the absorption edge toward the long wavelength region and enlargement toward the short wavelength region is detected by the Fourier transform infrared spectrometry.

### Keywords

Quantum dots Pits Liquid phase epitaxy Strain-induced III–V compound semiconductors## Introduction

In the last two decades, a large research effort has been devoted to quantum dots (QDs), the quantum wires, QD chains, nanoholes and pits [1–8] due to their modified density of states, fascinating optoelectronic properties and device applications for lasers, photodetectors and other electronic devices. Among quantum dots, pits and wires fabrication techniques, the self-organized Stranski–Krastanow method [9] is an important one by which dislocation-free dots, elongated islands and wires can be produced. Indeed, above a certain critical thickness, the growth mode switches from the conventional layer-by-layer (i.e., two-dimensional, 2D) to a 3D growth mode due to the accumulation of the elastic energy in the strained layer that, first, partially relaxes by spontaneously nucleating small islands of strained material and, later, by creating misfit dislocations. The elastic strain caused by lattice mismatch can also be relaxed by the formation of undulations, pits and their combination [5–8]. Depending on the growth conditions, the elastic strain can be relaxed by the formation of either quantum wires and quantum dots, or even unique island–pit pairs. Extensive experimental results suggest that surface morphologies are relying on growth conditions and matrix materials. On the basis of an atomistic model, it is shown that the energy change due to the step formation is negative or positive depending upon the sign of the misfit. The step formation energy can even be negative for compressive misfit stress in the heterolayer, while it is definitely positive for tensile misfit stress. This conclusion is in contrast to the classical model where the step energy is always positive and independent of the sign of the misfit. The step formation energy influences the critical thickness and the energy barrier for dislocation nucleation.

Using a simple atomistic simulation, it is shown that the critical thickness depends upon the sign of the misfit. For example, it changes from 4 nm for Ge films on Si(100) substrates to 6 nm for Si films on Ge(100) substrates having the same misfit [5]. The investigations of the surface morphology evolution of strained InAs/GaAs films at different growth conditions [6] demonstrated that there are at least three different strain relaxation mechanisms for the same material system. That is, depending on the growth conditions, the elastic strain can be relaxed by the formation of either quantum wires or quantum dots, or even unique island–pit pairs. The islands and pits first grow simultaneously as the layer deposition proceeds. Both the island height and the pit depth can be much greater than the average layer thickness. This suggests that considerable mass transport from substrate into the islands is taking place during the growth [7]. However, during heteroepitaxy, when the layer becomes sufficiently thick, the pits are eventually filled up either by the lateral overgrowth or by the expanding islands, forming nearly pure island morphology at the surface. The detailed analysis of the surface dynamics during phase transitions of GaAs(100) [10] and unusual role of the substrate at droplet-induced GaAs/AlGaAs QD pairs growth [11] also confirm this assumption.

From the industrial point of view, the narrow band gap III–V semiconductor materials like InAs, GaSb, InSb and their ternary and quaternary alloys are particularly interesting and useful since they are potentially promising to access mid-infrared and far infrared wavelength regions. These materials would provide the next generation of LEDs, lasers and photodiodes for applications such as infrared gas sensors, for molecular spectroscopy, thermal imaging, photovoltaic (PV) [12] and thermo-photovoltaic cells (TPV) [13]. The application of the InAsSbP and other similar quaternary materials opens up interesting physical and technological prospects for the dirigible growth of QDs, the pits and dots–pits cooperative systems. Independent variations of the third and fourth components provide corresponding sign of the misfit; i.e., providing the tensile or compressive misfit stress. At the first case, elastic strain will be relaxed by the formation of QDs, but at the second one—by the pits.

In this article, an example of InAsSbP quaternary QDs, the pits and dots–pits cooperative structure growth on InAs(100) substrates by LPE, as well as the interaction and surface morphology of the dots–pits combinations are presented and investigated.

## Experimental Results and Discussion

The samples are grown by LPE using a slide-boat crucible. To ensure a high purity of the epitaxial layers, the entire growth process is performed under the pure hydrogen atmosphere. The InAs(100) substrates have a 11 mm diameter are undoped, with a background electron concentration of *n* = 2 × 10^{16} cm^{−3}. The InAs_{0,742} Sb_{0,08} P_{0,178} quaternary alloy used here as basis composite is conveniently lattice-matched to InAs. The LPE growth solution components—undoped InAs, undoped InP and Sb (6 N) are solved in a In (7 N) solution that has been first homogenized for 1 h at *T* = 580 °C and then 3 h at the initial growth temperature of *T* = 550 °C to equilibrate the system thermodynamically. To expect the strain-induced QDs and pits formation, the undoped and supersaturated by antimony and phosphorus liquid phase was used to provide a different sign of lattice mismatch up to 4% between the InAs substrate and InAsSbP epilayer. To initiate the growth of QDs and pits, an oversaturation of the liquid phase is developed by decreasing the initial growth temperature up to 2 °C at the slower ramp rate.

_{0.53}Ga

_{0.47}As layers on InP(001) substrate [14, 15]. The effect of island density on pit nucleation in In

_{0.27}Ga

_{0.73}As films grown on GaAs(001) substrate is discussed in [16].

In order to be confident, we calculated the Gibbs free energy of InAsSbP quaternary alloy, as well as separately of InAs-InSb, InAs-InP and InSb-InP ternary alloys. We found that at *T* = 550 °C (our growth temperature), the Gibbs energy has the minimal value at *x* = 0.39 for InAs_{1−x}Sb_{x} and at *y* = 0.52 for InAs_{1−y}P_{y} alloys. Therefore, there is a trend for these binary pairs to mix. Otherwise, for the InSb_{1−z}P_{z} ternary alloy at the same temperature, the sufficiently wide immiscibility gap is exist at 0.05 < z < 0.97. In this concentration range, the Gibbs energy increases (from the both sides) and the mixing of these binary compounds becomes energetically not preferable. This result marginally proves our assumption that at the nucleation of InAsSbP quaternary dots and pits, the surface diffusion of the antimony and phosphorus in opposite direction has to be energetically more preferable. In addition, note that with the increasing of the liquid phase initial concentration, the islands and pits shape transformation from the truncated pyramids to ellipsoidal and globe shape was detected.

*S*= 4 µm

^{2}. In this figure, white points correspond to the QDs and black points to pits. The QDs and pits are clearly visible and quite uniformly distributed over the substrate surface. Figures 1b, 1c and 2b–2d show that cooperative nucleation of the dots–pits structures is occurring. In particularly, the “large” pits are banded by quantum wires and that the QDs are banded by pits (in the form of “nano-camomile”).

^{9}cm

^{−2}, with heights and widths dimensions from 2 to 20 nm and 5 to 45 nm, respectively. The average density of the “small” pits is equal to (6–10) × 10

^{9}cm

^{−2}with dimensions of 5–40 nm in width and depth. Surface density of the “large” dots and pits is less by almost on two orders of magnitude. The Lifshits–Slezov-like [17] distribution for both “small” QDs and pit amount, and surface density versus their average diameter calculated from the surface of

*S*= 4 µm

^{2}is detected and displayed in Fig. 3.

_{1−x−y}Sb

_{x}P

_{y}quaternary system was calculated by the linear approximation of the corresponding values for binary compounds at

*x*= 0.04 and

*y*= 0.08.

Finally, note that at the growth of diode heterostructures with the quantum dots and pits inside p–n junction spatial charge region, the main challenge to overcome is providing the lateral overgrowth of the pits (providing “reverse” QDs) and keeping the dots size during epitaxy of the cap epilayer. We assume that by using step-cooling LPE, the growth of the cap epilayer from the strongly cooled liquid phase will address this problem.

## Conclusion

Thus, we have presented an example of the InAsSbP quaternary QDs, pits and dots–pits cooperative structures growth on the InAs(100) substrates by LPE. The interaction and surface morphology of the dots–pits combinations were investigated. Bimodal growth mechanism for the both QDs and pits nucleation was observed. Lifshits–Slezov-like distribution for the amount and surface density of “small” QDs, and pits versus their average diameter was experimentally detected. Application of the InAsSbP and other similar quaternary materials opens up interesting physical and technological prospects for the dirigible growth of QDs, pits and dots–pits cooperative systems. By the corresponding and independent variations of the V-group elements concentrations, the preferred nucleation of the dots or pits can be selected. The results of our study can be also used for producing controlled arrays of strain-induced QDs, which is very important for the fabrication of wide-band photodiodes, thermo-photovoltaic cells and other InAs-based mid-infrared devices.

## Declarations

### Acknowledgments

The author gratefully acknowledges Prof. V. M. Aroutiounian, Prof. P. Soukiassian, Prof. R. Fornari and Dr. T. Boeck for comprehensive support and fruitful discussions and Ms. M. Schulze (present location—“Bosch AG”) for SEM and AFM measurements. This work was carried out in the frame of Armenian National Governmental Program for Nano-Electronics and ISTC Grant A—1232.

**Open Access**

This article is distributed under the terms of the Creative Commons Attribution Noncommercial License which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and source are credited.

## Authors’ Affiliations

## References

- Nishi K, Saito H, Sugou S, Lee JS:
*Appl. Phys. Lett.*. 1999,**74:**1111. COI number [1:CAS:528:DyaK1MXhtF2ht7Y%3D]; Bibcode number [1999ApPhL..74.1111N] COI number [1:CAS:528:DyaK1MXhtF2ht7Y%3D]; Bibcode number [1999ApPhL..74.1111N] 10.1063/1.123459View ArticleGoogle Scholar - Haft D, Warburton RJ, Karrai K, Huant S, Medeiros-Ribeiro G, Garcia JM, Schoenfeld W, Petroff PM:
*Appl. Phys. Lett.*. 2001,**78:**2946. COI number [1:CAS:528:DC%2BD3MXjt1ejtLs%3D]; Bibcode number [2001ApPhL..78.2946H] COI number [1:CAS:528:DC%2BD3MXjt1ejtLs%3D]; Bibcode number [2001ApPhL..78.2946H] 10.1063/1.1356445View ArticleGoogle Scholar - Gambaryan KM, Aroutiounian VM, Boeck T, Schulze M, Soukiassian PG:
*J. Phys. D Appl. Phys.*. 2008,**41:**162004. Bibcode number [2008JPhD...41p2004G] Bibcode number [2008JPhD...41p2004G] 10.1088/0022-3727/41/16/162004View ArticleGoogle Scholar - Wang ZM, Holmes K, Mazur YI, Salamo GJ:
*Appl. Phys. Lett.*. 2004,**84:**1931. COI number [1:CAS:528:DC%2BD2cXitFSnsb8%3D]; Bibcode number [2004ApPhL..84.1931W] COI number [1:CAS:528:DC%2BD2cXitFSnsb8%3D]; Bibcode number [2004ApPhL..84.1931W] 10.1063/1.1669064View ArticleGoogle Scholar - Ichimura M, Narayan J:
*Mater. Sci. Eng.*. 1995,**B31:**299. COI number [1:CAS:528:DyaK2MXls12gt7o%3D] COI number [1:CAS:528:DyaK2MXls12gt7o%3D] 10.1016/0921-5107(94)01146-XView ArticleGoogle Scholar - Gong Z, Fang Z, Miao Z, Niu Z:
*Int. J. Nanasci*. 2006,**5:**883. COI number [1:CAS:528:DC%2BD2sXitlGhsLg%3D] COI number [1:CAS:528:DC%2BD2sXitlGhsLg%3D] 10.1142/S0219581X06005315View ArticleGoogle Scholar - Li JH, Moss SC, Han BS, Mai ZH:
*J. Appl. Phys.*. 2001,**89:**3700. COI number [1:CAS:528:DC%2BD3MXitFKmt7g%3D]; Bibcode number [2001JAP....89.3700L] COI number [1:CAS:528:DC%2BD3MXitFKmt7g%3D]; Bibcode number [2001JAP....89.3700L] 10.1063/1.1354637View ArticleGoogle Scholar - Wang ZM, Liang BL, Sablon KA, Salamo GJ:
*Appl. Phys. Lett.*. 2007,**90:**113120. Bibcode number [2007ApPhL..90k3120W] Bibcode number [2007ApPhL..90k3120W] 10.1063/1.2713745View ArticleGoogle Scholar - Stranski I, Krastanow L:
*Math.-Naturwissenshaft*. 1938,**146:**797. COI number [1:CAS:528:DyaA1cXlvVyksg%3D%3D] COI number [1:CAS:528:DyaA1cXlvVyksg%3D%3D]Google Scholar - Wang ZM, Salamo GJ:
*Phys. Rev. B*. 2003,**67:**125324. Bibcode number [2003PhRvB..67l5324W] Bibcode number [2003PhRvB..67l5324W] 10.1103/PhysRevB.67.125324View ArticleGoogle Scholar - Wang ZM, Mazur YI, Sablon KA, Mishima TD, Johnson MB, Salamo GJ:
*Physica Status Solidi (RRL)*. 2008,**2:**281. COI number [1:CAS:528:DC%2BD1MXhsVWqsg%3D%3D]; Bibcode number [2008PSSRR...2..281W] COI number [1:CAS:528:DC%2BD1MXhsVWqsg%3D%3D]; Bibcode number [2008PSSRR...2..281W] 10.1002/pssr.200802196View ArticleGoogle Scholar - Aroutiounian VM, Petrosian SG, Khachatryan A, Touryan K:
*J. Appl. Phys.*. 2001,**89:**2268. COI number [1:CAS:528:DC%2BD3MXotlyhsw%3D%3D]; Bibcode number [2001JAP....89.2268A] COI number [1:CAS:528:DC%2BD3MXotlyhsw%3D%3D]; Bibcode number [2001JAP....89.2268A] 10.1063/1.1339210View ArticleGoogle Scholar - Gevorkyan VA, Aroutiounian VM, Gambaryan KM, Arakelyan AH, Andreev IA, Golubev LV, Yakovlev YuP:
*Solid State Electron.*. 2007,**52:**339. COI number [1:CAS:528:DC%2BD2sXjtFKntLs%3D] COI number [1:CAS:528:DC%2BD2sXjtFKntLs%3D]Google Scholar - Lee AJY, Pearson C, Millunchick JM:
*J. Appl. Phys.*. 2008,**103:**104309. Bibcode number [2008JAP...103j4309L] Bibcode number [2008JAP...103j4309L] 10.1063/1.2917276View ArticleGoogle Scholar - Riposan A, Pearson C, Millunchick JM:
*Appl. Phys. Lett.*. 2007,**90:**091902. Bibcode number [2007ApPhL..90i1902R] Bibcode number [2007ApPhL..90i1902R] 10.1063/1.2476259View ArticleGoogle Scholar - Riposan A, Martin GKM, Bouville M, Falk ML, Millunchick JM:
*Surf. Sci.*. 2003,**525:**222. COI number [1:CAS:528:DC%2BD3sXpsFCgtQ%3D%3D]; Bibcode number [2003SurSc.525..222R] COI number [1:CAS:528:DC%2BD3sXpsFCgtQ%3D%3D]; Bibcode number [2003SurSc.525..222R] 10.1016/S0039-6028(02)02563-3View ArticleGoogle Scholar - Lifshits IM, Slezov VV:
*J. Phys. Chem. Solids*. 1961,**19:**35. Bibcode number [1961JPCS...19...35L] Bibcode number [1961JPCS...19...35L] 10.1016/0022-3697(61)90054-3View ArticleGoogle Scholar - Li S-S, Xia J-B, Yuan ZL, Xu ZY, Ge W, Wang XR, Wang Y, Wang J, Chang LL:
*Phys. Rev. B*. 1996,**54:**11575. COI number [1:CAS:528:DyaK28Xms1Wnurk%3D]; Bibcode number [1996PhRvB..5411575L] COI number [1:CAS:528:DyaK28Xms1Wnurk%3D]; Bibcode number [1996PhRvB..5411575L] 10.1103/PhysRevB.54.11575View ArticleGoogle Scholar