Epitaxial Catalyst-Free Growth of InN Nanorods onc-Plane Sapphire
© to the authors 2009
Received: 24 December 2008
Accepted: 9 February 2009
Published: 27 February 2009
We report observation of catalyst-free hydride vapor phase epitaxy growth of InN nanorods. Characterization of the nanorods with transmission electron microscopy, and X-ray diffraction show that the nanorods are stoichiometric 2H–InN single crystals growing in the  orientation. The InN rods are uniform, showing very little variation in both diameter and length. Surprisingly, the rods show clear epitaxial relations with thec-plane sapphire substrate, despite about 29% of lattice mismatch. Comparing catalyst-free with Ni-catalyzed growth, the only difference observed is in the density of nucleation sites, suggesting that Ni does not work like the typical vapor–liquid–solid catalyst, but rather functions as a nucleation promoter by catalyzing the decomposition of ammonia. No conclusive photoluminescence was observed from single nanorods, while integrating over a large area showed weak wide emissions centered at 0.78 and at 1.9 eV.
InN marks the lower bandgap limit achievable within the group III-nitride semiconductor family. To date, it has also been the most difficult-to-grow among that family, mainly because at its growth temperature, InN decomposes almost as readily as ammonia. Incorporation of In into GaN has also been difficult, especially at high In percentage, due to the large difference in growth temperature between InN and GaN . An even more challenging scenario is encountered when one attempts a catalytic growth of InN nanowires. Catalytic growth is commonly preferred, for it allows control of size and position of the wires. A catalyst of choice is one that is inert and can liquefy, if not as a pure element, at least by eutectic reaction with another element, below the growth temperature. The most common choice is Au. Au can melt eutectically in reaction with Si but not as well on sapphire, the more common substrate for nitrides. Furthermore, nitrogen is claimed to be poorly soluble in Au . Growth with Au catalyst has been reported , but due to its relatively low efficiency, it typically requires large flow of ammonia. In many studies, catalyzed nitride nanowires are grown with Ni [4, 5]. In this paper, we report an observation of catalyst-free epitaxial growth of remarkably size-uniform and vertically-aligned InN nanorods on c-plane sapphire. We compare this growth to Ni catalyzed growth under the same conditions and suggest that a growth mechanism other than vapor–liquid–solid (VLS) may be responsible for the observed uniformity.
Process gasses were exhausted through a Lab Guard wet scrubbing system. The growth was carried out at atmospheric pressure. Ultra high purity Ar was used as a carrier gas. Typical carrier flow was 3000 sccm, HCl and NH3 flows were 1–10 and 50–200 sccm, respectively. The efficiency of ammonia decomposition drops with temperature, and is rather low at the InN growth temperatures. For this reason, the growth of InN requires a relatively high flow of ammonia . The growth was estimated to be at a rate of ∼45 nm/min and was carried out for 30 min.
Scanning electron microscopy was carried out in a LEO (Zeiss) 982 FEG-SEM Field Emission Gun Scanning Electron Microscope with a Noran thin-window electron-dispersive spectroscopy (EDS) detector. Tunneling electron microscopy (TEM) was performed using a JEOL 2010-FEG-TEM/STEM operated at 200 keV with attached EDAX thin-window detector. Photoluminescence (PL) was excited at room temperature using a HeCd laser (325 nm, 8 mW). The emitted luminescence was dispersed by a monochromator, filtered, and sensed using a Si CCD camera.
To assess the material resistivity, we carried out standard four-point probe sheet resistance measurement on continuous layers of fused nanorods grown using Ni catalyst. The measured sheet resistance of 55.5 Ohm/square, multiplied by the film thickness of 1.8 mm, yields 0.01 Ohm cm.
Weak radiative recombination is not uncommon in narrow gap III–V semiconductors, especially when nanostructured. Possibly, the increased surface-to-volume ratio gives rise to enhanced effect of surface recombination. Since surface states are typically below the bandgap energy, and since our InGaAs detector was limited to 0.6 eV, our experiment was practically blind to any emission below 0.6 eV. Surface deep levels usually mean surface depletion. However, narrow gap III–V semiconductors, especially In-based, such as InAs and InSb, are known to have their surface Fermi level pinned above the conduction band, giving rise to surface accumulation layer . The high density of accumulated electrons at the surface is a known cause for non-radiative recombination through Auger processes. Auger recombination has been shown to be the main non-radiative recombination mechanism in InGaAs semiconductor devices, having band gap energy in the range of 0.6–0.8 eV . While the effectiveness of Auger processes in InN is still under debate [12, 13], it is known to strongly depend on the doping. The resistivity of our material (0.01 Ohm cm) seems low enough to make this mechanism important.
While PL does not provide a conclusive identification of InN, both in general and specifically in our experiment, our X-ray and TEM/selective area diffraction data present a clear picture ofc-oriented material growth, with EDS clearly identifying the main elements as indium and nitrogen. The lack of Ni signal in EDS spectra does not exclude Ni incorporation within the InN rods, but conclusively confirms its absence at the rod tip, at the typical VLS catalyst placement, commonly observed in VLS growth.
Ni does not melt (not even by eutectic reaction with sapphire or aluminum) at the growth temperature range . Therefore, it is quite clear that if the growth still takes place by vapor–liquid–solid mode, the only available liquid metal in the system is that of the group III metal, i.e., the growth is most likely self-catalyzed by the group III metal . Nonetheless, we observe a clear increase in nucleation density in c-plane sapphire samples deposited with Ni compared with bare samples grown simultaneously at the same run (comparing the top and bottom panels of Fig. 2). We therefore suggest that Ni serves as a nucleation promoter possibly by virtue of its ability to catalyze ammonia decomposition [16–20]. This type of catalysis is less likely to yield diameter control, as does the common VLS-mode catalyst, but may easily explain the order of magnitude denser nucleation of rods we observe in the presence of Ni. Further structural studies, e.g., cross-sectional TEM of the nucleation phase of the growth, could shed more light on the details of the Ni role.
Self-VLS-catalysis, e.g., with In, as is possible in our case, is also unlikely to provide any control, as the metal vapor is being showered all over the sample continuously through the growth, unlike the case of VLS, where the size and placement of catalyst droplets is well-defined at the beginning of the growth and is relatively stable through the growth. Hence the outstanding diameter uniformity that we observe cannot be explained by the VLS model and does not seem to be related to the Ni catalyst either.
Another form of outstanding uniformity is the rotational alignment of the rods. Such alignment would only be possible under epitaxial relations. However, this is rather surprising considering a lattice mismatch of 29% between InN and sapphire, known to produce structural defects (misfit dislocations) in films. Typically in such cases, the wire structure shows a wider cone shaped base, where the strain is gradually relieved [21, 22]. No such effect, or any other effect of strain has been observed in our case. In a theoretical work, Ertekin et al. showed that nanowire heterostructures are more effective at relieving mismatch strain coherently compared with films. The critical diameter for coherent growth of nanowires on lattice-mismatched substrates was predicted to be up to one order of magnitude larger than that of thin film growth . Yet, most of the published works on growth of InN nanorods on c-plane sapphire typically observe random orientations emanating from each nucleus with no clear expitaxial relation to the substrate [24–26].
Epitaxial growth of InN on c-plane sapphire has been explored [27, 28]. However, to date, an intermediate layer of AlN (often formed by nitridation of the sapphire substrate) or a bilayer AlN\GaN have always been used to bridge the mismatch and reduce the defect formation. In our case, we did not perform any intentional pretreatment. Nitridation is highly unlikely to have taken place at 550 °C. Unintentional In2O3 is also unlikely to be able to bridge between InN and sapphire, because In2O3 is of cubic symmetry. Hence, it seems highly likely that the epitaxial relations we observed were direct, although the details of the actual mechanism require further investigation.
Our observation suggests that InN may establish direct epitaxial relation withc-plane sapphire and may also form nanoscale fibers without extrinsic catalyst. Use of Ni as catalyst is only seen to increase the nucleation density and is therefore suggested to work as nucleation promoter by catalyzing ammonia decomposition.
This work was supported by the National Science Foundation through grant # ECS-0322720. I.S. acknowledges a Converging Technologies personal grant from the Israeli Science Foundation - VATAT.
- Bhuiyan AG, Hashimoto A, Yamamoto A: J. Appl. Phys.. 2003, 94: 2779. COI number [1:CAS:528:DC%2BD3sXms1Cjtrw%3D]; Bibcode number [2003JAP....94.2779B] COI number [1:CAS:528:DC%2BD3sXms1Cjtrw%3D]; Bibcode number [2003JAP....94.2779B] 10.1063/1.1595135View ArticleGoogle Scholar
- Okamoto H, Massalski TB: J. Phase Equilib.. 1984, 5: 381.Google Scholar
- Hsu CW, Ganguly A, Liang CH, Hung YT, Wu CT, Hsu GM, Chen YF, Chen CC, Chen KH, Chen LC: Adv. Funct. Mater.. 2008, 18: 938. COI number [1:CAS:528:DC%2BD1cXkslyhs7s%3D] COI number [1:CAS:528:DC%2BD1cXkslyhs7s%3D] 10.1002/adfm.200700739View ArticleGoogle Scholar
- Duan XF, Lieber CM: J. Am. Chem. Soc.. 2000, 122: 188. COI number [1:CAS:528:DyaK1MXnvF2qt7w%3D] COI number [1:CAS:528:DyaK1MXnvF2qt7w%3D] 10.1021/ja993713uView ArticleGoogle Scholar
- Zhang J, Zhang L, Vac J: Sci. Technol. B. 2003, 21: 2415. COI number [1:CAS:528:DC%2BD2cXptFGnsQ%3D%3D] COI number [1:CAS:528:DC%2BD2cXptFGnsQ%3D%3D] 10.1116/1.1625968View ArticleGoogle Scholar
- Cai XM, Yeb F, Jing SY, Zhang DP, Fan P, Xie EQ: Appl. Surf. Sci.. 2008, 255: 2153. COI number [1:CAS:528:DC%2BD1cXhsVChsL7K]; Bibcode number [2008ApSS..255.2153C] COI number [1:CAS:528:DC%2BD1cXhsVChsL7K]; Bibcode number [2008ApSS..255.2153C] 10.1016/j.apsusc.2008.07.051View ArticleGoogle Scholar
- Wagner RS, Ellis WC: Appl. Phys. Lett.. 1964, 4: 89. COI number [1:CAS:528:DyaF2cXls1yhug%3D%3D]; Bibcode number [1964ApPhL...4...89W] COI number [1:CAS:528:DyaF2cXls1yhug%3D%3D]; Bibcode number [1964ApPhL...4...89W] 10.1063/1.1753975View ArticleGoogle Scholar
- Chen HY, Shen CH, Lin HW, Chen CH, Wu CY, Gwo S, Davydov VY, Klochikhin AA: Thin Solid Films. 2006, 515: 961. COI number [1:CAS:528:DC%2BD28XhtFKktbvN]; Bibcode number [2006TSF...515..961C] COI number [1:CAS:528:DC%2BD28XhtFKktbvN]; Bibcode number [2006TSF...515..961C] 10.1016/j.tsf.2006.07.086View ArticleGoogle Scholar
- Butcher KSA, Tansley TL: Superlattice. Microst.. 2005, 38: 1. COI number [1:CAS:528:DC%2BD2MXlsVCksLw%3D]; Bibcode number [2005SuMi...38....1B] COI number [1:CAS:528:DC%2BD2MXlsVCksLw%3D]; Bibcode number [2005SuMi...38....1B] 10.1016/j.spmi.2005.03.004View ArticleGoogle Scholar
- Stoica T, Meijers RJ, Calarco R, Richter T, Sutter E, Lueth H: Nano Lett.. 2006, 6: 1541. COI number [1:CAS:528:DC%2BD28XmtF2qsLs%3D] COI number [1:CAS:528:DC%2BD28XmtF2qsLs%3D] 10.1021/nl060547xView ArticleGoogle Scholar
- Metzger WK, Wanlass MW, Ellingson RJ, Ahrenkiel RK, Carapella JJ: Appl. Phys. Lett.. 2001, 79: 3272. COI number [1:CAS:528:DC%2BD3MXot1Slsbs%3D]; Bibcode number [2001ApPhL..79.3272M] COI number [1:CAS:528:DC%2BD3MXot1Slsbs%3D]; Bibcode number [2001ApPhL..79.3272M] 10.1063/1.1418032View ArticleGoogle Scholar
- Ascazubi R, Wilke I, Cho S, Lu H, Schaff WJ: Appl. Phys. Lett.. 2006, 88: 112111. Bibcode number [2006ApPhL..88k2111A] Bibcode number [2006ApPhL..88k2111A] 10.1063/1.2185407View ArticleGoogle Scholar
- Tsai T-R, Chang C-F, Gwo S: Appl. Phys. Lett.. 2007, 90: 252111. Bibcode number [2007ApPhL..90y2111T] Bibcode number [2007ApPhL..90y2111T] 10.1063/1.2751110View ArticleGoogle Scholar
- Massalski TB: Binary Alloy Phase Diagrams. ASM International, Bilthoven; 1990.Google Scholar
- Simpkins BS, Ericson LM, Stroud RM, Pettigrew KA, Pehrsson PE: J. Cryst. Growth. 2006, 290: 115. COI number [1:CAS:528:DC%2BD28XisFyju78%3D]; Bibcode number [2006JCrGr.290..115S] COI number [1:CAS:528:DC%2BD28XisFyju78%3D]; Bibcode number [2006JCrGr.290..115S] 10.1016/j.jcrysgro.2005.12.095View ArticleGoogle Scholar
- Grunze M, Golze M, Driscoll RK, Dowben PA: J. Vac. Sci. Technol.. 1981, 18: 611. COI number [1:CAS:528:DyaL3MXksV2qs7k%3D]; Bibcode number [1981JVST...18..611G] COI number [1:CAS:528:DyaL3MXksV2qs7k%3D]; Bibcode number [1981JVST...18..611G] 10.1116/1.570833View ArticleGoogle Scholar
- Grunze M, Dowben PA, Brundle CR: Surf. Sci.. 1983, 128: 311. COI number [1:CAS:528:DyaL3sXksF2ms74%3D]; Bibcode number [1983SurSc.128..311G] COI number [1:CAS:528:DyaL3sXksF2ms74%3D]; Bibcode number [1983SurSc.128..311G] 10.1016/S0039-6028(83)80034-XView ArticleGoogle Scholar
- Bassignana IC, Wagemann K, Kueppers J, Ertl G: Surf. Sci.. 1986, 175: 22. COI number [1:CAS:528:DyaL28XlsF2gsLg%3D]; Bibcode number [1986SurSc.175...22B] COI number [1:CAS:528:DyaL28XlsF2gsLg%3D]; Bibcode number [1986SurSc.175...22B] 10.1016/0039-6028(86)90081-6View ArticleGoogle Scholar
- Chrysostomou D, Flowers J, Zaera F: Surf Sci. 1999, 439: 34. COI number [1:CAS:528:DyaK1MXmslCgsLs%3D]; Bibcode number [1999SurSc.439...34C] COI number [1:CAS:528:DyaK1MXmslCgsLs%3D]; Bibcode number [1999SurSc.439...34C] 10.1016/S0039-6028(99)00458-6View ArticleGoogle Scholar
- Yina SF, Xub BQ, Zhouc XP, Au CT: Appl. Catal. A Gen.. 2004, 277: 1. 10.1016/j.apcata.2004.09.020View ArticleGoogle Scholar
- Martensson T, Patrik C, Svensson T, Wacaser BA, Larsson MW, Seifert W, Deppert K, Gustafsson A, Wallenberg LR, Samuelson L: Nano Lett.. 2004, 4: 1987. COI number [1:CAS:528:DC%2BD2cXnsleisbY%3D] COI number [1:CAS:528:DC%2BD2cXnsleisbY%3D] 10.1021/nl0487267View ArticleGoogle Scholar
- Kim H-M, Kim DS, Park YS, Kim DY, Kang TW, Chung KS: Adv. Mater.. 2004, 14: 991.View ArticleGoogle Scholar
- Ertekin E, Greaney PA, Chrzan DC, Sands TD: J. Appl. Phys.. 2005, 97: 114325. Bibcode number [2005JAP....97k4325E] Bibcode number [2005JAP....97k4325E] 10.1063/1.1903106View ArticleGoogle Scholar
- Syrkin A, Usikov A, Soukhoveev V, Kovalenkov O, Ivantsov V, Dmitriev V, Collins C, Readinger E, Shmidt N, Davydov V, Nikishin S, Kuryatkov V, Song D, Rosenbladt D, Holtz M: Phys. Status Solidi. 2006, 3: 1444. COI number [1:CAS:528:DC%2BD28XmvFOrsbY%3D] COI number [1:CAS:528:DC%2BD28XmvFOrsbY%3D] 10.1002/pssc.200565454View ArticleGoogle Scholar
- Kryliouk O, Park HJ, Won YS, Anderson T, Davydov A, Levin I, Kim JH, Freitas JA: Nanotechnology. 2007, 18: 135606. Bibcode number [2007Nanot..18m5606K] Bibcode number [2007Nanot..18m5606K] 10.1088/0957-4484/18/13/135606View ArticleGoogle Scholar
- Park HJ, Kryliouk O, Anderson T, Khokhlov D, Burbaev T: Physica E. 2007, 37: 142. COI number [1:CAS:528:DC%2BD2sXjtFKjtbY%3D]; Bibcode number [2007PhyE...37..142P] COI number [1:CAS:528:DC%2BD2sXjtFKjtbY%3D]; Bibcode number [2007PhyE...37..142P] 10.1016/j.physe.2006.06.022View ArticleGoogle Scholar
- Ohta J, Fujioka H, Honke T, Oshima M: Thin Solid Films. 2004, 457: 109. COI number [1:CAS:528:DC%2BD2cXktVajsrY%3D]; Bibcode number [2004TSF...457..109O] COI number [1:CAS:528:DC%2BD2cXktVajsrY%3D]; Bibcode number [2004TSF...457..109O] 10.1016/j.tsf.2003.12.003View ArticleGoogle Scholar
- Lua CJ, Duan XF, Lu H, Schaff WJ: J. Mater. Res.. 2006, 21: 1693. Bibcode number [2006JMatR..21.1693L] Bibcode number [2006JMatR..21.1693L] 10.1557/jmr.2006.0215View ArticleGoogle Scholar