Large-Scale Fabrication of Boron Nitride Nanotubes via a Facile Chemical Vapor Reaction Route and Their Cathodoluminescence Properties
© Zhong et al. 2010
Received: 10 July 2010
Accepted: 9 September 2010
Published: 26 September 2010
Cylinder- and bamboo-shaped boron nitride nanotubes (BNNTs) have been synthesized in large scale via a facile chemical vapor reaction route using ammonia borane as a precursor. The structure and chemical composition of the as-synthesized BNNTs are extensively characterized by X-ray diffraction, scanning electron microscopy, high-resolution transmission electron microscopy, and selected-area electron diffraction. The cylinder-shaped BNNTs have an average diameter of about 100 nm and length of hundreds of microns, while the bamboo-shaped BNNTs are 100–500 nm in diameter with length up to tens of microns. The formation mechanism of the BNNTs has been explored on the basis of our experimental observations and a growth model has been proposed accordingly. Ultraviolet–visible and cathodoluminescence spectroscopic analyses are performed on the BNNTs. Strong ultraviolet emissions are detected on both morphologies of BNNTs. The band gap of the BNNTs are around 5.82 eV and nearly unaffected by tube morphology. There exist two intermediate bands in the band gap of BNNTs, which could be distinguishably assigned to structural defects and chemical impurities.
KeywordsBoron nitride nanotubes Luminescence performance Growth mechanism Ammonia borane
As structural analogs of carbon nanotubes (CNTs), boron nitride nanotubes (BNNTs) have attracted continuous attention owing to their extraordinary structural and physical properties [1, 2]. Similar to CNTs, BNNTs possess a superior Young's modulus and a high thermal conductivity [3–6]. BNNTs are electrical insulator and transparent to visible light due to a wide band gap (around 5.2–5.8 eV) that is almost independent of tube chirality [7, 8]. Furthermore, BNNTs exhibit excellent chemical stability and inoxidizability [2, 9]. The unique structure-induced properties of BNNTs bring a series of opportunities for their potential applications as hydrogen storage media, biological probes, piezoelectric materials, composite reinforcements and harsh-environment semiconductor devices [10–17]. These promises have motivated intense research efforts seeking to develop synthetic strategies for preparing BNNTs.
Despite the structural similarity between BNNTs and conventional CNTs, great challenges have been encountered in fabricating BNNTs compared with the relative ease of synthesizing CNTs. Many techniques, such as arc-discharge , ball milling and annealing [18–21], laser ablation [22–24], chemical vapor deposition [25, 26], oven heating proper B and N containing precursors [27, 28], template confining [29, 30], and so forth, have been attempted to fabricate the BNNTs in recent years. Although some success has been achieved in producing pure and well-crystallized BNNTs, these techniques generally require special equipments or complex synthesis procedures and the yields of BNNTs are commonly disappointingly low.
Here, we describe a facile growth technique that can easily and reliably produce macroscopic amounts (~200 mg per experimental run) of BNNTs with cylinder and bamboo-shaped morphologies. Ammonia borane (AB, H3BNH3), which contains only B, N and H elements, is demonstrated to be an effective starting material for the fabrication of BNNTs. The structures and luminescence performance of the as-synthesized BNNTs have been extensively characterized. A two-step growth model has been established based on the analysis of the structures of BNNTs and the reaction process. The present work provides a facile synthetic approach and a deeper insight into the luminescence performance of BNNTs, which facilitates large-scale production of BNNTs and their application as compact ultraviolet (UV) laser devices.
In this study, we present a simple approach for the fabrication of BNNTs in a gas pressure furnace. Ammonia borane (AB) synthesized according to Ramachandran  was used as a starting material, and ferrocene was used as a catalyst. In a typical procedure, AB powder (4.0 g) and ferrocene (1.5 g) were mixed and charged into an graphite crucible of about 2 l capacity using a piece of graphite paper as inner lining, then the crucible was loaded into the furnace chamber. The chamber was sealed and pumped down to a base pressure of 0.1 Pa. Subsequently, 0.8 MPa high pure nitrogen was pressed into the furnace chamber. The furnace was heated to 1,450°C at a rate of 10°C min-1 and held for 60 min before it was finally cooled to room temperature. The BNNTs were found on the graphite paper. The samples obtained were extensively characterized by scanning electron microscopy (SEM, MX2600EF equipped with energy dispersive X-ray spectroscopy (EDX)), transmission electron microscopy (TEM, Philips Tecnai 20 and Tecnai F30 FEG equipped with electron energy loss spectroscopy (EELS)), X-ray powder diffraction (XRD, Rigaku D/max-γB X-ray diffractometer with Cu K radiation (λ = 0.154178 nm)), X-ray photoelectron spectroscopy (XPS, PHI 5700 ESCA System with a PC-ACCESS data analysis system (Physical Electronics Inc.)), Fourier transformation infrared spectroscopy (FTIR, Perkin Elmer spectrum one system by using pressed KBr disks) and ultraviolet–visible spectroscopy (Perkin-Elmer Lambda 950 UV/Vis Spectrophotometer). Cathodoluminescence (CL) measurements were performed using a Gatan MONOCL3 + system installed on a JSM-7000F SEM.
Results and Discussion
The particle on the tip of the cylindrical BNNT is believed to be the catalyst that catalyzes the growth of the nanotube. A representative SAED pattern taken from the particle is shown in Figure 3b, which can be indexed as that taken along the [1–11] zone axis of a Fe3C crystal (JCPDS 35-0772). Sharp spots from the (002) plane of h-BN (JCPDS 34-0421) are also clearly observed, which apparently originate from the BN walls encapsulating the particle. It is noteworthy that no spots could be indexed to α-Fe, implying that no α-Fe phase is encapsulated in the tip. The EDX spectrum acquired from the tip of a cylindrical BNNT is displayed in Figure 3d, which clearly shows the strong signals from Fe and C, together with B and N. The EDX result further demonstrates that the metal particles encapsulated in the tips of BNNTs are Fe3C rather than simple substance α-Fe, which is in agreement with the SAED analysis.
Quantitative analysis also gives a stoichiometric composition of BN, indicating that the bamboo-shaped 1D nanostructures are BNNTs. Although some empty knobs are occasionally observed, most knobs contain uniform quasi-spherical catalyst particles inside. These catalyst particles are confirmed to be Fe3C by SAED pattern, as shown in Figure 4b. Similar to that of cylindrical BNNTs, α-Fe phase was not detected in the knobs of bamboo-shaped BNNTs. EDX analysis was also performed to verify the chemical composition of the particles in the knobs, as shown in Figure 4f, which also confirms that the particle is Fe3C. Bamboo-shaped BNNTs containing α-Fe in their knobs has been reported previously , but in our case, the particles contained in the knobs of the BNNTs are Fe3C instead of α-Fe, which might imply a different formation mechanism of the bamboo-shaped BNNTs. It is noted that the catalyst that catalyzed the growth of both BNNTs is Fe3C rather than α-Fe. This is beneficial to the low-temperature growth of BNNTs since the melting point of Fe3C is much lower than that of α-Fe.
Several interesting features of the bamboo-shaped BNNTs are evidenced by HRTEM analysis. Figure 4c shows a HRTEM image of a BN shell that encapsulates a catalyst particle. Some dark regions originating from edge dislocations could be clearly observed, especially in zones far from the catalyst, as marked by arrows. These dislocations are caused by inherent strains , implying the existence of stresses in the outer BN layers. HRTEM image displayed in Figure 4d suggests that the junctions of bamboo units are formed by continuous BN layers and the bamboo units are tightly linked. Figure 4e shows a typical HRTEM image of the interface between a catalyst particle and the tube wall, revealing a poor compatibility between the catalyst particle and the inner wall of the BNNTs since the contact angle is about 140 degrees (much larger than 90 degrees). The poor compatibility facilitates the growth of hollow BNNTs without catalysts filling because molten catalyst particle with a high surface tension tends to fuse together and move as a whole.
To gain a better understanding of the growth mechanism of the BNNTs, a variety of controlled experiments were carried out. It is found that BNNTs could be obtained within a wide temperature range of 900–1,600°C (see Figure S1 in supporting information). The highest yield is achieved at about 1,450°C. BNNTs could also be obtained under argon atmosphere, but the yields are generally low (see Figure S2 in supporting information). When the amount of ammonia borane is increased, diameters of the BNNTs are dramatically enlarged and their structures are ultimately altered (see Figure S3 in supporting information). This is attributed to the high concentration of B and N containing gases, which may accelerate the growth rate of BNNTs and result in the structural alteration.
As soon as the supersaturated catalyst particles are formed, BN layers begin to precipitate from the catalyst particles onto the surfaces. At this juncture, BNNTs are likely to grow in different scenarios because the precipitation rate of B and N atoms might depend on the curvatures of the catalyst particles, similar to that occurs in the growth process of CNTs [41, 42]. BN sheets on smaller catalyst particles exhibit larger curvatures, and their formation are energetically unfavorable. Thus, the precipitation of B and N atoms from smaller catalyst particles is relatively slow. The B and N atoms have enough time to locate themselves onto favorable sites, i.e., the edges of the formerly formed BN sheets, which would push the catalyst particles on the tube tips to go ahead and facilitate the growth of the C-BNNTs, as shown in Figure 7f. This is essentially the well-known vapor–liquid–solid (VLS) growth process . On the contrary, the surfaces of the larger catalyst particles are more flat, and the precipitation of the B and N atoms on such surfaces are more energetically favorable. The BN sheets precipitate at such a high rate that they form a BN shell around the catalyst particles. The newly formed BN layers between the formerly formed BN shells and the molten catalyst particle would exert a stress on both sides, which may extrude the molten catalyst particle outside of the BN shell (Figure 7b). During the extruding process, the catalyst particle continues to adsorb source vapors and precipitate BN layers forming the tubular part of the bamboo-shaped BNNTs, as shown in Figure 7c and upper inset of Figure 4a. Consequently, the catalyst particle is present at the open end of the bamboo unit, and the growth of the following generation of bamboo unit will continue, as illustrated in Figure 7d, e.
To investigate the luminescence performances of bamboo-shaped BNNTs and cylindrical BNNTs, cathodoluminescence (CL) analyses were performed on the tubular parts of both BNNTs, as displayed in Figure 8b, c. Both spectra exhibit similar UV emission peaks, suggesting that the BNNTs could be potentially used as compact UV laser emitters. These emission peaks could be understood by virtue of an energy level diagram (see Figure 8d). The onsets of both CL spectra at about 5.82 eV correspond to the band-edge emission of BNNTs, which are consistent with the result of ultraviolet–visible spectroscopy analysis. The broad luminescence peaks around 4.0 eV and 1.8 eV in both spectra could be attributed to the same intermediate band (designated as band Ia), while the peaks centered at 3.09 and 2.71 eV could be ascribed to another intermediate band (designated as band Ib). Luminescence peaks originating from these two intermediate bands are commonly observed in the luminescence spectra of multiwalled BN nanotubes and BN whiskers, but the origin of these two intermediate bands is still the subject of debates [47–49]. Since both types of BNNTs used in our study are grown under the same experimental conditions, we therefore expect that the impurities contained in both BNNTs are similar and the differences of the luminescence performance are primarily caused by structure differences. The emission peaks identified in the two CL spectra are basically the same except that the emission peak around 4.0 eV is dramatically broadened in the CL spectrum of bamboo-shaped BNNTs. This implies that band Ia in bamboo-shaped BNNTs is broader than in C-BNNTs. Therefore, band Ia most probably arises from structural defects since it is morphology dependent, while band Ib is safely attributed to chemical impurities since this band is almost the same for both BNNTs and is not affected by tube morphologies.
In summary, we have developed a new approach to the fabrication of BNNTs with two morphologies using ammonia borane as a precursor. This method has the advantages of being simple and having a high yield. The structures and chemical compositions of the BNNTs are extensively characterized. The formation process of the BNNTs is interpreted by a two-stage growth mechanism. The luminescence performances of the BNNTs are investigated. It is found that the energy band gap of the BNNTs is independent of the tube morphologies. Luminescence peaks arising from the structural defects and chemical impurities have been distinguished. This method represents a facile path to large-scale synthesis of BNNTs with two morphologies, which can be used for future compact UV emitters.
This work was supported by National High-tech R&D Program (863 Program) (No. 2007AA03Z340), National Science Foundation of China (No. 50672018) and Program of Excellent Team in Harbin Institute of Technology.
- Chopra NG, Luyken RJ, Cherrey K, Crespi VH, Cohen ML, Louie SG, Zettl A: Science. 1995, 269: 966. 10.1126/science.269.5226.966View ArticleGoogle Scholar
- Golberg D, Bando Y, Tang CC, Zhi CY: Adv Mater. 2007, 19: 2413. 10.1002/adma.200700179View ArticleGoogle Scholar
- Chopra NG, Zettl A: Solid State Commun. 1998, 105: 297. 10.1016/S0038-1098(97)10125-9View ArticleGoogle Scholar
- Suryavanshi AP, Yu MF, Wen JG, Tang CC, Bando Y: Appl Phys Lett. 2004, 84: 2527. 10.1063/1.1691189View ArticleGoogle Scholar
- Kim P, Shi L, Majumdar A, McEuen PL: Phys Rev Lett. 2001, 8721: 215502. 10.1103/PhysRevLett.87.215502View ArticleGoogle Scholar
- Chang CW, Fennimore AM, Afanasiev A, Okawa D, Ikuno T, Garcia H, Li DY, Majumdar A, Zettl A: Phys Rev Lett. 2006, 97: 085901. 10.1103/PhysRevLett.97.085901View ArticleGoogle Scholar
- Zhi CY, Bando Y, Tang CC, Xie RG, Sekiguchi T, Golberg D: J Am Chem Soc. 2005, 127: 15996. 10.1021/ja053917cView ArticleGoogle Scholar
- Blase X, Rubio A, Louie SG, Cohen ML: Europhys Lett. 1994, 28: 335. 10.1209/0295-5075/28/5/007View ArticleGoogle Scholar
- Tang CC, Bando Y: Appl Phys Lett. 2003, 83: 659. 10.1063/1.1595721View ArticleGoogle Scholar
- Mpourmpakis G, Froudakis GE: Catal Today. 2007, 120: 341. 10.1016/j.cattod.2006.09.023View ArticleGoogle Scholar
- Bai XD, Golberg D, Bando Y, Zhi CY, Tang CC, Mitome M, Kurashima K: Nano Lett. 2007, 7: 632. 10.1021/nl062540lView ArticleGoogle Scholar
- Ciofani G, Raffa V, Menciassi A, Cuschieri A: Nano Today. 2009, 4: 8. 10.1016/j.nantod.2008.09.001View ArticleGoogle Scholar
- Chen X, Wu P, Rousseas M, Okawa D, Gartner Z, Zettl A, Bertozzi CR: J Am Chem Soc. 2009, 131: 890. 10.1021/ja807334bView ArticleGoogle Scholar
- Raffa V, Ciofani G, Cuschieri A: Nanotechnology. 2009, 20: 075104. 10.1088/0957-4484/20/7/075104View ArticleGoogle Scholar
- Maguer A, Leroy E, Bresson L, Doris E, Loiseau A, Mioskowski C: J Mater Chem. 2009, 19: 1271. 10.1039/b815954hView ArticleGoogle Scholar
- Zhi CY, Bando Y, Terao T, Tang CC, Kuwahara H, Golberg D: Adv Funct Mater. 2009, 19: 1857. 10.1002/adfm.200801435View ArticleGoogle Scholar
- Zhi CY, Bando Y, Tang CC, Huang Q, Golberg D: J Mater Chem. 2008, 18: 3900. 10.1039/b804575eView ArticleGoogle Scholar
- Chen Y, Conway M, Williams JS, Zou J: J Mater Res. 2002, 17: 1896. 10.1557/JMR.2002.0281View ArticleGoogle Scholar
- Chen H, Chen Y, Liu Y, Fu L, Huang C, Llewellyn D: Chem Phys Lett. 2008, 463: 130. 10.1016/j.cplett.2008.08.007View ArticleGoogle Scholar
- Li LH, Chen Y, Glushenkov AM: Nanotechnology. 2010, 21: 105601. 10.1088/0957-4484/21/10/105601View ArticleGoogle Scholar
- Lim SH, Luo JZ, Ji W, Lin J: Catal Today. 2007, 120: 346. 10.1016/j.cattod.2006.09.016View ArticleGoogle Scholar
- Laude T, Matsui Y, Marraud A, Jouffrey B: Appl Phys Lett. 2000, 76: 3239. 10.1063/1.126593View ArticleGoogle Scholar
- Lee RS, Gavillet J, de la Chapelle ML, Loiseau A, Cochon JL, Pigache D, Thibault J, Willaime F: Phys Rev B. 2001, 64: 121405(R).View ArticleGoogle Scholar
- Arenal R, Stephan O, Cochon J-L, Loiseau A: J Am Chem Soc. 2007, 129: 16183. 10.1021/ja076135nView ArticleGoogle Scholar
- Guo L, Singh RN: Nanotechnology. 2008, 19: 065601. 10.1088/0957-4484/19/6/065601View ArticleGoogle Scholar
- Lee CH, Xie M, Kayastha V, Wang JS, Yap YK: Chem Mater. 2010, 22: 1782. 10.1021/cm903287uView ArticleGoogle Scholar
- Tang C, Bando Y, Sato T, Kurashima K: Chem Commun. 2002., 1290:Google Scholar
- Chen ZG, Zou J, Li F, Liu G, Tang DM, Li D, Liu C, Ma XL, Cheng HM, Lu GQ, Zhang ZD: Adv Funct Mater. 2007, 17: 3371. 10.1002/adfm.200700296View ArticleGoogle Scholar
- Bechelany M, Bernard S, Brioude A, Cornu D, Stadelmann P, Charcosset C, Fiaty K, Miele P: J Phys Chem C. 2007, 111: 13378. 10.1021/jp074178kView ArticleGoogle Scholar
- Wang XZ, Wu Q, Hu Z, Chen Y: Electrochim Acta. 2007, 52: 2841. 10.1016/j.electacta.2006.08.047View ArticleGoogle Scholar
- Ramachandran PV, Gagare PD: Inorg Chem. 2007, 46: 7810. 10.1021/ic700772aView ArticleGoogle Scholar
- Ma RZ, Bando Y, Sato T, Kurashima K: Chem Mater. 2001, 13: 2965. 10.1021/cm0102741View ArticleGoogle Scholar
- Lee CH, Wang JS, Kayatsha VK, Huang JY, Yap YK: Nanotechnology. 2008, 19: 455605. 10.1088/0957-4484/19/45/455605View ArticleGoogle Scholar
- Moulder JF: Handbook of X-ray Photoelectron Spectroscopy: A Reference Book of Standard Spectra for Identification and Interpretation of XPS Data. Perkin-Elmer, Eden Prairie; 1992.Google Scholar
- Kuznetsov VL, Mazov IN, Delidovich AI, Obraztsova ED, Loiseau A: Phys Status Solidi B. 2007, 244: 4165. 10.1002/pssb.200776171View ArticleGoogle Scholar
- Barreiro A, Hampel S, Rummeli MH, Kramberger C, Gruneis A, Biedermann K, Leonhardt A, Gemming T, Buchner B, Bachtold A, Pichler T: J Phys Chem B. 2006, 110: 20973. 10.1021/jp0636571View ArticleGoogle Scholar
- Baitalow F, Baumann J, Wolf G, Jaenicke-Rossler K, Leitner G: Thermochim Acta. 2002, 391: 159. 10.1016/S0040-6031(02)00173-9View ArticleGoogle Scholar
- Paine RT, Narula CK: Chem Rev. 1990, 90: 73. 10.1021/cr00099a004View ArticleGoogle Scholar
- Wideman T, Sneddon LG: Inorg Chem. 1995, 34: 1002. 10.1021/ic00108a039View ArticleGoogle Scholar
- Shore SG, Hickam CW: Inorg Chem. 1963, 2: 638. 10.1021/ic50007a054View ArticleGoogle Scholar
- Sanchez-Portal D, Artacho E, Soler JM, Rubio A, Ordejon P: Phys Rev B. 1999, 59: 12678. 10.1103/PhysRevB.59.12678View ArticleGoogle Scholar
- Kuznetsov VL, Usoltseva AN, Chuvilin AL, Obraztsova ED, Bonard J-M: Phys Rev B. 2001, 64: 235401. 10.1103/PhysRevB.64.235401View ArticleGoogle Scholar
- Morales AM, Lieber CM: Science. 1998, 279: 208. 10.1126/science.279.5348.208View ArticleGoogle Scholar
- Wirtz L, Marini A, Rubio A: Phys Rev Lett. 2006, 96: 126104. 10.1103/PhysRevLett.96.126104View ArticleGoogle Scholar
- Arenal R, Stéphan O, Kociak M, Taverna D, Loiseau A, Colliex C: Phys Rev Lett. 2005, 95: 127601. 10.1103/PhysRevLett.95.127601View ArticleGoogle Scholar
- Kubota Y, Watanabe K, Tsuda O, Taniguchi T: Science. 2007, 317: 932. 10.1126/science.1144216View ArticleGoogle Scholar
- Tang CC, Bando Y, Zhi CY, Golberg D: Chem Commun. 2007., 4599:Google Scholar
- Su CY, Chu WY, Juang ZY, Chen KF, Cheng BM, Chen FR, Leou KC, Tsai CH: J Phys Chem C. 2009, 113: 14732. 10.1021/jp904583pView ArticleGoogle Scholar
- Zhu Y-C, Bando Y, Xue D-F, Sekiguchi T, Golberg D, Xu F-F, Liu Q-L: J Phys Chem B. 2004, 108: 6193. 10.1021/jp035856fView ArticleGoogle Scholar
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