Axial Young’s modulus prediction of single-walled carbon nanotube arrays with diameters from nanometer to meter scales C. H. Sun, F. Li, H. M. Cheng, and G. Q. Lu Citation: Applied Physics Letters 87, 193101 (2005); doi: 10.1063/1.2119409 View online: http://dx.doi.org/10.1063/1.2119409 View Table of Contents: http://scitation.aip.org/content/aip/journal/apl/87/19?ver=pdfcov Published by the AIP Publishing Articles you may be interested in Comment on “Computation of Young’s moduli for chiral single-walled carbon nanotubes” [Appl. Phys. Lett.88, 251908 (2006)] Appl. Phys. Lett. 89, 216101 (2006); 10.1063/1.2396843 Temperature-dependent elastic properties of single-walled carbon nanotubes: Prediction from molecular dynamics simulation Appl. Phys. Lett. 89, 081904 (2006); 10.1063/1.2336622 Computation of Young’s moduli for chiral single-walled carbon nanotubes Appl. Phys. Lett. 88, 251908 (2006); 10.1063/1.2201637 A self-similar array model of single-walled carbon nanotubes Appl. Phys. Lett. 86, 203106 (2005); 10.1063/1.1926418 Young’s modulus of single-walled carbon nanotubes J. Appl. Phys. 84, 1939 (1998); 10.1063/1.368323 Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions. Download to IP: 130.102.42.98 On: Mon, 24 Oct 2016 23:12:55 APPLIED PHYSICS LETTERS 87, 193101 共2005兲 Axial Young’s modulus prediction of single-walled carbon nanotube arrays with diameters from nanometer to meter scales C. H. Sun, F. Li, and H. M. Chenga兲 Shenyang National Laboratory for Materials Science, Institute of Metal Research, Chinese Academy of Sciences, Shenyang 110016, China G. Q. Lu ARC Center for Functional Nanomaterials, The University of Queensland, Brisbane, QLD 4072, Australia 共Received 2 May 2005; accepted 1 September 2005; published online 31 October 2005兲 Based on a self-similar array model, we systematically investigated the axial Young’s modulus 共Y axis兲 of single-walled carbon nanotube 共SWNT兲 arrays with diameters from nanometer to meter scales by an analytical approach. The results show that the Y axis of SWNT arrays decreases dramatically with the increases of their hierarchy number 共s兲 and is not sensitive to the specific size s is independent of the and constitution when s is the same, and the specific Young’s modulus Y axis packing configuration of SWNTs. Our calculations also show that the Y axis of SWNT arrays with diameters of several micrometers is close to that of commercial high performance carbon fibers s of SWNT arrays is much better than that of high performance CFs. © 2005 共CFs兲, but the Y axis American Institute of Physics. 关DOI: 10.1063/1.2119409兴 Theoretical and experimental results have shown that individual single-walled carbon nanotubes 共SWNTs兲 have extremely high elastic modulus, greater than 1 T Pa,1,2 which has stimulated great efforts to synthesize or fabricate large SWNT arrays with a macrosize.3–10 Unfortunately, even the best macroscopic fibers made up of aligned SWNTs fall far short of the expected values.8,9,11–13 Moreover, it is widely observed that the axial mechanical performance of SWNT bundles strongly decreases with the increase of their diameters.11–14 To explain this phenomenon, Salvetat suggested that it is due to the possibility that larger ropes contain more imperfections than small ones; moreover, the absence of registry between neighboring tubes induced by variations in tube diameter and helicity.11 Also Yu et al. proposed that only the perimeter SWNTs act as the load-carrying elements.13 From the earlier work, it is concluded that the fundamental problem in translating the wonderful mechanical properties of individual SWNT into larger bundles may be achieved by strengthening intertube bonding,15 which has been realized by Kis et al. through irradiation of SWNT bundles with high-energy electrons,14 and a high bending modulus is achieved. Ajayan commented that this work paves the way towards realizing stronger nanotube fibers in the future.15 Behind the impressive work reported by Kis,14 however, there is still another basic obstacle, the packing of SWNTs. It has been found that SWNTs are apt to aggregate into bundles, bundles into bundle arrays, and so on.6,7,10 Ebbesen et al. figured out a schematic diagram of this hierarchy packing pattern of SWNTs, from large bundles down to individual carbon nanotubes.16 Different from the close packing, hierarchy SWNT arrays are much looser, as observed in experiments.6,7,10 Therefore, estimations of the mechanical properties of SWNT arrays are required to take the hierarchical structure of SWNT arrays into account. Previously, we have proposed a self-similar array model to quantitatively describe the hierarchy structures in SWNT arrays.17 Using this model, SWNT arrays, including close and hierarchy packing patterns, are universally described.17 Figure 1 presented a schematic view of hierarchy structures, from isolated SWNT to SWNT bundle and bundle arrays, according to the self-similar array model.17 And the goal of the present work is to study the effect of the hierarchical structure of SWNT arrays on their mechanical properties based on the self-similar array model of SWNTs, and a systematical estimation of the axial Yong’s modulus, Y axis, is carried out for SWNT arrays with diameters from nanometer to meter scales. To estimate the best performance of SWNT arrays at different scales, those adverse factors, such as impurity and irregularity of SWNTs, are not taken into account here. Hence, identical, infinitely long and straight SWNTs 关for instance, 共12, 12兲 nanotubes with a diameter D = 1.62 nm and a van der Waals gap G = 0.3162 nm兴18 are employed. To further simplify our discussion but without loss generality, only three kinds of SWNT arrays are investigated: 共cm, 1兲 for one 共isolated兲 bundles consisting of cm SWNTs 共specially, cm = 1 denotes an isolated SWNT兲, 共cm , cn兲 for the arrays of cn bundles and each bundle consisting of cm SWNTs, and a兲 FIG. 1. Schematic image of hierarchy structures of SWNT arrays, from isolated SWNT to SWNT bundle and to bundle array. Author to whom correspondence should be addressed; electronic mail: [email protected] Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions. Download to IP: 130.102.42.98 On: Mon, 24 Oct 2016 0003-6951/2005/87共19兲/193101/3/$22.50 87, 193101-1 © 2005 American Institute of Physics 23:12:55 193101-2 Appl. Phys. Lett. 87, 193101 共2005兲 Sun et al. 共cm , cn , cl兲 for a superstructure consisting of cl bundle arrays 共cm , cn兲. Also we define a concept of hierarchy number, s, for SWNT arrays, and s labels the times of self-similar transformation under the self-similar array model.17 For instance, 1, 2, and 3 times of self-similar transformations are needed to be carried out for the construction of hierarchy structures of 共cm , 1兲cm⫽1 , 共cm , cn兲cn⫽1, and 共cm , cn , cl兲cl⫽1 under the selfsimilar array model, respectively, hence, s = 1, 2, and 3. Specially, for isolated SWNT marked as 共1兲, no packing is carried out and no self-similar transformation is performed, hence, s = 0. Examples of isolated SWNT, SWNT bundle 共7, 1兲 and bundle array 共7,7兲 are presented in Fig. 1. Details and these notations can be found elsewhere.17 Since our estimation is carried out from several nanometers to meters, an analytical calculation method,19 rather than atomistic simulations, is employed Y axis = 2E ⫻ L ⫻ A, 2 共1兲 where 2E / 2 is the second derivative of energy with respect to strain along the tubule axis, and the value of 58.2 eV atom−1 was used for 2E / 2 independent of the tuFIG. 2. 共a兲 Calculated Young’s modulus, Y axis, for 14 SWNT arrays with diameters from 1 nm to 1 m. The point labeled by 䊏 corresponds to isolated bule diameter and packing configuration of SWNTs.20 L is 共12, 12兲 SWNT. 共b兲 Measured Y axis for SWNT arrays at nanometer and the number of atoms per tubule per unit length and A is the micrometer dimensions are compared with the calculated results and those number of tubules per unit area in the cross section. Clearly, for commercial carbon fibers. Experimental data are reported by Salvetat et for different packing patterns and configurations, the al. 共see Ref. 11兲 and Li et al. 共see Ref. 12兲. Dada of commercial carbon difference comes from A. Based on the self-similar array fibers are taken from Torayca Carbon Fibers America, Inc. for their products of T300, T800H, M40, and M60J. Values of 5 nm and 1 m are taken for model, A = 8cm / 3冑3D21, 8cmcn / 3冑3D22, and 8cmcncl / 3冑3D23 the scale increments before and after the break of the horizontal axis for a for 共cm, 1兲, 共cm , cn兲, and 共cm , cn , cl兲, respectively, better legibility. where D1 = 共2m + 1兲D + 2mG, D2 = 共2n + 1兲D1 + 2nG, and D3 = 共2l + 1兲D2 + 2lG. those experimental and calculated data of SWNT arrays with Figure 2共a兲 shows how the axial Young’s modulus of a diameter of several micrometers with those of commercial SWNT arrays from Eq. 共1兲 varies with packing configuracarbon fibers 共CFs兲, as shown in Fig. 2共b兲. Data of the comtions. We can see: 共1兲 the calculated Y axis for an isolated mercial carbon fibers are taken from Torayca Carbon Fibers 共12, 12兲 is highly consistent with the experimental result America, Inc. for their products of T300, T800H, M40, and cited in Ref. 11 共but this result was given by Chopra et al.2兲; M60J. The comparison in Fig. 2共b兲 suggests that, even 共2兲 Y 共1兲 ⬎ Y 共cm,1兲 ⬎ Y 共cm,cn兲 ⬎ Y 共cm,cn,cl兲. Obviously, the Y axis deSWNT arrays at the micrometer scale have a perfect struccreases rapidly with the increase of the hierarchy number s ture and packing density 共for s = 1兲, their axial Young’s of SWNT arrays; hence, decreasing the hierearchy of SWNT modulus is just similar to that of high modulus CFs. Morearrays is an effective way to improve their Young’s modulus; over, in our estimation, some complex structural factors are 共3兲 for SWNT arrays with the same s, the Y axis is not sensinot considered in the model yet, such as the nonuniformity of tive to their sizes. Using 共37,91, cl兲 for instance, when its SWNT diameters, packing density, and length distribution, diameter changes from 1 m to 1 m, the Y axis only decreases the distance between SWNT bundles or ropes, and these facfrom 318.7 to 316.4 GPa. 共4兲 The best Y axis of SWNT arrays tors normally can worsen the axial mechanical performance can be expected in SWNT bundles 共cm, 1兲, about 550–600 of SWNT arrays. Therefore, SWNT arrays with diameters of GPa at the scale of micrometers to meters. several micrometers do not present much advantage with reFigure 2共b兲 presents the experimental results of axial spect to commercial high performance carbon fibers if only Young’s modulus of SWNT arrays at the nanometer11 and the Young’s modulus is considered. However, with the incremicrometer dimensions.12 According to the description in the ment of diameters and hierarchy number s, the density of earlier references, we select two possible hierarchy strucSWNT arrays decreases, suggesting the specific Young’s tures, 共cm, 1兲 and 共37, cn , cl兲, to describe the samples emmodulus of SWNT arrays has a different changing tendency ployed in Refs. 11 and 12, respectively. The parameters cm, from the Y axis. Using the continuum model of SWNTs, the cn, and cl are determined by the formula of Di earlier, and specific density of SWNT arrays can be described by experimental values are taken for Di; for 共37, cn , cl兲, an assumption of cn = cl is made since the Y axis is not sensitive to their values. By these simplifications, a rough estimation is = A ⫻ D ⫻ ⫻ M C , 共2兲 carried out, as shown in Fig. 2共b兲. Considering the model and where labels the surface density of carbon atoms, method used here for so complex structures, the calculated = 4 / 共冑3a2兲, a = 2.49 Å is the lattice constant of carbon results are well consistent with the experimental data, which suggest that the earlier analysis based on the self-similar arnanotubes.21 M C is the atomic mass of carbon. Based on Eq. Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions. Download to IP: 130.102.42.98 On: Mon, 24 Oct 2016 ray model of SWNTs is reliable. Hence, we can compare 共1兲, the specific Young’s modulu of SWNT arrays is 23:12:55 193101-3 Appl. Phys. Lett. 87, 193101 共2005兲 Sun et al. 2E ⫻L 2 Y axis s Y axis = = . D ⫻ ⫻ M C 共3兲 s Y axis Obviously, the is independent of the packing configuras of individual tion of SWNTs, which suggests that the Y axis SWNTs can be theoretically realized at a macrodimension. s = 469 GPa, For 共12,12兲 SWNT arrays, for instance, the Y axis which is much higher than those of commercial CFs selected above, 131, 162, 305, 217 GPa for T300, T800H, M60J, and M40, respectively. Hence, SWNT arrays present significant s , importance for those applications in which the Y axis rather than the Y axis, is strictly required, such as the space elevator proposed by Edwards.22 In summary, the theoretical Young’s modulus of SWNT arrays with diameter from 1 nm to 1 m have been calculated based on the self-similar array model of SWNTs by an analytical approach. The agreement between experimental data and calculated results suggests that the present analysis based on the self-similar array model is reliable. The results show that the axial Young’s modulus of SWNT arrays, Y axis, decreases dramatically with the increment of their hierarchy number s and is not sensitive to the specific size and constitution when s is the same, which suggests that, to improve the axial mechanical properties of SWNT arrays, it is necessary to reduce the hierarchy of SWNT arrays. Our calculation also indicates that the high mechanical properties of individual SWNTs are possibly realized in a macroscale dimension if SWNT bundles with low hierarchy numbers can be closely packed, but at the micrometer dimension, the Y axis of SWNT arrays with diameters of several micrometers is close to that of commercial high performance carbon fibers. s is independent However, our calculations show that the Y axis of the packing configuration of SWNTs and, to fabricate s much higher than those of high SWNT array with the Y axis performance CFs, is theoretically possible. The authors would like to thank Dr. A. Kis and Professor L. Forrófor for their kind help. This work was supported by NSFC 共50328204, 90406012兲 and the State Major Basic Research Project of MOST 共G2000026403兲. The support from CAS Centre for Interfacial Materials, China and the ARC Centre for Functional Nanomaterials, Australia to this work are also acknowledged. J. P. Lu, Phys. Rev. Lett. 79, 1297 共1997兲. N. G. Chopra and A. Zettl, Solid State Commun. 105, 297 共1998兲. 3 A. Thess, R. Lee, P. Nikolaev, H. J. Dai, P. Petit, J. Robert, C. H. Xu, Y. H. Lee, S. G. Kim, A. G. Rinzler, D. T. Colbert, G. E. Scuseria, D. Tománek, J. E. Fishcher, and R. E. Smalley, Science 273, 483 共1996兲. 4 C Journet, W. K. Maser, P. Bernier, A. Loiseau, M. Lamy De La Chapelle, S. Lefrant, P. Deniard, R. Lee, and J. Fischer Nature 388, 756 共1997兲. 5 H. M. Cheng, F. Li, X. Sun, S. D. M. Brown, M. A. Pimenta, A. Marucci, G. Dresselhaus, and M. S. Dresselhaus, Chem. Phys. Lett. 289, 602 共1998兲. 6 C. Liu, H. M. Cheng, H. T. Cong, F. Li, G. Su, B. L. Zhou, and M. S. Dresselhaus, Adv. Mater. 共Weinheim, Ger.兲 12, 1190 共2000兲. 7 B. Vigolo, A. Penicaud, C. Coulon, C. Sauder, R. Pailler, C. Journet, and P. Poulin, Science 290, 1331 共2000兲. 8 H. W. Zhu, C. L. Xu, D. H. Wu, B. Q. Wei, R. Vajtai, and P. M. Ajayan, Science 296, 884 共2002兲. 9 A. B. Dalton, S. Collins, E. Munoz, J. Razal, V. H. Ebron, J. P. Ferraris, J. N. Coleman, B. G. Kim, and R. H. Baughman, Nature 423, 703 共2003兲. 10 L. M. Ericson, H. Fan, H. Peng, V. A. Davis, W. Zhou, J. Sulpizio, Y. Wang, R. Booker, J. Vavro, C. Guthy, A. N. G. Parra-Vasquez, M. J. Kim, S. Ramesh, R. Saini, C. Kittrell, G. Lavin, H. Schmidt, W. W. Adams, W. E. Billups, M. Pasquali, W.-F. Hwang, R. H. Hauge, J. E. Fischer, and R. E. Smalley, Science 305, 1447 共2004兲. 11 J. P. Salvetat, G. A. D. Briggs, J. M. Bonard, R. R. Bacsa, A. J. Kulik, T. Stöckli, N. A. Burnham, and L. Forró, Phys. Rev. Lett. 82, 944 共1999兲. 12 F. Li, H. M. Cheng, S. Bai, G. Su, and M. S. Dresselhaus, Appl. Phys. Lett. 77, 3161 共2000兲. 13 M. F. Yu, B. S. Files, S. Arepalli, and R. S. Rouff, Phys. Rev. Lett. 84, 5552 共2000兲. 14 A. Kis, G. Csányi, J. P. Salvetat, T. N. Lee, E. Couteau, A. J. Kulik, W. Benoit, J. Brugger, and L. Forró, Nat. Mater. 3, 153 共2004兲. 15 P. M. Ajayan and F. Banhart, Nat. Mater. 3, 135 共2004兲. 16 T. W. Ebbesen, H. Hiura, J. Fujita, Y. Ochiai, S. Matsui, and K. Tanigaki, Chem. Phys. Lett. 209, 83 共1993兲. 17 C. H. Sun, F Li, C. G. Liu, G. Q. Lu, and H. M. Cheng. Appl. Phys. Lett. 86, 203106 共2005兲. 18 C. H. Sun, L. C. Yin, F. Li, G. Q. Lu, and H. M. Cheng. Chem. Phys. Lett. 403, 343 共2005兲. 19 S. B. Sinnott, O. A. Shenderova, C. T. White, and D. W. Brenner, Carbon 36, 1 共1998兲. 20 D. H. Robertson, D. W. Brenner, and J. W. Mintmire. Phys. Rev. B 45, 12592 共1992兲. 21 R. Saito, G. Dresshaus, and M. S. Dresshaus, Physical Properties of Carbon Nanotubes 共Imperial College Press, London, 1998兲. 22 B. C. Edwards, NIAC Phase I Final Report, www.niac.usra.edu/studies under Edwards: Phase I under Final Report, 2000. 1 2 Reuse of AIP Publishing content is subject to the terms at: https://publishing.aip.org/authors/rights-and-permissions. Download to IP: 130.102.42.98 On: Mon, 24 Oct 2016 23:12:55
© Copyright 2026 Paperzz