Diameter-Dependent Bending Modulus of Individual Multiwall Boron Nitride Nanotubes

Modulus-BNNTs-2013

The mechanical properties of individual multi-wall boron nitride nanotubes (MWBNNTs) synthesized by a growth-vapor-trapping chemical vapor deposition method are investigated by a three-point bending technique via atomic force microscopy. Multiple locations on suspended tubes are probed in order to determine the boundary conditions of the supported tube ends. The bending moduli (EB) calculated for 20 tubes with diameters ranging from 18 to 58 nm confirm the exceptional mechanical properties of MWBNNTs, with an average EB of 760 ± 30 GPa. For the first time, the bending moduli of MWBNNTs are observed to increase with decreasing diameter, ranging from 100 ± 20 GPa to as high as 1800 ± 300 GPa. This diameter dependence is evaluated by Timoshenko beam theory. The Young’s modulus and shear modulus were determined to be 1800 ± 300 and 7 ± 1 GPa, respectively, for a trimmed data set of 16 tubes. The low shear modulus of MWBNNTs is the reason for the detected diameter-dependent bending modulus and is likely due to the presence of interwall shearing between the crystalline and faceted helical nanotube structures of MWBNNTs.

High-density vertically aligned multiwalled carbon nanotubes with tubular structures

CNTs-APL2005

Ammonia sNH3d gas was thought to be essential for the growth of vertically aligned multiwalled

carbon nanotubes sVA-MWCNTsd and led to the formation of bamboo-like structures. Here, we

show that VA-MWCNTs with ideal tubular structures can be grown on substrates by various mixed

gases with or without NH3 gas. The growth of these VA-MWCNTs is guided by a growth model that

combined the dissociative adsorption of acetylene molecules sC2H2d and the successive

vapor-liquid-solid growth mechanism. Results indicate that the key factor for growing these

VA-MWCNTs is a balance between the decomposition rate of the C2H2 molecules on the iron

catalyst and the subsequent diffusion and segregation rates of carbon.

© 2005 American Institute of Physics. fDOI: 10.1063/1.1952575g