Ruo-Yu Dong and
Bing-Yang Cao*
Key Laboratory for Thermal Science and Power Engineering of Ministry of Education, Department of Engineering Mechanics, Tsinghua University, Beijing 100084, P. R. China. E-mail: caoby@tsinghua.edu.cn; Fax: +86-10-6279-4531; Tel: +86-10-6279-4531
First published on 14th October 2015
The superhigh-speed unidirectional rotation of a carbon nanotube (CNT) induced by a linear shear flow is investigated by molecular dynamics simulations. We have identified three rotational types: “continuous rotation”, “interrupted rotation” and “simple oscillation”, corresponding to a decreased number of unidirectional rotation circles over the same time duration. It was found that the unidirectional motion and oscillation respectively originate from the applied shear and rotary Brownian motion by a decoupled analysis of the rotational features. The angular velocity of the unidirectional motion is over one order of magnitude larger than the Jeffery's theory. To construct a CNT-based rotary motor with good performance, the high-speed unidirectional angular velocity can be achieved by carefully selecting the shear rate (e.g. ∼2 × 108 rad s−1 at 35 GHz) and the continuous rotating state can be approached by using a low aspect ratio carbon nanotube.
When CNTs are dispersed in suspensions, an easy way to control its rotational motion is by imposing a fluid flow. Studies on this issue were mostly focusing on the orientation state18,19 and related rheological phenomena20 of CNT suspensions. However, the related motor study is scarce, only recently a nano-turbine model consisted of a CNT and three graphene blades was designed to rotate unidirectionally in water flow by molecular dynamics (MD) simulations.21 Some light was shed on this problem by Jeffrey22 in 1922 who theoretically predicted that a single ellipsoid would rotate unidirectionally in a single parameter family of closed orbits in a sheared viscous fluid. Later studies extended the Jeffery orbits to rod-shaped particles,23 just like CNT, and considered the influences of rotary Brownian motion.24,25 The MD results25 confirmed that the rotation period of a low aspect ratio CNT in linear shear agrees with Jeffery's theory with only a slight difference. The flow-induced nanoparticle rotation is actually a coupled effect from the applied shear and Brownian rotation, whose impacts have not been distinguished from each other previously. This study thus provides detailed analyses on a single CNT's two-dimensional (2D) rotational behavior and dynamics as well as the decoupled features and their origin by MD simulations. The simulated very small aspect ratio CNT is treated as a rigid rod19,25 without considering the effect of deformation.26,27 The high-speed unidirectional rotation is observed and the criteria to achieve it are discussed to better facilitate the CNT-based rotary motor design.
The superimposed simple linear shear flow is illustrated in Fig. 1(b) and in the form of vx = y, vy = vz = 0, where
stands for the shear rate. It was realized by utilizing the SLLOD algorithm.31 The Lee–Edwards boundary condition32 was applied in the y direction, which is the velocity gradient direction with periodic boundary conditions for the other two directions. The excess heat produced by the shear flow was extracted by the thermostat. The thermostat was only applied in two directions (y, z) and not in the flow direction (x).19,33,34 The results were collected after 3 × 105 time steps (3000 ps) to allow time for the flow to develop.
The CNT is confined only to rotate two-dimensionally (2D) on the x–y plane.35 Also shown in Fig. 1(b) is the definition of the CNT's directional angle φ, which is within a range of (−90°, 90°] and φ = 0° means the CNT axis is parallel to the flow direction x. To model a rod-shaped object, the CNT was treated as a rigid body. The base case is defined here: the nanotube has the armchair (5, 5) configuration with a diameter, d, of 0.7 nm and length, L, of 4.4 nm. The density, ρ, of the argon is 1091 kg m−3 and the temperature, T, is 300 K and the shear rate, , is 20.0 GHz. The simulated argon system is in a supercritical state. Later analyses will alter various factors based on the above selected state.
Next, the rotational modes will be decoupled to explore their physical origin as well as to better comprehend and control the above three rotational types. Shown in Fig. 2(b), the labels “1”, “2” and “3” indicate the distinctive segments of the CNT's rotational motion, about to be analyzed one by one in the following discussion. Label “1”: the oscillatory motion between two successive unidirectional rotations. The strength of the oscillation is characterized by the time-averaged frequency f. Label “2”: the total time period Tp of two successive unidirectional rotations and the oscillation in between. The simulation time is prolonged to ensure there are at least 10 individual sets of Tp to achieve its reliable average value. Label “3”: the unidirectional rotation, which is the focus of the present study. We use the angular velocity ω to characterize the unidirectional rotation speed, which was also averaged over 10 individual unidirectional rotations appearing with time. It should be noticed that the boundary between rotation and oscillation is not distinct and there exists a preferred orientation angle around +10° where the CNT oscillates around (Fig. 2(b)). Therefore, the intermediate total rotation angles of 120°, corresponding to the CNT orientation from −30° to 30° (refer to Fig. 2(d)), is used to measure the unidirectional angular velocity ω. As the simple oscillatory state does not exhibit any unidirectional motion (Fig. 2(a)), labels “2” and “3” will not be discussed at that circumstance.
Fig. 3(a) & (b) show the time-averaged oscillatory frequency f (label “1”) versus the rotational diffusion coefficient Dr or shear rate . The Dr used is a 2D rotary diffusivity calculated by equilibrium MD method based on the Einstein relation Dr = 〈(Δφ)2〉/2t, where 〈…〉 denotes the ensemble average, Δφ is the angular displacement and t is time.35 Here, we change the CNT length L, diameter d or fluid temperature T of the base case to obtain various Dr values. Interestingly, a positive linear function fits the relationship between the frequency f and Dr very well (Fig. 3(a)), while the frequency does not change with the increase of the shear rate (Fig. 3(b)). The calculated frequency is actually a measure of the strength of the back-and-force oscillation. The monotonic dependence in Fig. 3(a) indicates that in nature the oscillation originates from the rotary Brownian motion, which can be quantified by the rotational diffusivity Dr. As Dr is a transport coefficient and not affected by the applied shear, the time-averaged frequency will also stay constant when the shear rate changes.
Our current results show that the unidirectional rotations get interrupted occasionally by oscillatory motion, and thus it is not in agreement with the characteristics of continuous Jeffery orbits.22 Note that the CNT approximately experiences 180° during one unidirectional rotation, and then the time elapsed between two successive rotations, i.e. Tp (label “2”), may be assumed as the periodic time of the rotating CNT, which can be compared with Jeffery's theory. For a particle circulating around the Jeffery orbits, , where re can be expressed as a function of the CNT's aspect ratio L/d (ref. 23)
. The dependence of the periodic time Tp on aspect ratio L/d in Fig. 4(a) exhibits some similar trends, i.e. larger L/d leads to larger Tp, as that of the theoretical predictions. However, quantitative agreement is lacking, especially at high shear rate
= 35.0 GHz. This discrepancy can be further revealed in Fig. 4(b), where Tp first decreases with the increase of the shear rate, in agreement with the theoretical line, while followed by a completely opposite trend at high shear rate. When the shear rate is further increased (>50 GHz), the orientation type of simple oscillation appears and Tp equals to infinity. The above observation thus indicates that the periodic time is not only determined by the applied shear, indicated in Jeffery's theory, but also affected by the rotary Brownian motion, whose presence somehow brings about the unexpected simple oscillatory state and in turn alters the periodic time.
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Fig. 4 Dependences of the periodic time Tp (a) on the aspect ratio L/d and (b) on the shear rate ![]() |
The above calculated periodic time contains the information of both the unidirectional rotations and the oscillatory motion in between. When we focus on the design of a CNT-based motor, the segments of unidirectional rotations are of primary concern. Then, like Fig. 2(d), only the clockwise rotary motion is picked out for analysis (label “3”). Quite different from the dependences of the angular frequency on Dr and , the angular velocity ω of the unidirectional rotations does not change with the rotational diffusivity (Fig. 5(a)), i.e. ω not affected by the CNT length, diameter and fluid temperature, while it increases linearly with the shear rate (Fig. 5(b)). This evidently suggests that the unidirectional rotation is dominated by the applied shear and not much influenced by the random Brownian motion.
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Fig. 5 Dependences of the angular velocity ω of the unidirectional rotation (a) on the rotational diffusion coefficient Dr and (b) on the shear rate ![]() |
The present shear-induced rotary CNT can yield a clockwise angular velocity as high as 2.86 × 1010 rad s−1 at = 35 GHz (Fig. 5(b)). When Jeffery's predictions are expressed in terms of the angular velocity, we find that the simulated superhigh angular velocity is larger than those by over one order of magnitude (Fig. 5(b)). As the angular velocity increases with the shear rate, it may be tempting to conclude that the higher shear rate, the faster and more functional rotary motor. This is however not the case because of the occurrence of simple oscillatory state at very high shear (
> 50 GHz) as previously mentioned. The other limit of very small shear rate (
< 1 GHz) is not desirable either, for the rotary motion is random and unpredictable, approaching the equilibrium state. Therefore, some intermediate shear rate values should be selected for designing such CNT motor. Moreover, among the three introduced rotational types, the continuous rotating state (Fig. 2(a)) may be preferable, while no clear boundary exists between “interrupted rotation” and “continuous rotation”. What we need then is to approach the continuous state, by directly reducing the aspect ratio L/d, reflected by the fact that a smaller L/d brings about a smaller Tp in Fig. 4(a) and thus more circles of clockwise rotations over the same time duration.
Another issue that should be discussed is the very high shear rate used in MD simulations: the shear rates (0.1–200 GHz, i.e. 1 × 108 to 2 × 1011 s−1) in the present calculations are much higher than those in real cases, e.g. experiments on carbon nanotube suspensions, : 0.1 s−1 to 500 s−1.36,37 This high shear was selected to avoid a poor signal to noise ratio, which is harmful to nonequilibrium MD simulations. If the signal, i.e. shear rate, is too small, the established velocity profile will be greatly distorted from the linear shape and the shear-induced results will not be meaningful.38 Moreover, although the GHz value cannot be realized in real experiments, to relate the current study with practical situations we should rather utilize the Peclet number. It is defined as Pe =
/Dr, and was previously used as a scaling parameter to quantitatively characterize CNT's orientation order under high shear.19 The above analyses have revealed that the rotational behavior in nature originates from the coupled effects of
and Dr, and thus Pe rather than the shear rate should be paid more attention.20,39 In our simulations, Pe was in the range of 0–2000. However, in experiments, Pe can be as large as 108 (ref. 39) due to a very small Dr. A negative correlation exists between Dr and the particle length. When the length of the particle is at the scale of submicron or micron, Dr can be extremely small and Pe is very large. It is then expected that at similar Pe number, we may find the experimental counterparts of the simulated results.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c5ra18901b |
This journal is © The Royal Society of Chemistry 2015 |