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Transportation efficiency of hydrodynamically coupled spherical oscillators in low Reynolds number fluids

Weiwei Su [ Email: [email protected] Department of Mathematical Informatics, The University of Tokyo, Bunkyo City, Tokyo 113-8654, Japan    Yuki Izumida Email: [email protected]    Hiroshi Kori Email: [email protected] Department of Mathematical Informatics, The University of Tokyo, Bunkyo City, Tokyo 113-8654, Japan Department of Complexity Science and Engineering, The University of Tokyo, Kashiwa, Chiba 277-0882, Japan
Abstract

Most bacteria are driven by the cilia or flagella, consisting of a long filament and a rotary molecular motor through a short flexible hook. The beating pattern of these filaments shows synchronization properties from hydrodynamic interactions, especially in low Reynolds number fluids. Here, we introduce a model based on simple spherical oscillators which execute oscillatory movements in one dimension by an active force, as a simplified imitation of the movements of cilia or flagella. It is demonstrated that the flow, measured by the net transportation of a test particle, is generated by a chain of oscillators and enhanced by the hydrodynamic interactions between beads, with supports from both perturbative and numerical results. Transportation efficiency also highly correlates with hydrodynamic interactions. Increments of bead numbers are generally expected to produce stronger flow and efficiency, at least for small numbers of beads.

preprint: APS/123-QED

I Introduction

The cilia and flagella are the fundamental organs for microorganisms as the instruments of swimming in low Reynolds number environments [1, 2] and transporting materials like protein [3]. The undergoing mechanics in their wave-like behaviors is also a perfect paradigm for the study of active matter [4]. The synchronization of the beating pattern of these filaments is common [5]. Usually, for example, bacteria perform a two-gait “run-and-tumble” motion in fluids [6]. From repeating such motion the bacteria gain the net momentum in order to move. Thus it is worth investigating the mechanism behind such behavior in an analytical interpretation.

Some experimental studies take efforts to discover the relation between viscous hydrodynamic interaction and synchronization, as Taylor originally proposed [7]. Experiments on carpets of bacteria with active flagella [8] and arrays of artificial magnetically actuated cilia [9, 10, 11] have found collective effects via hydrodynamic interactions such as complex flow patterns and collective phase shifts. Through the synchronization of filaments, it is well known that the energy dissipation of the model can be minimized [12], so one can expect that such collective effects provide sufficient influence over the performance of the oscillator model.

The dynamic of passively induced movement generated by the flagella is a highly complex elastohydrodynamic problem [13]. Therefore, in order to solve such a model, a computationally simple but still practically accurate model is required. It has been a popular idea of representing slender filaments by spheres for hydrodynamic modeling [14]. Uchida and Golestanian propose a generic criterion to reach stabilized states for two beads with arbitrary but periodic trajectory and force profile [15]. Recently, the details of hydrodynamic effects are categorized by direct and indirect effects from the slender structure of filaments, from approximating the filament as a point mass orbiting around the cell [16].

One representative of a minimal model can be found in Ref. [17]. In this literature, a pair of spherical beads orbiting in the same shape of periodic trajectory near a wall is investigated. At first, the linear stability of the synchronized state is analyzed and examined by, for instance, circular, linear, and elliptical trajectories. Furthermore, the analysis of nonlinear evolution for these trajectories is done in the far-field limit, as well as their near-field interaction between two beads due to the finite size of the trajectory.

For a better comprehension of the low Reynolds number hydrodynamics, there are literatures such as Kotar et al. [18], which focuses on the optimal condition of hydrodynamic synchronization for rotors in circular trajectories. This article numerically examines the model setups proposed by Niedermayer et al. [19] and Uchida & Golestanian [15], that a smaller spring stiffness or larger asymmetry leads to stronger coupling condition and synchronization. Another conclusion is, if some thermal noise is included in the original setup, the synchronization still holds for not very high temperatures. Liao & Lauga [20] have examined a model of two spherical bodies in circular orbits of late as well, and the condition of minimal energy dissipation rate is discovered.

In this article, we build a simple model, namely, a chain of spherical beads that oscillate in a one-dimensional orbit and are hydrodynamically coupled with one another, and focus on the transportation efficiency of the system, which is rarely focused on by previous literature. Our results are expected to contribute to describe the ciliary motion in mucociliary transport of the respiratory system and oviduct transport of the female reproductive system [21, 22, 23, 24]. Moreover, the metachronal pattern we discovered in the case of many beads provides theoretical implications for some motion generated from motile cilia in bacteria like Paramecium cells [25].

The flow of text is as the following: We will first introduce a minimal model, with only two beads inside. In the two-bead model, we provide the theoretical analysis of the dynamical system using a perturbation method, yielding expressions for net transportation, work, and efficiency. We then numerically analyze the case of many beads, indicating the positive cooperative effect via hydrodynamic interaction between the beads.

II The general setup

Refer to caption
Figure 1: The setup of spherical bead model. Here, dd is the distance between the equilibrium positions of neighboring beads; ll is the typical distance between the beads and the test particle.

As an analytically tractable model of a flow generator, a one-dimensional setup is established and illustrated in Fig. 1. Specifically, consider NN spherical beads that can move only along the xx-axis, obeying

γ[x˙iv(xi)]=Fi,\displaystyle\gamma\left[\dot{x}_{i}-v(x_{i})\right]=F_{i}, (1)

where γ=6πμa\gamma=6\pi\mu a is the drag coefficient for the fluid viscosity μ\mu, aa is the radius of the beads, xix_{i} (i=1,2,,N)i=1,2,\ldots,N) is the position of bead ii, v(xi)v(x_{i}) is the flow field at xix_{i} generated by the beads jij\neq i, and FiF_{i} is the active force applied to bead ii. The flow field is given by

v(xi)jiHijFj,\displaystyle v(x_{i})\coloneqq\sum_{j\neq i}H_{ij}F_{j}, (2)

where HijH_{ij} (1i,jN)(1\leq i,j\leq N) is the Oseen tensor for the Stokeslet in incompressible Newtonian fluid [26]. Because only one-dimensional motion in the xx-direction is considered, the Oseen tensor is given as

Hij=1γ3a2|xij|+O[(ad)3],\displaystyle H_{ij}=\frac{1}{\gamma}\frac{3a}{2|x_{ij}|}+O\left[\left(\frac{a}{d}\right)^{3}\right], (3)

where xij=xixjx_{ij}=x_{i}-x_{j} and dd is the distance between the equilibrium positions of the neighboring beads. Hereafter, all O[(ad)3]O\left[\left(\frac{a}{d}\right)^{3}\right] terms are neglected. Also consider a test particle of radius aa, obeying

γ[x˙0v(x0)]=0,\displaystyle\gamma\left[\dot{x}_{0}-v(x_{0})\right]=0, (4)

where

v(x0)j=1NH0jFj,\displaystyle v(x_{0})\coloneqq\sum_{j=1}^{N}H_{0j}F_{j}, (5)

v(x0)v(x_{0}) is the velocity profile of the test particle. Denote the typical distance between the flow generator and the test particle by ll. Here, we assume ldl\gg d and employ the following approximation throughout this study:

H0j=1γ3a2l.\displaystyle H_{0j}=\frac{1}{\gamma}\frac{3a}{2l}. (6)

With this approximation, ll only affects the magnitude of displacement of x0x_{0} and can be chosen arbitrarily. Active force FiF_{i} is modeled as follows. Assume that each bead is connected to a pinned point by an elastic beam, which exerts force by periodically changing its natural length. Specifically, consider

Fi=k[xi+L(ϕi)xi],\displaystyle F_{i}=k\left[x_{i}^{*}+L(\phi_{i})-x_{i}\right], (7)
L(ϕi)=ϵL0sinϕi,\displaystyle L(\phi_{i})=\epsilon L_{0}\sin{\phi_{i}}, (8)
ϕi=ωt+ψi\displaystyle\phi_{i}=\omega t+\psi_{i} (9)

where xi+L(ϕi)x_{i}^{*}+L(\phi_{i}) is the equilibrium position, L(ϕi)L(\phi_{i}) is the change of the natural length, ϕi\phi_{i} is the phase of beating, kk is the spring constant, ψi\psi_{i} is the phase offset, and ϵL0\epsilon L_{0} is the oscillation amplitude of the natural length, ϵ\epsilon is a nondimensional quantity introduced for later convenience. Without loss of generality, set xi=(i1)dx_{i}^{*}=(i-1)d and ψ1=0\psi_{1}=0. One can interpret that beams repeat contraction and expansion with period T=2πωT=\frac{2\pi}{\omega} with some phase differences between the neighbors. In the following numerical simulations, without specific mentions we fix numerical values of parameters as: a=0.1a=0.1, γ=1,l=1000,L0=1,ω=1\gamma=1,l=1000,L_{0}=1,\omega=1 and vary N,d,ϵN,d,\epsilon and ψi\psi_{i} (i=2,,N)(i=2,\ldots,N). Typical behavior for N=4N=4 is displayed in Fig. 2.

To quantify the system performance, define the following efficiency for the transportation of the test particle:

η^γ<v0>2P=γR2WT,\displaystyle\hat{\eta}\coloneqq\frac{\gamma\big{<}v_{0}\big{>}^{2}}{P}=\frac{\gamma R^{2}}{WT}, (10)

where <>\big{<}\cdot\big{>} denotes the average over one cycle, PP and WW are the total power and work exerted by the flow generator for one cycle, respectively, and RR is the net transportation of the test particle for one period. More precisely, define

RlimnnT(n+1)Tx˙0𝑑t=limnnT(n+1)Tv(x0)𝑑t=limn3a2γlnT(n+1)Tj=1NFjdt,\displaystyle R\coloneqq\lim_{n\to\infty}\int_{nT}^{(n+1)T}\dot{x}_{0}\ dt=\lim_{n\to\infty}\int_{nT}^{(n+1)T}v(x_{0})\ dt=\lim_{n\to\infty}\frac{3a}{2\gamma l}\int_{nT}^{(n+1)T}\sum_{j=1}^{N}F_{j}\ dt, (11)

where nn is the number of cycles and consider a large nn limit to eliminate the transient behavior. Also define

Wi=1NWi,\displaystyle W\coloneqq\sum_{i=1}^{N}W_{i}, (12)

where

WilimnnT(n+1)T(x˙iv(xi))Fi𝑑t=limn1γnT(n+1)TFi2𝑑t.\displaystyle W_{i}\coloneqq\lim_{n\to\infty}\int_{nT}^{(n+1)T}\big{(}\dot{x}_{i}-v(x_{i})\big{)}F_{i}\ dt=\lim_{n\to\infty}\frac{1}{\gamma}\int_{nT}^{(n+1)T}F_{i}^{2}\ dt. (13)

One may evaluate RR, WW, and thus η^\hat{\eta} if the time-asymptotic behavior of xi(t)x_{i}(t) (i=1,,N)(i=1,\ldots,N) is obtained.

We are interested in the cooperative effect on the efficiency and thus later compare the efficiency for different NN values. Thus, it is convenient to introduce the per-unit efficiency:

η=η^N=γR2WTN.\displaystyle\eta=\frac{\hat{\eta}}{N}=\frac{\gamma R^{2}}{WTN}. (14)

A positive cooperative effect is indicated if η\eta significantly increases with NN.

A similar kind of efficiency could be found, such as the Lighthill hydrodynamic efficiency (cf. Ref. [27]) which happens to be one of the most popular among literatures (for instances, in Ref. [28, 29]). There, the particle is approximately spherical and deformable in order to move by morphing and the expression is

η^γ<v0>2<P>\displaystyle\hat{\eta}^{\prime}\coloneqq\frac{\gamma\big{<}v_{0}\big{>}^{2}}{\big{<}P\big{>}} (15)

where v0v_{0} is the velocity of the particle and PP is the work done from morphing. This is fundamentally the same definition as ours if one replaces the work done from morphing to the work done by beads.

Refer to caption
Figure 2: Typical dynamical behavior of the system for N=4,ψi=1.0(i1),d=1N=4,\psi_{i}=1.0(i-1),d=1 and ϵ=0.1\epsilon=0.1. The displacements of the beads, xixix_{i}-x_{i}^{*} (i=1,2,3,4i=1,2,3,4), are plotted together with that of the test particle, 103x010^{3}x_{0} (instead of x0x_{0} for visibility). The amplitudes of beads are different because of the effect of hydrodynamic coupling. The slope of the envelope of x0x_{0} is approximately R/TR/T.

III The minimal model: a 2-bead case

Here, by considering the minimal model, the flow generator consisting of only two beads (N=2)(N=2), and perturbatively solving such system, we derive the expressions for R,WR,W, and η^\hat{\eta}. For simplicity, ψ2\psi_{2} is denoted as ψ\psi in this section; thus, ϕ1=ωt\phi_{1}=\omega t and ϕ2=ωt+ψ\phi_{2}=\omega t+\psi. Then, our model for N=2N=2 is

x˙1=3a2γ|x2x1|F2+1γF1,\displaystyle\dot{x}_{1}=\frac{3a}{2\gamma|x_{2}-x_{1}|}F_{2}+\frac{1}{\gamma}F_{1}, (16a)
x˙2=3a2γ|x2x1|F1+1γF2.\displaystyle\dot{x}_{2}=\frac{3a}{2\gamma|x_{2}-x_{1}|}F_{1}+\frac{1}{\gamma}F_{2}. (16b)

The perturbation method might be applied by treating ϵ\epsilon as a small parameter. Firstly introduce the dimensionless version of canonical basis as

X:=x1+x2d,\displaystyle X:=\frac{x_{1}+x_{2}}{d}, (17)
Y:=x2x1d.\displaystyle Y:=\frac{x_{2}-x_{1}}{d}. (18)

For simplicity, always assume Y>0Y>0, which is a reasonable assumption physically, meaning that the beads never overlap with each other, so no collision occurs. Then, Eq. (16) becomes

X˙\displaystyle\dot{X} =kγ(3a2dY+1)[1+ϵL^0(sinϕ1+sinϕ2)X],\displaystyle=\frac{k}{\gamma}\left(\frac{3a}{2dY}+1\right)\left[1+\epsilon\hat{L}_{0}(\sin{\phi_{1}}+\sin{\phi_{2}})-X\right], (19a)
Y˙\displaystyle\dot{Y} =kγ(3a2dY+1)[1+ϵL^0(sinϕ2sinϕ1)Y],\displaystyle=\frac{k}{\gamma}\left(-\frac{3a}{2dY}+1\right)\left[1+\epsilon\hat{L}_{0}(\sin{\phi_{2}}-\sin{\phi_{1}})-Y\right], (19b)

where L^0:=L0d\hat{L}_{0}:=\frac{L_{0}}{d}. Now, solve this using the perturbative forms:

X(t)\displaystyle X(t) =1+ϵX1(t)+ϵ2X2(t)+O(ϵ3),\displaystyle=1+\epsilon X_{1}(t)+\epsilon^{2}X_{2}(t)+O(\epsilon^{3}), (20)
Y(t)\displaystyle Y(t) =1+ϵY1(t)+ϵ2Y2(t)+O(ϵ3).\displaystyle=1+\epsilon Y_{1}(t)+\epsilon^{2}Y_{2}(t)+O(\epsilon^{3}). (21)

Note

1Y=1ϵY1+ϵ2(Y2+Y12)+O(ϵ3).\displaystyle\frac{1}{Y}=1-\epsilon Y_{1}+\epsilon^{2}(-Y_{2}+Y_{1}^{2})+O(\epsilon^{3}). (22)

Therefore, by collecting O(ϵ)O(\epsilon) in Eq. (19),

X˙1=\displaystyle\dot{X}_{1}={} α[m(t)X1],\displaystyle\alpha\left[m(t)-X_{1}\right], (23a)
Y˙1=\displaystyle\dot{Y}_{1}={} β[h(t)Y1],\displaystyle\beta\left[h(t)-Y_{1}\right], (23b)

where α:=kγ(3a2d+1)\alpha:=\frac{k}{\gamma}(\frac{3a}{2d}+1), β:=kγ(3a2d+1)\beta:=\frac{k}{\gamma}(-\frac{3a}{2d}+1), m(t):=sinϕ1+sinϕ2m(t):=\sin{\phi_{1}}+\sin{\phi_{2}}, and h(t):=sinϕ2sinϕ1h(t):=\sin{\phi_{2}}-\sin{\phi_{1}}. Similarly, for O(ϵ2)O(\epsilon^{2}),

X˙2\displaystyle\dot{X}_{2} =3akY12γd[m(t)X1]αX2,\displaystyle=-\frac{3akY_{1}}{2\gamma d}\left[m(t)-X_{1}\right]-\alpha X_{2}, (24a)
Y˙2\displaystyle\dot{Y}_{2} =3akY12γd[h(t)Y1]βY2.\displaystyle=\frac{3akY_{1}}{2\gamma d}\left[h(t)-Y_{1}\right]-\beta Y_{2}. (24b)

Solving these equations, the time-asymptotic expressions are obtained as

X1=\displaystyle{X}_{1}= 2αcos(ψ2)[αsin(ωt+ψ2)ωcos(ωt+ψ2)]α2+ω2,\displaystyle\frac{2\alpha\cos\left(\frac{\psi}{2}\right)\left[\alpha\sin\left(\omega t+\frac{\psi}{2}\right)-\omega\cos\left(\omega t+\frac{\psi}{2}\right)\right]}{\alpha^{2}+\omega^{2}}, (25a)
Y1=\displaystyle{Y}_{1}= 2βsin(ψ2)[βcos(ωt+ψ2)+ωsin(ωt+ψ2)]β2+ω2,\displaystyle\frac{2\beta\sin\left(\frac{\psi}{2}\right)\left[\beta\cos\left(\omega t+\frac{\psi}{2}\right)+\omega\sin\left(\omega t+\frac{\psi}{2}\right)\right]}{\beta^{2}+\omega^{2}}, (25b)
X2=\displaystyle{X}_{2}= 3aβkωsin(ψ)2αγd(α2+ω2)(α2+4ω2)(β2+ω2)\displaystyle-\frac{3a\beta k\omega\sin(\psi)}{2\alpha\gamma d\left(\alpha^{2}+\omega^{2}\right)\left(\alpha^{2}+4\omega^{2}\right)\left(\beta^{2}+\omega^{2}\right)}
[(α2+4ω2)(αβ+ω2)+αω(α2+3αβ2ω2)sin(2ωt+ψ)+α(α2β3αω22βω2)cos(2ωt+ψ)],\displaystyle\left[\left(\alpha^{2}+4\omega^{2}\right)\left(\alpha\beta+\omega^{2}\right)+\alpha\omega\left(\alpha^{2}+3\alpha\beta-2\omega^{2}\right)\sin(2\omega t+\psi)+\alpha\left(\alpha^{2}\beta-3\alpha\omega^{2}-2\beta\omega^{2}\right)\cos(2\omega t+\psi)\right], (25c)
Y2=\displaystyle{Y}_{2}= 3aβkωsin2(ψ2)[(2ω34β2ω)cos(2ωt+ψ)+β(β25ω2)sin(2ωt+ψ)]γd(β2+ω2)2(β2+4ω2).\displaystyle-\frac{3a\beta k\omega\sin^{2}\left(\frac{\psi}{2}\right)\left[\left(2\omega^{3}-4\beta^{2}\omega\right)\cos(2\omega t+\psi)+\beta\left(\beta^{2}-5\omega^{2}\right)\sin(2\omega t+\psi)\right]}{\gamma d\left(\beta^{2}+\omega^{2}\right)^{2}\left(\beta^{2}+4\omega^{2}\right)}. (25d)

With these expressions, one may now calculate RR and WW. Substituting Eq. (25) into Eq. (11),

R=9πa2k2sin(ψ)β(αβ+ω2)2lγ2α(α2+ω2)(β2+ω2)ϵ2[1+O(ϵ)]\displaystyle R=\frac{9\pi a^{2}k^{2}\sin(\psi)\beta\left(\alpha\beta+\omega^{2}\right)}{2l\gamma^{2}\alpha\left(\alpha^{2}+\omega^{2}\right)\left(\beta^{2}+\omega^{2}\right)}\epsilon^{2}\left[1+O(\epsilon)\right] (26)

which vanishes in the first order of ϵ\epsilon while generally not in the second order of ϵ\epsilon (cf. Eq. (10) and Eq. (25)). Substituting Eq. (25) into Eq. (12) and using F12+F22=(F1+F2)2+(F1F2)22F_{1}^{2}+F_{2}^{2}=\frac{(F_{1}+F_{2})^{2}+(F_{1}-F_{2})^{2}}{2},

W=\displaystyle W= πk2ωd2[(β2α2)cos(ψ)+α2+β2+2ω2]γ(α2+ω2)(β2+ω2)ϵ2[1+O(ϵ)]\displaystyle\frac{\pi k^{2}\omega d^{2}\left[\left(\beta^{2}-\alpha^{2}\right)\cos(\psi)+\alpha^{2}+\beta^{2}+2\omega^{2}\right]}{\gamma\left(\alpha^{2}+\omega^{2}\right)\left(\beta^{2}+\omega^{2}\right)}\epsilon^{2}\left[1+O(\epsilon)\right] (27)

which implies similar minimal energy dissipation versus phase difference as in Ref. [20]. Therefore,

η\displaystyle\eta =81a4β2k2sin2(ψ)(αβ+ω2)216γ2α2d2l2(α2+ω2)(β2+ω2)[(β2α2)cos(ψ)+α2+β2+2ω2]ϵ2[1+O(ϵ)].\displaystyle=\frac{81a^{4}\beta^{2}k^{2}\sin^{2}(\psi)\left(\alpha\beta+\omega^{2}\right)^{2}}{16\gamma^{2}\alpha^{2}d^{2}l^{2}\left(\alpha^{2}+\omega^{2}\right)\left(\beta^{2}+\omega^{2}\right)\left[\left(\beta^{2}-\alpha^{2}\right)\cos(\psi)+\alpha^{2}+\beta^{2}+2\omega^{2}\right]}\epsilon^{2}\left[1+O(\epsilon)\right]. (28)

It should be noted that all quantities start from O(ϵ2)O(\epsilon^{2}) because the contributions of first-order terms are averaged out over one cycle. As shown in Fig. 3, these expressions are in excellent agreement with the simulation results.

Furthermore, by recalling that ad\frac{a}{d} is assumed to be small and using α=β=kγ+O(ad)\alpha=\beta=\frac{k}{\gamma}+O(\frac{a}{d}), the expressions can be much simplified as

R\displaystyle R =9πa2L02k2sin(ψ)2ld2(k2+γ2ω2)ϵ2[1+O(ϵ,ad)],\displaystyle=\frac{9\pi a^{2}L_{0}^{2}k^{2}\sin(\psi)}{2ld^{2}(k^{2}+\gamma^{2}\omega^{2})}\epsilon^{2}\left[1+O\left(\epsilon,\frac{a}{d}\right)\right], (29a)
W\displaystyle W =2πL02k2ωγ(k2+γ2ω2)ϵ2[1+O(ϵ,ad)],\displaystyle=\frac{2\pi L_{0}^{2}k^{2}\omega\gamma}{\left(k^{2}+\gamma^{2}\omega^{2}\right)}\epsilon^{2}\left[1+O\left(\epsilon,\frac{a}{d}\right)\right], (29b)
η\displaystyle\eta =81a4L02k2sin2(ψ)32l2d4(k2+γ2ω2)ϵ2[1+O(ϵ,ad)].\displaystyle=\frac{81a^{4}L_{0}^{2}k^{2}\sin^{2}(\psi)}{32l^{2}d^{4}\left(k^{2}+\gamma^{2}\omega^{2}\right)}\epsilon^{2}\left[1+O\left(\epsilon,\frac{a}{d}\right)\right]. (29c)

From these expressions, observe that RR decreases with increasing dd, proportionally to 1/d21/d^{2}. Thus, RR vanishes at a large dd limit, indicating the essential role of hydrodynamic interaction on the generation of the net flow. In contrast, WW is almost independent of dd and the leading term is just the sum of the works of two independent beads; the hydrodynamic interaction gives little contribution to the work for dad\gg a. Therefore, η\eta is approximately proportional to R2R^{2} and its maxima approximately coincide with the maxima of RR.

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Figure 3: The net transportation RR and the work WW over one cycle as well as the efficiency η\eta with respect to the phase difference ψ\psi in the two-bead case (N=2)(N=2). Solid curves are the theoretical ones given in Eq. (26)–(28) while blue dots are the simulation results of Eq. (1) and Eq. (4). Parameter values: d=50d=50, l=1000l=1000, and ϵ=0.1\epsilon=0.1.

IV Multiple bead case

In this section, a more general setup is considered, where the number of bead NN is no longer restricted by two. In the simulation, we set ψi=iΔψ\psi_{i}=i\Delta\psi, where Δψ\Delta\psi is a constant describing the phase difference. In this setup, one only needs to consider 0Δψπ0\leq\Delta\psi\leq\pi because of the symmetry of the system. Such a pattern mimics the metachronal wave ubiquitously found in the collective motion of flagella or cilia (cf. Ref. [30]). For N=3N=3, as shown in Fig. 4, this setup is numerically proven to approximately produce the maximum efficiency output for the cases of N=3N=3. The figure represents the efficiency as a function of ψ2\psi_{2} and ψ3\psi_{3}, in which the optimality is found at (ψ2,ψ3)(1.3,2.6)(\psi_{2},\psi_{3})\approx(1.3,2.6), thus ψ32ψ2\psi_{3}\approx 2\psi_{2}.

We first observe the dependence of per-unit efficiency η\eta on Δψ\Delta\psi, shown in Fig. 5(a). It is seen that the optimal phase difference, denoted as Δψ\Delta\psi^{*}, decreases as NN increases. In Fig. 5(b), we further plot the dependence of Δψ\Delta\psi^{*} on the bead number NN, suggesting that Δψ\Delta\psi^{*} approaches a certain value as NN increases. There, we test two different dd values and find that the dependence on dd is rather weak.

We then observe the NN-dependencies of R,WR,W and η\eta values for Δψ=Δψ\Delta\psi=\Delta\psi^{*}, denoted as R,WR^{*},W^{*}, and η\eta^{*}, respectively. We plot these values in Fig. 6, where the vertical axes are scaled as Rd2ϵ2,W1ϵ2R^{*}\frac{d^{2}}{\epsilon^{2}},W^{*}\frac{1}{\epsilon^{2}}, and ηd4ϵ2\eta^{*}\frac{d^{4}}{\epsilon^{2}}. This scaling is motivated from the theoretical predicted dependence on dd and ϵ\epsilon for N=2N=2, given in Eq. (29); i.e., Rϵ2d2,Wϵ2R\propto\frac{\epsilon^{2}}{d^{2}},W\propto\epsilon^{2}, and ηϵ2d4\eta\propto\frac{\epsilon^{2}}{d^{4}}. Figure 6(a) indicates that RR increases approximately linearly with NN, particularly for large dd. Moreover, as shown in Fig. 6(b), WW^{*} increases virtually linearly with NN, indicating that the work was approximately equal to the summation of independent beads. Assuming R,WNR,W\propto N, η=R2WN\eta=\frac{R^{2}}{WN} should be independent of NN; however, as shown in Fig. 6(c), η\eta is actually strongly dependent on NN, indicating that the growth of RR significantly deviates from a linear growth. Importantly, η\eta for N>2N>2 is larger than η\eta for N=2N=2, indicating the positive cooperative effect of hydrodynamic coupling. It should also be noted that η\eta saturates or even turns to decrease for large NN, which could come from our simple setting for the phase offsets and can possibly be improved by considering a more complex pattern of ψi\psi_{i}. It is also observed that all the quantities at given NN in Fig. 6 have similar magnitudes, suggesting that the dependence Rϵ2d2,Wϵ2R\propto\frac{\epsilon^{2}}{d^{2}},W\propto\epsilon^{2}, and ηϵ2d4\eta\propto\frac{\epsilon^{2}}{d^{4}} roughly holds true for N3N\geq 3.

Refer to caption
Figure 4: Efficiency η\eta of the three-bead system as a function of phase offsets ψ2\psi_{2} and ψ3\psi_{3} for N=3N=3. Parameter values are the same as those in Fig. 3.
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Figure 5: (a) Per-unit efficiency η\eta versus phase difference Δψ\Delta\psi in the NN-beads cases. (b) Optimal phase difference

Δψ\Delta\psi^{*} versus NN.

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Figure 6: Net transportation RR^{*}, work WW^{*}, and per-unit efficiency η\eta^{*} for optimal phase difference Δψ\Delta\psi^{*} as functions of NN.

V Conclusion

We introduced a simple one-dimensional coupled sphere motor model, with the generated flow and transportation efficiency investigated both theoretically and numerically. For the minimal case with two beads, the proper theoretical expression for both the net transportation and the efficiency are derived by the perturbation method, and it is proven that these results are in excellent agreement with the numerical results. Furthermore, we numerically investigated the case of N3N\geq 3 and found that the efficiency increases with NN.

For a more practical usage, the effect of a wall, to which the system is pinned, should also be examined; such a setup can be treated by using the Blake tensor [31, 17] instead of the Oseen tensor. It could be very helpful to derive theoretical expressions for the net transportation and efficiency for this case. In our model, oscillators were designed non-autonomous for simplicity; to understand the role of synchronization and self-organized metachronal wave pattern, it is essential to extend the model to the case of autonomous oscillators and compose a theoretical framework. Such an effort would substantially contribute to deepening the understanding of the hydrodynamic effect of interactive objects in low Reynolds numbers. Moreover, it is worth discovering whether the higher order interactions will eventually destroy the positive coupling effect completely for very large number of oscillators, and if this is also true with effect of a wall. In addition, a two-dimensional movement model could be considered, as many other publications have focused, while the complexity in finding a theoretical expression could be fairly challenging.

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