This paper was converted on www.awesomepapers.org from LaTeX by an anonymous user.
Want to know more? Visit the Converter page.

Exact polarization energy for clusters of contacting dielectrics

Huada Lian Department of Materials Science & Engineering, Stanford University Jian Qin Department of Chemical Engineering, Stanford University Corresponding author: [email protected]
Abstract

The induced surface charges appear to diverge when dielectric particles form close contacts. Resolving this singularity numerically is prohibitively expensive because high spatial resolution is needed. We show that the strength of this singularity is logarithmic in both inter-particle separation and dielectric permittivity. A regularization scheme is proposed to isolate this singularity, and to calculate the exact cohesive energy for clusters of contacting dielectric particles. The results indicate that polarization energy stabilizes clusters of open configurations when permittivity is high, in agreement with the behavior of conducting particles, but stabilizes the compact configurations when permittivity is low.

For particle aggregates or clusters stabilized by electrostatic interactions,1, 2, 3 the cohesive energy depends on the dielectric permittivities of both the particles and the medium. Permittivity quantifies the density of dipoles induced by externally applied electric fields, which is proportional to polarization in the linear regime. When the permittivity contrast between the particles and the medium is high, as is often the case, the polarizations from the two sides of the interface do not fully compensate each other, resulting in the accumulation of induced surface charges.

Resolving the surface charges is needed to evaluating the electrostatic interactions among particles in close proximity, and is challenging because polarization is intrinsically a many-body effect, depending on the positions of all particles. For instance, careful measurements in colloidal suspensions have shown that the inter-particle force is non-additive, which is at least partially due to the polarization effect.4 In another set of experiments on metallic nanoparticles, it has been found that the aggregation of multiple particles surrounding a charged particle can be stabilized by the polarization effect alone.3, 5 More dramatic demonstration of such polarization effects is found in the so-called like-charge attraction caused by the strong polarization effect, for particles of large size or permittivity ratios.6, 7

Computational methods, such as the boundary element method,8 the spectral methods 9, 10 and the image method,11 have been developed to account for this polarization effect. In practice, these methods all need to evaluate the induced surface charge densities in one form or another, and have been successfully applied to study a wide range of problems involving the aggregation of polarizable particles.12, 13, 14 However, when particles are in close proximity, the surface charge densities apparently diverge because the electric field in the narrow gap region is strong even for a small difference in the electrostatic potentials of particles. This is analogous to the divergent lubrication force between approaching solid particles in the Stokesian regime.15 Resolving these apparently diverging charge densities requires a high spatial resolution that becomes computationally prohibitive for nearly touching particles.8 For conductors like metalic particles, the functional form of the divergent charge density has been identified and used to isolate the singularity obscuring numerical calculations, and to obtain the exact energy and force for contacting particles.5 For dielectric particles, the question remains unsolved.

Refer to caption
Figure 1: Surface charges between two particles separated by a distance hh. The separation of two surfaces at a radial distance rr from the contact points can be approximated by h+r2/ah+r^{2}/a, where a2/(a11+a21)a\equiv 2/(a_{1}^{-1}+a_{2}^{-1}). The permittivity of the medium is ϵout\epsilon_{\rm out}. Surface of conducting particles are equipotential with potential set to VV and 0. Surfaces of dielectric particles, with permittivities ϵ1\epsilon_{1} and ϵ2\epsilon_{2}, have surface potential distributions ϕ1(r)\phi_{1}(r) and ϕ2(r)\phi_{2}(r), respectively.

One way to reveal these singular surface charges is to consider two conducting particles separated by a small gap, as sketched in Fig. 1. The points on the two surfaces separated by the minimum distance, or gap distance hh, are referred to as contact points. The surface charge density is proportional to the strength of the normal component of electric field on surfaces, according to Gauss’s law. When hh is small, the electric field lines in the gap region are nearly parallel to the line connecting the two contact points. The strength of the electrical field is, in turn, proportional to the difference in the surface electrical potentials. This relation between the surface potential and the electrical field is analogous to that between the longitudinal velocities of converging particles and the transverse velocity of squzzed fluid velocity in the lubrication theory.15

To calculate the surface charge density, both the surface potentials and the vertical separations are needed. Since conductors are equipotential, the surface potentials can be set to VV and 0 respectively. The vertical separation depends on the radial distance rr, and can be expressed within the Derjaguin approximation as h+r2/ah+r^{2}/a, where aa is the harmonic average of radii of curvature a1a_{1} and a2a_{2} at the two contact points, i.e., a1=(a11+a21)/2a^{-1}=(a_{1}^{-1}+a_{2}^{-1})/2. Here, the spherical apexes are assumed for simplicity, but more general curvatures can be treated similarly. Consequently, the field strength at radius rr is E(r)=V/(h+r2/a)E(r)=V/(h+r^{2}/a), and the surface charge density σ(r)=14πϵoutV/(h+r2/a)\sigma(r)=\frac{1}{4\pi}\epsilon_{\rm out}V/(h+r^{2}/a) on the top surface, where ϵout\epsilon_{\rm out} is the medium permittivity. Integrating σ(r)\sigma(r) for rr from 0 to R0R_{0}, where R0R_{0} is a cutoff of order aa, results in the singular part of the surface charge

Qs\displaystyle Q_{\rm s} =Vϵout4π0R0dr2πrh+r2/aVϵouta4ln(ah).\displaystyle=\frac{V\epsilon_{\rm out}}{4\pi}\int_{0}^{R_{0}}\!{\rm d}r\frac{2\pi r}{h+r^{2}/a}\simeq\frac{V\epsilon_{\rm out}a}{4}\ln\left(\frac{a}{h}\right). (1)

The unity in the logarithmic term is dropped because R0ahR_{0}\simeq a\gg h. Further, the difference between R0R_{0} and aa is neglected because it only leads to a constant shift. Equation (1) shows how surface charges of the upper surface become singular as the gap distance decreases. That of the lower surface is also singular, but of opposite sign. In the limit h0h\to 0, the energy does not blow up because the potential difference VV vanishes once particles form contact.

The ratio of the singular charge QsQ_{\rm s} and the potential difference VV gives the singular part of the capacitance cs=ϵoutaln(a/h)/4c_{\rm s}=\epsilon_{\rm out}a\ln(a/h)/4, which has been found previous for spherical dimers.6, 7 The above analysis shows that this singular capacitance is local. Thus, the same singularity applies to non-spherical particles, and for aggregates of multiple particles. This fact has been employed to find the exact energy for clusters of contacting, conducting particles.5 In this work, the full capacitance array is first numerically calculated for an ensemble of conducting particles at finite but small separations. The singular contribution is then subtracted, leaving a regular part that can be extrapolated to h=0h=0. Finally, when the singular and regular parts are pieced together, the variation of energy with separation is obtained.

For the dielectric case, a straightforward generalization of the above treatment fails, because the particles are not equipotential. The potential difference ΔV(r)\Delta V(r) needed to evaluate the charge density in eq. (1) can not be fully specified by the potential difference between the contact points ΔV(0)\Delta V(0). The variation of ΔV(r)\Delta V(r) with rr in the gap region is expected to be quadratic, but the curvature is unknown a priori. In an early, and analogous work on thermal conduction of composite materials, Batchelor et al.16 noticed that the potential distribution, which determines the surface charges, is itself dominated by the contribution from the surface charges nearby, so that a self-consistent treatment is needed.

To illustrate this point, we consider the dielectric case in Fig. 1. Let the surface potentials of the two particles be ϕ1(r)\phi_{1}(r) and ϕ2(r)\phi_{2}(r), and the surface charges be σ1(r)\sigma_{1}(r) and σ2(r)\sigma_{2}(r). The surface potential ϕi(r)\phi_{i}(r), with i=1,2i=1,2, can be calculated by integrating the coulombic potential of the respective surface charges. Near the contact point, we have

ϕi(r)=Vi~+12πϵi0dr02πdθrσi(r)r2+r22rrcosθ.\phi_{i}(r)=\tilde{V_{i}}+\frac{1}{2\pi\epsilon_{i}}\int_{0}^{\infty}\!\!{\rm d}r^{\prime}\!\!\int_{0}^{2\pi}\!\!{\rm d}\theta^{\prime}\frac{r^{\prime}\sigma_{i}(r^{\prime})}{\sqrt{r^{2}+r^{\prime 2}-2rr^{\prime}\cos\theta^{\prime}}}. (2)

Here, V~i\tilde{V}_{i} are the contributions to the surface potential from the surface charge outside the contact region. The integral are those from the surface charges in the contact region. The prefactor is 12π\frac{1}{2\pi} (instead of 14π\frac{1}{4\pi}) because of the well-known jump condition for surface potentials.17 The distance at denominator is approximated using that for the flat surface, which leads to negligible error because only the contact region is of concern. The upper bound is set to infinity for convenience; as we shall see below, the singular surface charge density dies off rapidly outside the contact region.

The surface charge density σi(r)\sigma_{i}(r) in eq. (2) are related to the potential difference, ΔV(r)ϕ1(r)ϕ2(r)\Delta V(r)\equiv\phi_{1}(r)-\phi_{2}(r). By analogy to the conductor case, the electric field is approximately vertical and its magnitude is ΔV(r)/(h+r2/a)\Delta V(r)/(h+r^{2}/a). Then applying Gauss’s law, we get the charge density on the top surface

σ1(r)=ϵout(1ϵr,11)ΔV(r)h+r2/a,\sigma_{1}(r)=\epsilon_{\rm out}\left(1-\epsilon_{{\rm r},1}^{-1}\right)\frac{\Delta V(r)}{h+r^{2}/a}, (3)

where ϵr,1ϵ1/ϵout\epsilon_{{\rm r},1}\equiv\epsilon_{1}/\epsilon_{\rm out}. The charge density σ2\sigma_{2} is given similarly, but with a negative sign. Substituting the charge densities to eq. (2) and taking the difference gives an integral equation for ΔV(r)\Delta V(r). The dependence on the unknown, V~1V~2\tilde{V}_{1}-\tilde{V}_{2}, can be factored out by introducing an auxiliary, f(r)1ΔV(r)/(V~1V~2)f(r)\equiv 1-\Delta V(r)/(\tilde{V}_{1}-\tilde{V}_{2}), which satisfies

f(r)=ϵr,11+ϵr,212π0dr1f(r)h+r2/a4rr+rK(x).f(r)=\frac{\epsilon_{{\rm r},1}^{-1}+\epsilon_{{\rm r},2}^{-1}}{2\pi}\int_{0}^{\infty}\!\!{\rm d}r^{\prime}\ \frac{1-f(r^{\prime})}{h+r^{\prime 2}/a}\frac{4r^{\prime}}{r+r^{\prime}}K(x). (4)

Here the integral over the azimuthal angle has been replaced with the complete elliptic function of the first kind K(x)K(x), where x4rr(r+r)2x\equiv\frac{4rr^{\prime}}{(r+r^{\prime})^{2}}. When ϵ1=ϵ2\epsilon_{1}=\epsilon_{2}, eq. (4) reduces to Batchelor’s original result, eq. (4.5) in ref.16. Since f(r)f(r) is proportional to the contribution from the surface charges in the contact region, we see that it is dominated by particles of lower permittivity. When both permittivities approach infinity, we have f(r)=0f(r)=0 and ΔV(r)=V~1V~2\Delta V(r)=\tilde{V}_{1}-\tilde{V}_{2}, which is identical to the expression for the conductors discussed above. More general cases are discussed below.

The solution to eq. (4) is uniquely determined by the normalized distance h/ah/a and the average permittivity, ϵr2/(ϵr,11+ϵr,21)\epsilon_{\rm r}\equiv 2/(\epsilon_{\rm r,1}^{-1}+\epsilon_{\rm r,2}^{-1}). As shown by Batchelor,16 eq. (4) can be non-dimensionalized to

f(ρ)=1π0dρ1f(ρ)λ+ρ24ρρ+ρK(x)f(\rho)=\frac{1}{\pi}\int_{0}^{\infty}\!{\rm d}\rho^{\prime}\,\frac{1-f(\rho^{\prime})}{\lambda+\rho^{\prime 2}}\frac{4\rho^{\prime}}{\rho+\rho^{\prime}}K(x) (5)

in which ρrϵr/a\rho\equiv r\epsilon_{\rm r}/a and λhϵr2/a\lambda\equiv h\epsilon_{\rm r}^{2}/a. The numerically solved f(ρ)f(\rho) for a few representative λ\lambda values are shown in Fig. 2a. For large gap distance, with λ1\lambda\gg 1, f(ρ)f(\rho) is nearly uniform, as expected. For smaller λ\lambda values, f(ρ)f(\rho) decreases from f(0)f(0) with rr monotonically. The difference in electric potential at the contact points is proportional to 1f(0)1-f(0). The value of f(0)f(0) increases as hh decreases, and reaches unity at h=0h=0, ensuring that the surface potential is continuous at the contact point. The variation of f(ρ)f(\rho) obtained from the above local analysis is confirmed by directly solving the full potential distribution for dielectric dimers (inset, Fig. 2a).

Similar to eq. (1) for the conductor case, the singular part of surface charges on particle 11 is given, with R0R_{0} being the regularizing cutoff of order aa, by

Qs,1=(V~1V~2)ϵout4π(1ϵr,11)0R0dr2πr[1f(r)]h+r2/aQ_{\rm s,1}=\frac{(\tilde{V}_{1}-\tilde{V}_{2})\epsilon_{\rm out}}{4\pi}\left(1-\epsilon_{{\rm r},1}^{-1}\right)\int_{0}^{R_{0}}\!\!{\rm d}r\frac{2\pi r\left[1-f(r)\right]}{h+r^{2}/a} (6)

The dependence on the dielectric permittivity appears in the prefactor 11/ϵr,11-1/\epsilon_{{\rm r},1} and in f(r)f(r). The singular surface charge Qs,2Q_{\rm s,2} on the particle 2 is given analogously, but with a negative sign. However, because of the dependence on the dielectric permittivity, Qs,2Q_{{\rm s},2} and Qs,1Q_{{\rm s},1} do not add up to zero. The first term in the square bracket gives the same ln(a/h)\ln(a/h) singular contributions as eq. (1). The second term represents the correction due to dielectric screening.

Refer to caption
Refer to caption
Figure 2: (a) Variation of surface potential f(ρ)f(\rho) along the radial direction for λ=0\lambda=0, 0.50.5, 1.01.0, 10.010.0 and 10001000. The inset shows the normalized potential difference for spherical dimer with a minimum separation h=0.1ah=0.1a and parameters (Qi,ϵi,ai)(Q_{i},\epsilon_{i},a_{i}): (1,100,1)(1,100,1) and (1,10,2)(-1,10,2). Dots are numerically solved by a spectral method in bispherical coordinate 10 and the solid line is proportional to 1f(r)1-f(r). (b) The singular capacitance c1c_{1} is presented as a function of normalized surface separation h/ah/a and relative permittivity ϵr\epsilon_{\rm r}.

The singular capacitance defined by c1(h)Qs,1/(V~1V~2)c_{1}(h)\equiv Q_{{\rm s},1}/(\tilde{V}_{1}-\tilde{V}_{2}) also has these two contributions. In the non-dimensionalized form, it reads

c1(h)\displaystyle c_{1}(h) =1ϵr,114aϵout(lnahP(λ)),\displaystyle=\frac{1-\epsilon_{{\rm r},1}^{-1}}{4}a\epsilon_{\rm out}\left(\ln\frac{a}{h}-P\left(\lambda\right)\right),\quad (7)
P(λ)\displaystyle P(\lambda) 0dρ2ρλ+ρ2f(ρ).\displaystyle\equiv\int_{0}^{\infty}\!{\rm d}\rho\,\frac{2\rho}{\lambda+\rho^{2}}f(\rho).

In the last term, the upper bound is set to infinity because f(ρ)f(\rho) decays rapidly (as lnρ/ρ\ln\rho/\rho, ref.16). The dielectric correction is contained in the term P(λ)P(\lambda), which depends on permittivity ϵr\epsilon_{\rm r} and relative gap distance h/ah/a through the combination λ=hϵr2/a\lambda=h\epsilon_{\rm r}^{2}/a. The behavior of P(λ)P(\lambda) is derived from that of f(ρ)f(\rho). For λ1\lambda\gg 1, P(λ)P(\lambda) is vanishingly small, so the capacitance is dominated by ln(a/h)\ln(a/h), the characteristic behavior of conductors. On the other hand, when λ0\lambda\to 0, the leading contribution to P(λ)P(\lambda) is lnλ-\ln\lambda, which cancels exactly the ln(a/h)\ln(a/h) dependence, leaving a term 2lnϵr2\ln\epsilon_{\rm r} that diverges instead with the average permittivity. Further, we note that c1(h)c_{1}(h) approaches the conductor limit for ϵr1\epsilon_{\rm r}\gg 1.

The difference in contact charges between dielectric and conductor cases is solely contained in P(λ)P(\lambda). For intermediate separation, c1(h)c_{1}(h) shows a singular ln(a/h)\ln(a/h) dependence that is similar to the conductor behavior. However, as long as ϵr\epsilon_{\rm r} is finite, this logarithmic behavior will eventually be cut off by contribution from P(λ)P(\lambda) at sufficiently small separation. Therefore, unlike the conductor case, the contact capacitance for dielectrics is finite at h=0h=0. Instead, it approaches a constant proportional to 2lnϵr2\ln\epsilon_{\rm r}. Physically, the logarithmic hh-dependence originates from the accumulated polarization charges at the interface. It is cut off for dielectrics because the potential difference, which gives rise to the polarization charge, is self-consistently determined by the latter. The weaker polarization effect for dielectrics eventually can not keep up with the needed potential difference for producing the polarization charge. The variation of c1c_{1} on hh and ϵr\epsilon_{\rm r} are shown in Fig. 2b. The crossover can be estimated by setting λ=hϵr2/a=1\lambda=h\epsilon_{\rm r}^{2}/a=1. The logarithmic divergence, although being cut at small gap separation, still plagues numerical calculations in practice.18

This type of crossover behavior has been confirmed in a study on dielectric spherical dimers using the image method.19 The limiting value of the capacitance 2lnϵr2\ln\epsilon_{\rm r} as well as the crossover is also consistent with the analytically known result between a conducting sphere and a dielectric plane.20 However, unlike these two work on dimer particles, Batchelor’s result is strictly local, suggesting that the same type of singularity as represented by eq. (7) is applicable to all contact region in cluster of multiple dielectric particles, irrespective of the particle shape. In the following, we show that, the approach for isolating the singularity for contact between conductors can be generalized to treat the dielectric clusters, yielding the exact contact energy and distance-dependence with modest numerical cost.

We consider the cluster consisting of nn dielectric spheres. Given the free charge distribution ρ(𝐫)f\rho\lower 3.0pt\hbox{${}_{\rm f}$}({\bf r}), the potential ϕ\phi is governed by Poisson’s equation ϵ(𝐫)ϕ=ρ(𝐫)f/ϵout\nabla\cdot\epsilon({\bf r})\nabla\phi=-{\rho\lower 3.0pt\hbox{${}_{\rm f}$}({\bf r})}/{\epsilon_{\rm out}}, where ϵout\epsilon_{\rm out} is the medium permittivity. The (relative) material permittivity ϵ(𝐫)\epsilon({\bf r}) is set to ϵrϵin/ϵout\epsilon_{\rm r}\equiv\epsilon_{\rm in}/\epsilon_{\rm out} inside particles and unity in the medium. Although the general charge distribution poses no added difficulty, for simplicity, we focus on the case when only the free surface charge σf\sigma_{\rm f} are present. In such case, the system energy can be written as surface integrals of the product of the free surface charge and the surface potential over all surfaces. Furthermore, when the surface charge distribution is uniform, the energy reduces to the sum of the product of the total charge and the average surface potential. Therefore, we denote the set of net charges on particles by 𝐐{{\bf Q}}, and the mean surface potentials 𝐕{{\bf V}}. The net charges and the mean potentials are linearly related, i.e.,

𝐐=𝐂𝐕,{\bf Q}={\bf C}{\bf V}, (8)

where 𝐂{\bf C} is an n×nn{\times}n “capacitance array”. In this notation, the total energy can be expressed as =12𝐐𝐂1𝐐\mathcal{E}=\frac{1}{2}{{\bf Q}}\cdot{\bf C}^{-1}\cdot{\bf Q}. For convenience, the total energy \mathcal{E} presented below is always normalized by the self-energy of a single isolated sphere with the radius aa and a net charge qq, q2/(8πϵouta)q^{2}/(8\pi\epsilon_{\rm out}a). We note that this formulation applies to arbitrary particle shapes and cluster configurations. If the surface charge distribution is non-uniform or any external excitation exists, a multipole expansion of surface charge in terms of dipole, quadrupole etc. is needed. The constitutive relation eq. (8) and the quadratic expansion to energy can be generalized to include the contribution from these higher multipoles and external electric fields. For the purpose of demonstrating how the contact singularity is isolated, we focus on the case of the uniform surface charge distribution.

Our method for dielectrics is an extension to our earlier work on conductors.5 Because the conductors are equipotential, the mean potential is also the surface potential at every point on the surface. Since the capacitance 𝐂\bf C in eq. (8) contains two types of contributions, one type dominated by close contacts between neighboring particles, and the other type from the remaining interactions from all particles, we decompose the capacitance 𝐂\bf C as follows

𝐐=(cs𝐋+𝐇)𝐕.{\bf Q}=\left(c_{\rm s}{\bf L}+{\bf H}\right){\bf V}. (9)

Here, cs(h)=aϵout4ln(a/h)c_{\rm s}(h)=\frac{a\epsilon_{\rm out}}{4}\ln(a/h) is the singular capacitance for conductors derived above (assuming that all gap distances are hh). Since csc_{\rm s} becomes significant only for small gaps, the entries in the array 𝐋\bf L are nonvanishing only for closely neighboring particles. Specifically, if particle ii and jj form a close contact, we set the entries Lij=Lji=1L_{ij}=L_{ji}=-1. The diagonal entry LiiL_{ii} equals the number of close neighbors of the particle ii. All other entries of 𝐋\bf L are set to zero. The singular capacitance 𝐋\bf L as defined here is the same as the adjacency matrix representing the connectivity of clusters (see ref.5 for explicit examples). In practice, for a given cluster configuration, we first numerically solve the full capacitance array 𝐂\bf C at finite but small hh values, then subtract from 𝐂\bf C the singular term cs(h)𝐋c_{\rm s}(h){\bf L}, to get the regular capacitance 𝐇{\bf H}. The hh-dependence of this regular capacitance is then fitted to a straight line when hh is small, allowing us to obtain the full hh-dependence for the capacitance array 𝐂\bf C and, consequently, the full hh-dependence of energy, down to h=0h=0.

Generalizing eq. (9) to dielectrics requires two nontrivial modifications. First, the decomposition in eq. (9) is valid because the potential of the conductors can be used to evaluate the contact potential difference. But dielectrics are not equipotential, and the surface potential at the contact points V~i\tilde{V}_{i} generally differ from the average potential ViV_{i} by a numerical factor that depends on the dielectric permittivity and the cluster configuration. Its variation with gap distance hh is weak, and approaches a constant as h0h\to 0. So we generalize eq. (9) to

𝐐=(~𝐋+𝐇)𝐕,L~ij1ϵr,j1Vj{V~j(i)cij,ij;k=1NV~j(k)cjk,i=j.{\bf Q}=\left(\hbox{$\bf\tilde{\phantom{L}}$\kern-5.50003pt\hbox{$\bf L$}}+{\bf H}\right){\bf V},\quad\tilde{L}_{ij}\equiv\frac{1-\epsilon_{{\rm r},j}^{-1}}{V_{j}}\begin{cases}\tilde{V}_{j}^{(i)}c_{ij},&i\neq j;\\[5.0pt] {\sum_{k=1}^{N}}\tilde{V}_{j}^{(k)}c_{jk},&i=j.\end{cases} (10)

Above, the superscript ‘(i)(i)’ in V~j(i)\tilde{V}_{j}^{(i)} indicates that the contact potential is evaluated on the particle jj at the contact formed with the particle ii. The singular capacitance cijc_{ij} is given from eq. (7) by cij=ϵoutaij4(lnaijhijP(λij))c_{ij}=\frac{\epsilon_{\rm out}a_{ij}}{4}\left(\ln\frac{a_{ij}}{h_{ij}}-P(\lambda_{ij})\right), which depends on the mean radius of curvature aa, gap distance hh, and λ\lambda value evaluated for the particle pair ii and jj. From the definition, it is clear that ~\bf\tilde{\phantom{L}}𝐋\bf L is generally not symmetric, which however reduces to the (symmetric) form identical to eq. (9) in the conductor limit, since V~j(i)=Vj\tilde{V}_{j}^{(i)}=V_{j} for all contacts on the particle jj.

Second, it turns out that the contact potentials exhibit strong dependence on the second order and more distant neighbors, because the dielectric screening is comparatively weak (see Fig. 4 below). Therefore, to ensure rapid convergence of the correct contact potentials, our construction of the adjacency array ~\bf\tilde{\phantom{L}}𝐋\bf L contains all pairs of particles. Fortunately, as we shall see below, this construction requires no extra computation other than evaluating the surface potentials at additional contact points.

In order to identify the regular part 𝐇{\bf H} using eq. (10), we numerically compute the full capacitance matrix 𝐂(h){\bf C}(h) and all the contact potentials V~j(i)\tilde{V}_{j}^{(i)}, for a range of small but nonzero hh values. We used the boundary element method (BEM) implemented in the package COPSS 18 to solve Poisson’s equation. The solution is expressed in terms of the induced bound (polarization) charges σb\sigma_{\rm b}, which satisfies the following boundary integral equation,

1+ϵr2σb+(1ϵr)ϵout(𝐄b+𝐄f)𝐧^=1ϵr2σf.\frac{1+\epsilon_{\rm r}}{2}\sigma_{\rm b}+(1-\epsilon_{\rm r})\epsilon_{\rm out}\left({\bf E}_{\rm b}+{\bf E}_{\rm f}\right)\cdot\hat{\bf n}=\frac{1-\epsilon_{\rm r}}{2}\sigma_{\rm f}. (11)

Above, the electric field strength at the surface due to induced bound charge σb\sigma_{\rm b} and free charges σf\sigma_{\rm f} are expressed as surface integrals (α=b,f\alpha={\rm b,f}),

𝐄α=14πϵoutdS𝐫𝐫|𝐫𝐫|3σα(𝐫).{\bf E}_{\alpha}=\frac{1}{4\pi\epsilon_{\rm out}}\int\!{\rm d}S^{\prime}\,\frac{{\bf r}-{\bf r}^{\prime}}{|{\bf r}-{\bf r}^{\prime}|^{3}}\sigma_{\alpha}({\bf r}^{\prime}). (12)

By our convention, the surface normal 𝐧^\hat{\bf n} points outward. For clusters of multiple particles, it is understood that different particles may have different values of permittivity ϵr\epsilon_{\rm r}. Equation (11) is linear in σb\sigma_{\rm b} and σf\sigma_{\rm f}. After discretization, the bound charge is obtained by inverting the coefficient array. The apparent divergent diagonal entries while discretizing the surface integral eq. (12) can be re-parameterized to reproduce the correct self-energy. Further numerical details can be found in ref.8. In all calculations by BEM presented in this work (the dimer example used the exact series expansion.10), we meshed each spherical surface into 1734217342 triangular patches such that mesh size is about 0.03a0.03\,a.

In general, for a cluster of nn particles, nn separate numerical calculations with nn independent charge vectors 𝐐\bf{Q} are needed to determine the full capacitance matrix 𝐂{\bf C}. The computational cost can be reduced by imposing the symmetry of the cluster configuration. Subtracting from 𝐂\bf C the singular contribution ~\bf\tilde{\phantom{L}}𝐋\bf L is expected to give the hh-dependence of the regular part 𝐇\bf H. However, unlike the conductor case, where the coefficient to the logarithmic term is exactly known, the singular capacitance ~\bf\tilde{\phantom{L}}𝐋\bf L for dielectrics depends on the calculated contact potentials V~j(i)\tilde{V}_{j}^{(i)}, which is susceptible to the numerical precision and what is meant by ‘contact point’ on a surface mesh. In practice, we vary the gap distance hh and compute a few trial values of contact potentials, then select the one that ensures the difference Hij(h)=CijL~ijH_{ij}(h)=C_{ij}-\tilde{L}_{ij} converges linearly with hh as h0h\to 0 for all the entries. In the following, three examples are presented to demonstrate the nature of the contact singularity, and to show that the regularization scheme allows us to obtain the energy of cluster of dielectric particles with small hh.

The first example is a dimer of identical dielectric spheres. It is the simplest example for demonstrating the effects of interfacial polarization.6, 9, 10, 21 Except a study on the interaction between a conducting sphere and a dielectric plane,20 very few past work tried to evaluate the energy at small separation, presumably due to the difficulty of resolving the aforementioned contact singularity. Therefore, we analyzed the polarization effect for dielectric dimers in close contact, verified the singular behavior in eq. (7), and showed that eq. (10) yields the full hh-dependence of energy. We studied both symmetric (𝐐=(q,q){\bf Q}=(q,q)) and asymmetric (𝐐=(q,q){\bf Q}=(q,-q)) cases, for a range of permittivity values (1ϵr1061\leq\epsilon_{\rm r}\leq 10^{6}). The energy at h=0h=0 is presented as a function of relative permittivity, which agrees with the exact result (see SI) found using the tangent-sphere coordinate.

Refer to caption
Figure 3: Electrostatic energy of a pair of identical spheres. (a) and (b): asymmetric charge 𝐐=(q,q){\bf Q}=(q,-q). (c) and (d): symmetric charge 𝐐=(q,q){\bf Q}=(q,q). In (b) and (d), dots are numerical results obtained using our proposed method, and curves are exact prediction obtained using the tangent-sphere coordinate (SI).

For the asymmetric case, interfacial polarization enhances the inter-particle attraction. To illustrate this effect, we subtract the energy of two isolated spheres from that of a dimer, then plot it against the gap distance in Fig. 3, for three representative values of ϵr\epsilon_{\rm r}: 1010, 10210^{2} and 10410^{4}. In absence of the polarization effect, the energy curves would exhibit no dependence on ϵr\epsilon_{\rm r}, and appear flat over this narrow range of h/ah/a values. As ϵr\epsilon_{\rm r} is increased from 11, we confirm the expected, stronger distance dependence, as h0h\to 0. In particular, for the case of ϵr=104\epsilon_{\rm r}=10^{4}, an apparent logarithmic dependence on hh is seen in Fig. 3a, which is precisely the singularity revealed in eq. (7) and is stronger for higher permittivity values. On the other hand, when the permittivity ϵr\epsilon_{\rm r} is decreased, this logarithmic dependence is cut off at an increasingly larger separation and becomes almost invisible when ϵr=10\epsilon_{\rm r}=10.

The normalized energy difference, as shown in Fig. 3a, evaluated at h=0h=0, is show in Fig. 3b for different ϵr\epsilon_{\rm r} values. This contact energy represents the energy gain for bringing two particles from infinity to contact. In terms of the normalizing energy unit, q2/(8πϵouta)q^{2}/(8\pi\epsilon_{\rm out}a), its value is 1-1 without the polarization effect, and becomes more negative as ϵr\epsilon_{\rm r} increases, eventually reaching 2-2 at ϵr=\epsilon_{\rm r}=\infty.5 The contribution from the polarization effect for ϵr100\epsilon_{\rm r}\gtrsim 100 is comparable to the coulombic attraction alone. Moreover, we notice a slow convergence of contact energy for permittivities ϵr103\epsilon_{\rm r}\gtrsim 10^{3}, owing to the weak lnϵr2\ln\epsilon_{\rm r}^{2} dependence in the contact capacitance eq. (7) at h=0h=0. Finally, we affirm our results obtained from eq. (10), by comparing the contact energies to the exact analytical results (SI).

For the symmetric case, the interfacial polarization weakens the inter-particle repulsion, which is seen from the hh-dependence of dimer energy. However, by symmetry, the potential difference in the gap region vanishes and thus no logarithmic behavior is observed in Fig. 3c. The energy scales linearly with hh and a straightforward extrapolation gives the contact energy for all permittivity values plotted in Fig. 3d. A much weaker polarization effect is found. Even for the conductor case, only about 10%10\% contact energy can be attributed to polarization effects. The contact energies converge for ϵr100\epsilon_{\rm r}\gtrsim 100, and reach 2(1/ln21)0.882(1/\ln 2-1)\simeq 0.88, in agreement with Maxwell’s result22 for the conducting dimers. As for the asymmetric case, the full ϵr\epsilon_{\rm r}-dependence matches the analytical calculation (SI). To conclude this example, we note that the symmetric case is a peculiar example where the contact singularity is strictly absent. For all other charge ratios, using the decomposition in eq. (10) to isolate the strong hh-dependence is necessary.

The second example concerns the energy of 88 identical spheres placed at the vertices of a cube, which illustrates the importance of the second order contact for dielectric clusters. As discussed above, the singular capacitance ~\bf\tilde{\phantom{L}}𝐋\bf L in eq. (10) contains not only contributions from the nearest neighbors, but also those from the second-order and higher order neighbors. Therefore, a sphere at a vertex of a cube forms a secondary contact with its 33 plane diagonal vertices, and a third order contact with the body diagonal vertex. Even though the higher order contributions are minor, because at such large separation, these contacts cease to be singular, keeping the second order contribution is essential for obtaining the correct linear scaling of the regular capacitance with gap distance hh shown in Fig. 4a.

As in the dimer case, these regularized capacitance allow us to evaluate the energy at arbitrarily small gap distance. Figure 4b shows the normalized energies when only one particle is charged, for which all the energetic contributions come from the interfacial polarization. Comparing the results from BEM and our regularization schemes containing varying order of contact contributions, it is clear that keeping the higher order singular contribution is necessary for correctly evaluating the energy for h/a0.05h/a\lesssim 0.05. In contrast, no such terms are needed for the conducting case.

Refer to caption
Refer to caption
Figure 4: (a) Variation of entry H11H_{11} in the regular capacitance array against separation. The results for the other entries are provided in Fig. S3. (b) Variation of electrostatic energy against separation for dielectric spheres with ϵr=100\epsilon_{\rm r}=100 placed on cubic vertices, where one sphere is charged.

The third example is our main result on the energy of clusters, from which the cohesive energy is obtained by subtracting the self-energy of particles at infinite separation. We considered two limiting configurations: the most extended one with all spheres arranged along a straight line (string), and the most compact one with all spheres posited at the vertices of the platonic solids (polyhedron). In our earlier work on the conducting spheres, the charges are allowed to flow freely between contacting spheres. The energy of polyhedron packing is found to be lower than that of the string packing at a finite separation. However, as the gap distance decreases, the polarization effects due to contact singularity become increasingly relevant, which ultimately makes the string packing to be energetically more favorable than the polyhedron packing. For the dielectric cases, we show that the weakened contact singularity causes another crossover between the relative stability of string-like and polyhedral packings.

Refer to caption
Refer to caption
Figure 5: Size dependence of electrostatic energy \mathcal{E} for string-like and polyhedral configurations, with fixed total charge. (a) Charge transfer is permitted. Dashed curve: =(2/n)1/3/(2ln2)\mathcal{E}=(2/n)^{1/3}/(2\ln 2), the energy for polyhedral configurations of conducting spheres.5 Solid curve: =ln(2na/r0)/[nln2ln(2a/r0)]\mathcal{E}=\ln(2na/r_{0})/[n\ln 2\,\ln(2a/r_{0})], the energy for a conducting cylinder of the same volume with length L=2naL=2na and radius r0=0.816ar_{0}=0.816\,a.23 (b) Charge transfer is prohibited. The total charge qq resides on the middle particle of the string (string-22) and an arbitrary vertex of polyhedron (polyhedron).

As the previous example, to highlight the polarization effects, a unit charge qq is placed on one sphere. For symmetric polyhedron packing, this charged sphere is arbitrarily chosen. For the string packing, we considered two extreme placings: at one end (string-1) and in the middle (string-2). For each particle configuration and charge assignment, we considered two scenarios: charge transfer between contacting particles is permitted (Fig. 5a) and prohibited (Fig. 5b).

When inter-particle charge transfer is permitted, while maintaining uniform charge distribution on each individual particle, the energy \mathcal{E} can be calculated using 𝐐𝐂1𝐐/2{\bf Q}\cdot{\bf C}^{-1}\cdot{\bf Q}/2. Minimizing this energy subject to the constraint of constant total charge qq, the optimal charge assignment is found to be 𝐐e=q𝐂𝐮/Ce{\bf Q}_{e}=q\,{\bf C}\cdot{\bf u}/C_{\rm e}, where 𝐮(1,1,,1){\bf u}\equiv(1,1,\cdots,1) and Cei,j=1nCijC_{\rm e}\equiv\sum_{i,j=1}^{n}C_{ij}. This implies that the optimal charge 𝐐e{\bf Q}_{e} produces identical average surface potentials for all the particles, which generalizes the ‘equipotential’ concept for conductors.5 Correspondingly, the minimized energy is given by q2/(2Ce)q^{2}/(2C_{\rm e}), where the mean capacitance CeC_{\rm e} weakly depends on the dielectric permittivity. In this scenario, there is no need to differentiate string-11 and string-22 configurations. The energies of string and polyhedron configurations at h=0h=0 are plotted in Fig. 5a, for  ϵr=10\epsilon_{\rm r}=10 and 500500. For all configurations, the energy decreases with the cluster size nn monotonically since the redistributed surface charges are further apart. The dependence on permittivity is surprisingly weak, and the size-dependence is nearly indistinguishable from that of the conductor case.5 Two curves are obtained by treating the cluster as a single conductor respectively, whose capacitance scales with the length scale of the cluster, i.e., n1/3n^{1/3} for the polyhedron packing and n/ln(n)n/\ln(n) for the string packing.5 The extended string packing has a lower cohesive energy because its effective capacitance is higher than that of the compact polyhedron packing.

More interesting behavior is found (Fig. 5b) when charge transfer is prohibited. The dependence on permittivity is evident for all three cases: string-11, string-22, and polyhedron. To better visualize energies of string-22 and polyhedron packing, energies of string-11 is presented in Fig. S4) The energy is lower for the cluster with higher permittivity, because the polarization effect is stronger. The energy of string-22 is lower than that of string-11 for identical nn, because the charged particles in the middle of the string can polarize the particles in two half strings. Further, the energies for both string-11 and string-22 configurations saturate as the cluster size grows beyond n=12n=12, because the polarization effect is short-ranged. To assess the relative stability of compact or extended configurations, we then only need to focus on the string-22 and the polyhedron cases.

Our results indicate that the relative energetic stability depends on the permittivity. For ϵr=10\epsilon_{\rm r}=10, the energy of the polyhedron packing is lower than the string-2 packing, which is opposite to the characteristic result for conductors shown in Fig. 5a. Therefore, we expect a crossover from stable compact packing to stable open packing at intermediate permittivity values. This is indeed the case shown for ϵr=500\epsilon_{\rm r}=500, whereby the energies of compact and open configurations closely trace each other, and the relative energetic stability changes at n=4n=4 and n=8n=8 respectively. As ϵr\epsilon_{\rm r} is further increased, the energy curves of corresponding configuration will converge to those in Fig. 5a, reversing the relative stability of open and compact packings.

In summary, we generalized our previous work on conducting particles,5 and developed a scheme to resolve the singular contact charges between touching dielectric spheres, which regularizes the full capacitance array by isolating the singular contributions, i.e., eq. (10). Using this scheme, we obtain the cohesive energies for dielectric clusters at zero separation containing up to n=20n=20 particles, which is difficult to resolve with brutal force numerical calculations. Our results show that the shape of stable clusters formed from dielectric particles depends on the permittivity ratio ϵr\epsilon_{\rm r}: open clusters is more stable for large ϵr\epsilon_{\rm r}, and compact clusters is more stable for small ϵr\epsilon_{\rm r}. Our scheme is applicable to systems with arbitrary packing geometry, charge distribution, and containing asymmetric interfaces that have different permittivities and radii of curvature on the contacting particles. At the heart of our scheme is the contact singularity, which resembles those encountered in the study of thermal conduction 16 and momentum transport across a narrow gap.24

References

  • 1 J. Kolehmainen, A. Ozel, Y. Gu, T. Shinbrot, and S. Sundaresan. Phys. Rev. Lett., 121:124503, 2018.
  • 2 V. Lee, S. R. Waitukaitis, M. Z. Miskin, and H. M. Jaeger. Nature Phys., 11:733, 2015.
  • 3 E. V. Shevchenko, D. V. Talapin, N. A. Kotov, S. O’Brien, and C. B. Murray. Nature, 439:55, 2006.
  • 4 J. W. Merrill, S. K. Sainis, and E. R. Dufresne. Phys. Rev. Lett., 103:138301, 2009.
  • 5 J. Qin, N. W. Krapf, and T. A. Witten. Phys. Rev. E, 93:022603, 2016.
  • 6 A. Russell. P. R. Soc. Lond. A-Conta., 82:524, 1909.
  • 7 J. Lekner. P. Roy. Soc. A-Math. Phy., 468:2829, 2012.
  • 8 K. Barros, D. Sinkovits, and E. Luijten. J. Chem. Phys., 140:064903, 2014.
  • 9 E. B. Lindgren, A. J. Stace, E. Polack, Y. Maday, B. Stamm, and E. Besley. J. Comput. Phys., 371:712, 2018.
  • 10 H. Lian and J. Qin. Mol. Syst. Des. Eng., 3:197, 2018.
  • 11 J. Qin, J. J de Pablo, and K. F. Freed. J. Chem. Phys., 145:124903, 2016.
  • 12 M. Shen, H. Li, and M. O. De La Cruz. Phys. Rev. Lett., 119:138002, 2017.
  • 13 K. Barros and E. Luijten. Phys. Rev. Lett., 113:017801, 2014.
  • 14 Z. M. Sherman, D. Ghosh, and J. W Swan. Langmuir, 34:7117, 2018.
  • 15 L. G. Leal. Advanced Transport Phenomena: Fluid Mechanics and Convective transport Processes. Cambridge University Press, 2007.
  • 16 G. K. Batchelor and R. W. O’Brien. P. Roy. Soc. A-Math. Phy., 355:313, 1977.
  • 17 O. D. Kellogg. Foundations of Potential Theory. Courier Corporation, 1953.
  • 18 X. Jiang, J. Li, X. Zhao, J. Qin, D. Karpeev, J. Hernandez-Ortiz, J. J. de Pablo, and O. Heinonen. J. Chem. Phys., 145:064307, 2016.
  • 19 L. Poladian. Q. J. Mech. Appl. Math., 41:395, 1988.
  • 20 S. V. Kalinin, E. Karapetian, and M. Kachanov. Phys. Rev. B, 70:184101, 2004.
  • 21 J. D. Love. Q. J. Mech. Appl. Math., 28:449, 1975.
  • 22 J. C. Maxwell. A Treatise on Electricity and Magnetism. Oxford: Clarendon Press, 1873.
  • 23 J. D. Jackson. Classical Electrodynamics. John Wiley & Sons, 1999.
  • 24 R. H. Davis, J. A. Schonberg, and J. M. Rallison. Phys. Fluids. A-Fluid., 1:77, 1989.