2.1. Governing equations

The mass transport from the surface of the particle is governed by the convection–diffusion equation. This may be written in dimensionless form as

(2.1)\begin{equation} \frac{\partial \theta}{\partial t} + \boldsymbol{u}\boldsymbol{\cdot}\boldsymbol{\nabla} \theta = \frac{1}{{Pe}}\nabla^2 \theta, \end{equation}

where $\boldsymbol {u}(\boldsymbol {x},t)$ is the velocity field and $\theta (\boldsymbol {x},t)$ is the concentration of the solute (Leal Reference Leal2012). The characteristic length scale is $r$, the linear dimension of the particle, so that the spatial coordinate is non-dimensionalised as $\boldsymbol {x} = \boldsymbol {x}^*/r$. The characteristic time scale is prescribed by the shear rate $E^*$, so that time is non-dimensionalised as $t=t^*E^*$. The Péclet number is defined ${Pe} \equiv r^2 E^* / \kappa$, where $\kappa$ is the diffusion coefficient of the solute. Our convention is to write dimensional quantities with a superscript $^*$ unless otherwise stated.

We shall adopt a frame of reference moving with the particle, such that the boundary of the particle $S_p$ is stationary. We impose the boundary condition

(2.2)\begin{equation} \left.\begin{array}{c@{}} \theta = 1 \quad \text{and}\quad \boldsymbol{u} = 0 \quad \text{for } \boldsymbol{x} \in S_p \\ \theta \rightarrow 0 \quad \text{as } |\boldsymbol{x}| \rightarrow \infty \end{array},\right\} \end{equation}

so that the concentration of solute at the particle surface is uniform. This boundary condition corresponds to non-dimensionalising the concentration field $C(\boldsymbol {x}^*,t^*)$ as $\theta = (C-C_0)/(C_1-C_0)$, where $C_1$ and $C_0$ are the concentration of solute at the surface and infinity in physical units.

The non-dimensional measure of the surface flux $Q$ is the Sherwood number

(2.3)\begin{equation} {Sh} = \frac{Q}{4{\rm \pi} r\kappa(C_1 - C_0)} ={-}\frac{1}{4{\rm \pi}} \iint_{S_p} \boldsymbol{\nabla} \theta \boldsymbol{\cdot} \mathrm{d}\boldsymbol{S}. \end{equation}

The denominator in (2.3) corresponds to the steady state flux from a sphere of radius $r$ in the absence of flow. A convenient choice for the length scale $r$ is $\sqrt {A/4{\rm \pi} }$, where $A$ is the surface area of the particle. The Sherwood number is therefore the factor by which convection enhances the mass transfer relative to the diffusive flux from a spherical particle with the same surface area.

2.2. General solution of the surface flux in steady flow

In steady flow, the scalar transport equation reduces to

(2.4)\begin{equation} \boldsymbol{u}\boldsymbol{\cdot} \boldsymbol{\nabla} \theta = \frac{1}{{Pe}} \nabla^2 \theta. \end{equation}

We seek an asymptotic solution for (2.4) subject to (2.2) at large Péclet number.

At large Péclet number, the concentration of solute is small almost everywhere far from the particle, apart from a thin wake, along which material from the surface is swept. Near the particle, there is a concentration boundary layer whose thickness is $O(\delta )$, across which there is a sharp jump in concentration. For the boundary layer approximation to hold, the pathlines near the surface of the particle must originate and terminate at infinity, such that the surface of the particle is exposed to a constant stream of fresh fluid. Recirculating regions (closed pathlines), which can occur in some geometries, are not permitted.

We shall construct a general curvilinear coordinate system $(\xi , \eta , \zeta )$ to describe the flow near the surface in terms of the distance from the surface and the direction of the flow near the surface. This coordinate system is not necessarily orthogonal and we will find it useful to describe it in terms of the covariant coordinate vectors

(2.5a–c)\begin{equation} \boldsymbol{h}_\xi = \frac{\partial \boldsymbol{x}}{\partial \xi}, \quad \boldsymbol{h}_\eta = \frac{\partial \boldsymbol{x}}{\partial \eta}, \quad \boldsymbol{h}_\zeta= \frac{\partial \boldsymbol{x}}{\partial \zeta}, \end{equation}

and their pathlines, which we have illustrated in figure 1. We note that the adoption of a general curvilinear coordinate system, rather than an orthogonal one, is crucial in the generalisation to an arbitrary flow or body.

Figure 1.

Illustration of the curvilinear coordinate system $(\xi ,\eta ,\zeta )$ defined on the surface ($\xi =0$) of a spheroid in an arbitrary linear shear. Thick black lines show $\eta$-coordinate pathlines ($\xi =0,\zeta =\text {const.}$), which are tangent to the local viscous shear stress on the surface. Thin grey lines are $\zeta$-coordinate pathlines ($\xi = 0, \eta =\text {const.}$). Three fixed points of the surface streamlines are shown: red (source), green (saddle) and blue (sink).

The coordinate $\xi$ is defined as the normal distance from the particle surface, so that at the particle surface, $\boldsymbol {h}_\xi$ is a unit vector normal to the surface. The $\eta$ and $\zeta$ coordinates lie tangent to the surface. We shall define the $\eta$ coordinate so that at a small distance $\xi$ above the surface, the component of fluid velocity which is tangent to the surface is parallel to $\boldsymbol {h}_\eta$. The curves along the $\eta$ direction are therefore ‘surface streamlines’ which are tangent to the direction of the surface velocity gradient $\boldsymbol {w} = \partial \boldsymbol {u}/\partial \xi |_{\xi =0}$.

We can therefore express the velocity near the surface as

(2.6)\begin{align} \boldsymbol{u}&= u^\xi \boldsymbol{h}_\xi + u^\eta\boldsymbol{h}_\eta + u^\zeta\boldsymbol{h}_\zeta \nonumber\\ &= \boldsymbol{w}\xi + O(\xi^2), \end{align}

so that near the particle surface, the velocity components are of the form

(2.7a–c)\begin{equation} u^\xi = G(\eta,\zeta)\xi^2 + O(\xi^3), \quad u^\eta = \xi F(\eta,\zeta) + O(\xi^2), \quad u^\zeta = O(\xi^2). \end{equation}

By definition, the velocity at the surface is zero; the tangential component $u^\eta$ is linear in $\xi$ to leading order, whereas the surface-normal component is quadratic (Leal Reference Leal2012). The function $F(\eta , \zeta )$ is therefore obtained in terms of the velocity gradient at the surface of the particle as

(2.8)\begin{equation} F = \boldsymbol{w} \boldsymbol{\cdot} \boldsymbol{\nabla} \eta, \end{equation}

and is related to $G(\eta ,\zeta )$ through the continuity equation.

To obtain the surface-normal velocity component $u^\xi$, we express the continuity equation as (Grinfeld Reference Grinfeld2013)

(2.9)\begin{equation} \rho\nabla_i u^i = \frac{\partial (\rho u^\xi)}{\partial \xi} + \frac{\partial (\rho u^\eta)}{\partial \eta} + \frac{\partial (\rho u^\zeta)}{\partial \zeta} = 0, \end{equation}

where $\rho = \rho (\eta , \zeta ) \equiv \sqrt {\det {g}}$ and $\det {g}$ is the determinant of the metric tensor ${\mathsf{g}}_{ij} \equiv \boldsymbol {h}_i\boldsymbol {\cdot }\boldsymbol {h}_j$. Since $g_{\xi \xi } = 1$, $g_{\xi \eta } = g_{\xi \zeta } = 0$ by definition, the physical interpretation of $\rho$ is a local area density of the surface streamlines, such that $\delta A = \rho \delta \eta \delta \zeta$ is the area covered by a small region on the surface measuring $\delta \eta$ along a surface streamline and $\delta \zeta$ across adjacent streamlines. We can then define a streamfunction $\psi$ as

(2.10a,b)\begin{equation} u^\xi ={-}\frac{1}{\rho} \frac{\partial \psi}{\partial \eta} + O(\xi^3), \quad u^\eta = \frac{1}{\rho} \frac{\partial \psi}{\partial \xi}+ O(\xi^2), \end{equation}

so that

(2.11)\begin{equation} \psi = \tfrac{1}{2}\xi^2 \rho F, \end{equation}

is a solution which satisfies (2.7a–c) and the continuity equation (2.9) to leading order in $\xi$.

Writing (2.4) in these curvilinear coordinates, our solution now proceeds analogously to the works of Acrivos & Goddard (Reference Acrivos and Goddard1965) and Batchelor (Reference Batchelor1979). We shall formalise Batchelor's analysis here in our new curvilinear coordinate system for the purpose of exposition. To leading order in $\xi$, the convection term is

(2.12)\begin{equation} u^i \nabla_i \theta ={-}\frac{1}{\rho}\frac{\partial \psi}{\partial \eta}\frac{\partial \theta}{\partial \xi} +\frac{1}{\rho}\frac{\partial \psi}{\partial \xi}\frac{\partial \theta}{\partial \eta} + O(\xi^2), \end{equation}

whereas the diffusion term may be written

(2.13)\begin{equation} \nabla^2 \theta = \frac{1}{\rho} \left[ \frac{\partial}{\partial \xi^i}\left(\rho {\mathsf{g}}^{ij} \frac{\partial \theta}{\partial \xi^j}\right) \right] = \frac{1}{\rho} \frac{\partial}{\partial \xi}\left(\rho \frac{\partial \theta}{\partial \xi}\right) + \cdots , \end{equation}

where ${\mathsf{g}}^{ij}$ is the inverse metric tensor and $\xi ^i$ indexes the coordinates $(\xi ,\eta ,\zeta )$. The terms omitted in the expansion of (2.13) do not involve any gradients in $\xi$. By neglecting them, we assume that the diffusive flux of material across the surface is small in comparison to that normal to the surface. This essentially requires that the particle surface be smooth and contain no regions of extreme curvature where this assumption may break down.

We now rescale our coordinate system and streamfunction so that the surface-normal concentration gradient is $O(1)$. Rescaling $\xi$ by the boundary layer thickness $\delta$, we write

(2.14a,b)\begin{equation} \varXi = \frac{\xi r}{\delta} = \xi{Pe}^m, \quad \varPsi = \frac{1}{2}\varXi^2 \rho F = {Pe}^{2m} \psi, \end{equation}

where we suppose $\delta /r$ scales as ${Pe}^{-m}$. We can rewrite (2.4) using (2.12) and (2.13)

(2.15)\begin{equation} {-}\frac{\partial \varPsi}{\partial \eta}\frac{\partial \theta}{\partial \varXi} +\frac{\partial \varPsi}{\partial \varXi}\frac{\partial \theta}{\partial \eta} +O({Pe}^{{-}m}) = {Pe}^{3m-1} \frac{\partial}{\partial \varXi} \left(\rho \frac{\partial \theta}{\partial \varXi}\right). \end{equation}

The first two terms in (2.15) are $O(1)$ and thus $m=1/3$, as expected.

We can now solve (2.15) with the well-known von Mises transformation. Adopting the change of variables $(\varXi ,\eta ,\zeta ) \rightarrow (\varPsi ,\eta ,\zeta )$, we have

(2.16)\begin{equation} \frac{\partial \theta}{\partial \eta} = \frac{\partial}{\partial \varPsi}\left( \rho \frac{\partial \theta}{\partial \varPsi} \frac{\partial \varPsi}{\partial \varXi} \right) = \frac{\partial}{\partial \varPsi}\left( \frac{\partial \theta}{\partial \varPsi}(2\rho^3 F\varPsi)^{1/2} \right). \end{equation}

Equation (2.16) now admits a self-similar solution of the form $\theta = \theta (\chi ), \chi = \varPsi ^{1/2}/\tau ^{1/3}$, where the functions $\theta (\chi )$ and $\tau (\eta )$ must satisfy

(2.17)\begin{equation} \frac{\mathrm{d}^2 \theta}{\mathrm{d} \chi^2} + \frac{4}{3}\chi^2 \frac{\mathrm{d} \theta}{\mathrm{d} \chi} = 0, \end{equation}

for

(2.18)\begin{equation} \frac{\mathrm{d}\tau}{\mathrm{d}\eta} = (2\rho^3 F)^{1/2}. \end{equation}

The solution of (2.17) satisfying the imposed boundary conditions (2.2) of $\theta (0) = 1$ and $\theta = 0$ as $\chi \rightarrow \infty$ is

(2.19)\begin{equation} \theta(\chi) = \frac{\varGamma(\frac{1}{3}, \frac{4}{9} \chi^3)}{\varGamma(\frac{1}{3},0)}, \end{equation}

where $\varGamma$ is the incomplete gamma function. We can obtain $\tau$ by integrating (2.18) along the surface streamlines, which must begin and terminate at critical points $F=0$ on the surface, since the surface shear stress is continuous. We will therefore choose the constant of integration so that

(2.20)\begin{equation} \tau(\eta) = \int_{\eta_0}^{\eta} (2\rho^3 F)^{1/2}\, \mathrm{d}\eta, \end{equation}

has $\tau (\eta _0) = 0$ at the beginning of the surface streamline $\eta =\eta _0$ and $\tau (\eta _1) = \tau _1$ at the end $\eta = \eta _1$.

At the surface, the local flux of material per unit area is

(2.21)\begin{align} {-}\left.\frac{\partial \theta}{\partial \xi}\right|_{\xi = 0} &=\left. -{Pe}^{1/3} \frac{\partial \theta}{\partial \varXi}\right|_{\varXi=0} = \left.-{Pe}^{1/3} \frac{\partial \theta}{\partial \chi}\right|_{\chi=0} \cdot\left.\frac{\partial \chi}{\partial \varXi}\right|_{\varXi=0} \nonumber\\ &= {Pe}^{1/3} \frac{12^{1/3}}{\varGamma(\frac{1}{3})} \cdot \frac{\left(\frac{1}{2}\rho F\right)^{1/2}}{\tau^{1/3}}. \end{align}

The Sherwood number (2.3) is therefore given by

(2.22)\begin{align} {Sh}&={-}\frac{1}{4{\rm \pi}} \left.\iint_{S_p} \frac{\partial \theta}{\partial \xi}\right|_{\xi=0} \rho\,\mathrm{d}\eta \,\mathrm{d}\zeta \nonumber\\ &= \frac{12^{1/3} {Pe}^{1/3}}{8{\rm \pi} \varGamma(\frac{1}{3})} \iint_{S_p} \frac{(2 \rho^3 F)^{1/2}}{\tau^{1/3}}\, \mathrm{d}\eta \,\mathrm{d}\zeta, \end{align}

which we can integrate by parts by recognising that

(2.23)\begin{equation} \int_{\eta_0}^{\eta_1} \frac{\left(2 \rho^3 F\right)^{1/2}}{\tau^{1/3}}\, \mathrm{d}\eta =\int_{\eta_0}^{\eta_1} \frac{\mathrm{d}\tau}{\mathrm{d}\eta} \tau^{{-}1/3}\, \mathrm{d}\eta =\frac{3}{2} \tau_1^{2/3}, \end{equation}

and thus

(2.24)\begin{equation} {Sh}= \frac{0.808 {Pe}^{1/3}}{4{\rm \pi}} \int \left( \int_{\eta_0}^{\eta_1} \rho^{3/2} F^{1/2}\, \mathrm{d}\eta \right)^{2/3}\mathrm{d}\zeta + O(1). \end{equation}

As expected, the limiting dimensionless flux scales as $\alpha {Pe}^{1/3}$, with a prefactor $\alpha$ which can now be explicitly computed in terms of the shape of the body and the surface velocity gradient.

The main point of (2.24) is that we have generalised the results of Acrivos & Goddard (Reference Acrivos and Goddard1965) and Batchelor (Reference Batchelor1979) to any distribution of surface streamlines on an arbitrary body, not just those which result in an orthogonal coordinate system. The caveat remains that the pathlines around the body should be open for the boundary layer approximation to hold and the boundary should be smooth and contain no regions of extreme curvature. Furthermore, we have a natural way of numerically constructing the local area density $\rho$, as shown graphically in figure 1. By integrating (2.5a–c) with respect to $\eta$ to generate a set of surface streamlines over the body, we obtain lines of constant $\zeta$ at intervals of varying $\eta$. With a sufficiently fine discretisation, we can numerically approximate the local area density $\rho$ and evaluate the coefficient in (2.24) numerically. We shall demonstrate this procedure later in § 3.

2.3. Unsteady solution at large Péclet number

We now seek to generalise our steady solution to an unsteady, periodic flow. Our argument is analogous to that proposed by Batchelor (Reference Batchelor1980), who examined the scalar flux to spherical particles in turbulent flow.

We shall consider the case where the motion is periodic with period $T = E^*T^*$. We seek the time average Sherwood number $\overline{\textit{Sh}}$ at the surface, which depends upon the time average concentration field $\overline{\theta }$. The time average over a period $T$ is defined simply as

(2.25)\begin{equation} \overline{\theta }(\boldsymbol{x}) = \frac{1}{T} \int_{0}^{T} \theta(\boldsymbol{x},t) \mathrm{d}t. \end{equation}

Applying this averaging procedure to (2.1), we obtain

(2.26)\begin{equation} \overline{\boldsymbol{u}} \boldsymbol{\cdot} \boldsymbol{\nabla}\overline{\theta } + \overline{\boldsymbol{u}' \boldsymbol{\cdot} \boldsymbol{\nabla} \theta'} = \frac{1}{{Pe}} \nabla^2 \overline{\theta }, \end{equation}

where we have decomposed the velocity field $\boldsymbol {u} = \overline {\boldsymbol {u}} + \boldsymbol {u}'$ and concentration field $\theta =\overline{\theta }+\theta '$ into their respective average and fluctuating components. Likewise, the transport equation for the concentration fluctuation $\theta '(\boldsymbol {x}, t)$ is

(2.27)\begin{equation} \frac{\partial \theta'}{\partial t} + \boldsymbol{u}\boldsymbol{\cdot}\boldsymbol{\nabla} \theta' - \overline{\boldsymbol{u}'\boldsymbol{\cdot}\boldsymbol{\nabla} \theta'} - \frac{1}{{Pe}} \nabla^2 \theta' ={-}\boldsymbol{u}'\boldsymbol{\cdot} \boldsymbol{\nabla} \overline{\theta }. \end{equation}

We shall argue that the solution of (2.27) satisfying the boundary conditions (2.2) and

(2.28a,b)\begin{equation} \theta' = 0 \text{ at } \xi = 0 \quad\text{and} \quad \theta' = 0 \text{ as } \xi \rightarrow \infty, \end{equation}

is such that $\theta ' \sim {Pe}^{-1/3}$ as ${Pe} \rightarrow \infty$. As before, we reason that the solution consists of a slender concentration boundary layer of thickness $\delta /r \sim {Pe}^{-1/3}$. Outside the boundary layer $\xi \gg \delta$, $\overline{\theta } \rightarrow 0$ and $\theta ' \rightarrow 0$. Inside the boundary layer, the amplitude of the concentration fluctuations are $\theta ' = O({Pe}^{m'})$ and the jump in the mean concentration across the boundary layer is $O(1)$. Clearly, $m' \le 0$ since there is no mechanism in (2.1) which can amplify scalar fluctuations. If $m' < 0$, then scalar fluctuations should decay in amplitude at large ${Pe}$, whereas if $m' = 0$ they remain comparable in magnitude to the mean flow.

Let us examine the order of magnitude of the terms in (2.27). Since scalar fluctuations are $O({Pe}^{m'})$ and occur on a time scale of $O(T)$, the time derivative term scales as

(2.29)\begin{equation} \frac{\partial \theta}{\partial t} \sim \frac{{Pe}^{m'}}{T}. \end{equation}

The convective terms on the left-hand side scale as

(2.30)\begin{equation} \boldsymbol{u}\boldsymbol{\cdot} \boldsymbol{\nabla} \theta' = u^\xi \frac{\partial \theta'}{\partial \xi} + \cdots \sim \left(\frac{\delta^2}{r^2}\right) \left(\frac{r}{\delta} {Pe}^{m'} \right) \sim {Pe}^{m'-1/3}, \end{equation}

whereas the convective term on the right-hand side scales as

(2.31)\begin{equation} \boldsymbol{u}' \boldsymbol{\cdot} \boldsymbol{\nabla} \overline{\theta } = {u^\xi}' \frac{\partial \overline{\theta }}{\partial \xi} + \cdots \sim \left(\frac{\delta^2}{r^2}\right) \left(\frac{r }{\delta}\right) \sim {Pe}^{{-}1/3}. \end{equation}

Finally, the diffusion term scales as

(2.32)\begin{equation} \frac{1}{{Pe}}\nabla^2 \theta' \approx \frac{1}{{Pe}} \frac{\partial^2 \theta'}{\partial \xi^2} \sim \frac{1}{{Pe}} \frac{r^2}{\delta^2} {Pe}^{m'} \sim {Pe}^{m' - 1/3}. \end{equation}

Annotating (2.27) with the order of magnitude of each term, we have

(2.33)\begin{equation} \underbrace{\frac{\partial \theta'}{\partial t}}_{O({Pe}^{m'}/T)} \underbrace{ + \boldsymbol{u}\boldsymbol{\cdot}\boldsymbol{\nabla} \theta' - \overline{\boldsymbol{u}'\boldsymbol{\cdot}\boldsymbol{\nabla} \theta'} - \frac{1}{{Pe}} \nabla^2 \theta' }_{O({Pe}^{m'-1/3})} ={-}\underbrace{\boldsymbol{u}'\boldsymbol{\cdot} \boldsymbol{\nabla} \overline{\theta }}_{O({Pe}^{{-}1/3})}. \end{equation}

We see that the solution requires $m'=-1/3$, such that the first term on the left-hand side dominates and balances the unsteady convection term on the right-hand side, provided the dimensionless period $T \ll {Pe}^{1/3}$. Thus, at large Péclet, we have

(2.34)\begin{equation} \frac{\partial \theta'}{\partial t} \approx{-}\boldsymbol{u}'\boldsymbol{\cdot} \boldsymbol{\nabla} \overline{\theta } \sim {Pe}^{{-}1/3}, \end{equation}

which is equivalent to (3.9) of Batchelor (Reference Batchelor1980). However, we have derived the result on more general grounds. Physically, this result means that when the time scale of diffusion within the boundary layer becomes large in comparison to the time scale of the unsteadiness, there is insufficient time for diffusion to redistribute scalar fluctuations. Instead, scalar fluctuations inside the boundary layer occur due to the convection of the mean concentration field by unsteady velocity fluctuations.

Thus, to leading order, the concentration and its time mean are equal and the mean scalar field is well approximated by

(2.35)\begin{equation} \overline{\boldsymbol{u}}\boldsymbol{\cdot}\boldsymbol{\nabla}\overline{\theta } = \frac{1}{{Pe}}\nabla^2 \overline{\theta } + O({Pe}^{{-}2/3}). \end{equation}

This allows us to apply our general result (2.24) to unsteady, time periodic flows where the period of motion is sufficiently small. As before, for the boundary layer approximation to hold, it is required that the surface of the particle be exposed to a continuous stream of fresh fluid. Therefore, it is required that the pathlines of fluid parcels adjacent to the surface be open, such that the fluid does not simply recirculate around a closed path.

3.1. Motion of a freely suspended spheroid

Let us consider the motion of a spheroidal particle in an arbitrary, linear shear flow. The background linear shear is $\boldsymbol {v} = \boldsymbol{\mathsf{G}}\boldsymbol{y}$, where $\boldsymbol {y}=\boldsymbol {y}^*/r$ is the coordinate system of the fixed laboratory frame and $\boldsymbol{\mathsf{G}} = \boldsymbol{\mathsf{E}} + \boldsymbol{\mathsf{W}}$ is an arbitrary, steady velocity gradient in this reference frame. The velocity gradient is composed of a symmetric strain tensor $\boldsymbol{\mathsf{E}}=\boldsymbol{\mathsf{E}}^*/E^*$ and antisymmetric rotation tensor $\boldsymbol{\mathsf{W}}=\boldsymbol{\mathsf{W}}^*/E^*$. We shall choose the characteristic shear rate ${\mathsf{E}}^* = ({\mathsf{E}}_{ij}^*{\mathsf{E}}_{ij}^*)^{1/2}$ so that ${\mathsf{E}}_{ij}{\mathsf{E}}_{ij}=1$.

The spheroid is centred at the origin and its semiaxes $a_i = (a,c,c)$ are spanned by an orthogonal set of unit vectors $\boldsymbol {p},\boldsymbol {q},\boldsymbol {r}$. Thus, the coordinate $\boldsymbol {x}$ in the body frame maps to the laboratory frame as $\boldsymbol {y} = \boldsymbol{\mathsf{R}}\boldsymbol {x}$, where $\boldsymbol{\mathsf{R}} = [\boldsymbol {p}, \boldsymbol {q}, \boldsymbol {r}]$. The unit vector $\boldsymbol {p}$ points along the symmetry axis towards the ‘pole’ of the spheroid, whilst $\boldsymbol {q}$ and $\boldsymbol {r}$ point radially outward around the ‘equator’. The body rotates with angular velocity $\boldsymbol {\varOmega }=\boldsymbol {\varOmega }(t)$, such that $\dot {\boldsymbol{\mathsf{R}}} = [\boldsymbol {\varOmega }]_\times \boldsymbol{\mathsf{R}}$, and the velocity field in the body frame is

(3.1)\begin{equation} \boldsymbol{u}(\boldsymbol{x},t) = \boldsymbol{\mathsf{R}}^\textrm{T}\boldsymbol{v}(\boldsymbol{\mathsf{R}}\boldsymbol{x},t) - \boldsymbol{\varOmega}\times(\boldsymbol{\mathsf{R}}\boldsymbol{x}). \end{equation}

Thus, the background velocity gradient $\boldsymbol {u}=\boldsymbol{\mathsf{A}}\kern1.5pt\boldsymbol {x}$ appears in the body frame as

(3.2)\begin{equation} \boldsymbol{\mathsf{A}} = \boldsymbol{\mathsf{R}}^\textrm{T} (\boldsymbol{\mathsf{G}} - [\boldsymbol{\varOmega}]_\times) \boldsymbol{\mathsf{R}}, \end{equation}

and, in general, varies in time as the particle rotates. Jeffery (Reference Jeffery1922) showed that, when the couple upon a spheroid is zero, the solid body rotation rate $\boldsymbol {\varOmega }$ of the body is given by

(3.3)\begin{equation} \boldsymbol{\varOmega} = \frac{1}{2}\boldsymbol{\omega} + \frac{\lambda^2-1}{\lambda^2+1} \boldsymbol{p}\times \boldsymbol{\mathsf{E}}\boldsymbol{p}, \end{equation}

where $\omega _i = -\epsilon _{ijk}{\mathsf{W}}_{jk}$ is the background vorticity in the laboratory frame. Thus, the orientation of the particle $\boldsymbol {p}$ then evolves according to Jeffery's equation

(3.4)\begin{equation} \dot{\boldsymbol{p}} = \boldsymbol{\mathsf{W}}\boldsymbol{p} + \frac{\lambda^2-1}{\lambda^2+1} \left(\boldsymbol{\mathsf{E}}\boldsymbol{p} - \boldsymbol{p}\left(\kern1.5pt\boldsymbol{p}^\textrm{T}\boldsymbol{\mathsf{E}}\boldsymbol{p}\right)\right)\!, \end{equation}

where ${\mathsf{W}}_{ij} = \frac {1}{2}\epsilon _{ijk}\omega _k$ is the rate of rotation tensor.

When the background shear is constant in time, the solution to (3.4) can be written in terms of a matrix exponential as

(3.5a–c)\begin{equation} \boldsymbol{p}(t) = \frac{\breve{\boldsymbol{p}}}{|\breve{\boldsymbol{p}}|}, \quad \breve{\boldsymbol{p}}(t) = \exp\left(\boldsymbol{\mathsf{K}}t\right) \boldsymbol{p}_0, \quad \boldsymbol{\mathsf{K}} = \boldsymbol{\mathsf{W}} + \frac{\lambda^2-1}{\lambda^2+1}\boldsymbol{\mathsf{E}}, \end{equation}

subject to the initial condition $\boldsymbol {p}=\boldsymbol {p}_0$ at $t=0$ (Szeri Reference Szeri1993).

We shall now examine the fixed points and stable attractors of (3.4). This analysis elaborates upon the previous work by Bretherton (Reference Bretherton1962). Decomposing $\boldsymbol{\mathsf{K}}$ in terms of its eigenvectors $\boldsymbol {e}_i$ and eigenvalues $\lambda _i$, we can write (3.5a–c) as

(3.6)\begin{equation} \breve{\boldsymbol{p}} = \sum_i (\boldsymbol{p}_0\boldsymbol{\cdot}\boldsymbol{e}_i) \exp(\lambda_i t) \boldsymbol{e}_i. \end{equation}

From (3.6) we see that the fixed points of (3.4) coincide with the eigenvectors $\boldsymbol {e}_i$. The stability of the fixed points depends upon the eigenvalues $\lambda _i$, and because $\sum _i \lambda _i =0$, there is always only one (neutrally) stable fixed point or limit cycle (excepting $\lambda _i=0$). Thus after a finite time, the motion of the particle will always approach a stable attractor whose nature depends upon the largest eigenvalue(s) of $\boldsymbol{\mathsf{K}}$.

We can categorise the stable attractors into five different cases: 1a, 1b, 2a, 2b and 3. These five cases map to four different motions: resting, spinning, 2-D (two-dimensional) tumbling and 3-D (three-dimensional) tumbling. These are summarised in table 1. We shall now examine each case.

Table 1.

Classification of the motion and time average perceived velocity gradient experienced by a spheroid.

In cases 1a and 1b, all the eigenvalues $\lambda _1 \le \lambda _2 \le \lambda _3$ of $\boldsymbol{\mathsf{K}}$ are real and (3.5a–c) has three fixed points $\boldsymbol {p} = \boldsymbol {e}_i$, where $\boldsymbol {e}_i$ are the eigenvectors of $\boldsymbol{\mathsf{K}}$. From (3.6) we see that only the fixed point corresponding to the largest eigenvalue $\lambda _3$ is stable, so for nearly any initial condition, the particle will reorient itself to be parallel to $\boldsymbol {e}_3$. In this configuration, the particle will in general rotate about its axis with angular velocity $\boldsymbol {\varOmega } = \varOmega _3 \boldsymbol {e}_3$, where $\varOmega _3 = \boldsymbol {\omega }\boldsymbol {\cdot }\boldsymbol {e}_3/2$ (case 1a). We call this motion spinning. However, for particular configurations, $\varOmega _3 = 0$ and the particle does not rotate (case 1b). We call this motion resting.

In cases 2a, 2b and 3, $\boldsymbol{\mathsf{K}}$ has a pair of complex eigenvalues and the system has one fixed point and a periodic point. In these cases, we can write the eigenvalues as $\lambda _1 = \lambda _2^{\dagger}ger = \sigma + \textrm {i}\omega , \lambda _3 = -2\sigma$, where ${\dagger}ger$ denotes the complex conjugate. When $\sigma < 0$, the fixed point is stable and the periodic point is unstable (case 2a, spinning). Thus the particle aligns with $\boldsymbol {e}_3$ as in cases 1a and 1b, but unlike case 1b, the particle must rotate about this axis because the angular velocity $\boldsymbol {\varOmega } = \varOmega _3 \boldsymbol {e}_3$ is bounded $\varOmega _3^2 \ge \omega ^2 > 0$. When $\sigma > 0$, the fixed point is unstable and the periodic point is stable (case 2b). Thus the particle will evolve towards a planar limit cycle oscillation described by

(3.7)\begin{equation} \breve{\boldsymbol{p}} = \boldsymbol{a}\cos(\omega t) + \boldsymbol{b}\sin(\omega t), \end{equation}

where $\boldsymbol {e}_1 = \boldsymbol {e}_2^{\dagger}ger = \boldsymbol {a}+\textrm {i}\boldsymbol {b}$. We call this motion 2-D tumbling. In case 3, $\sigma = 0$ and the motion follows 3-D Jeffery orbits (Jeffery Reference Jeffery1922), where $\boldsymbol {p}$ precesses around the axis $\boldsymbol {e}_3$ with period $2{\rm \pi} /\omega$. We call this motion 3-D tumbling (Jeffery orbits are in general three-dimensional, but for some initial conditions, the motion can be reduced to spinning or 2-D tumbling).

The solution of (2.26) depends upon the average flow field in the particle frame. The instantaneous flow field around the particle consists of a superposition of the background gradient $\boldsymbol{\mathsf{A}}\kern0.09em \boldsymbol {x}$ and a perturbation owing to the presence of the particle. Since this perturbation is linear in $\boldsymbol{\mathsf{A}}$, the time average flow field in the particle frame is determined by the average velocity gradient perceived by the particle. We shall now calculate the average velocity gradient perceived by the particle in the general limiting cases identified above.

In cases 1a and 2a (spinning), the particle rotates around a fixed axis $\boldsymbol {p}=\boldsymbol {e}_3$, which is illustrated in figure 2(a). For this spinning motion, the unit vectors of the body frame rotate as

(3.8a–c)\begin{equation} \boldsymbol{p} = \boldsymbol{e}_3,\quad \boldsymbol{q} = \cos(\varOmega_3 t) \boldsymbol{q}_0 + \sin(\varOmega_3 t) \boldsymbol{r}_0, \quad \boldsymbol{r} ={-}\sin(\varOmega_3 t) \boldsymbol{q}_0 + \cos(\varOmega_3 t) \boldsymbol{r}_0. \end{equation}

To obtain the time average velocity gradient, we can substitute (3.8a–c) into (3.2) and take the time average over one revolution, whose period is $T = 2{\rm \pi} /\varOmega _3$. After a little algebra, we obtain

(3.9)\begin{equation} \overline{\boldsymbol{\mathsf{A}}} = \frac{1}{T} \int_{0}^T \boldsymbol{\mathsf{R}}^\textrm{T}(\boldsymbol{\mathsf{G}}-[\boldsymbol{\varOmega}]_\times)\boldsymbol{\mathsf{R}}\, \mathrm{d}t = E_3 \begin{bmatrix} 1 & 0 & 0 \\ 0 & -\frac{1}{2} & 0 \\ 0 & 0 & -\frac{1}{2} \end{bmatrix}, \end{equation}

where

(3.10)\begin{equation} E_3 = \boldsymbol{e}_3^\textrm{T}\boldsymbol{\mathsf{E}}\boldsymbol{e}_3 = \frac{\lambda^2+1}{\lambda^2-1} \sigma, \end{equation}

is the rate of strain perceived by the particle along its fixed axis of rotation. Thus, the average velocity field experienced by a particle steadily rotating about its axis is an axisymmetric strain, whose magnitude is given by the component of strain along the rotation axis.

Figure 2.

Motion of a freely suspended spheroid: (a) spinning, (b) 2-D tumbling and (c) 3-D tumbling. For 2-D tumbling and spinning, the motion is periodic, whereas for 3-D tumbling only the motion of the symmetry axis is necessarily periodic.

In case 1b (resting), the particle axis aligns with $\boldsymbol {e}_3$, but the rotation rate about this axis vanishes. The average velocity field in the body frame is then simply

(3.11)\begin{equation} \overline{\boldsymbol{\mathsf{A}}} = \boldsymbol{\mathsf{RGR}}^{T}. \end{equation}

The average velocity gradient $\overline {\boldsymbol {A}}$ can be specified with three parameters, up to an arbitrary scaling and rotation about the symmetry axis of the particle. To see this, we note that $\boldsymbol{\mathsf{G}}$ has nine components with eight degrees of freedom, since continuity requires $\textrm {tr}(\boldsymbol{\mathsf{G}}) = 0$. The requirement that $\boldsymbol {\varOmega } = 0$ imposes the constraint

(3.12)\begin{equation} \boldsymbol{\omega} ={-}2\frac{\lambda^2-1}{\lambda^2+1} \boldsymbol{p}\times \boldsymbol{\mathsf{E}}\boldsymbol{p}, \end{equation}

reducing the number of unknowns by three. The choice of scale introduces another redundant parameter; our non-dimensionalisation requires ${\mathsf{E}}_{ij}{\mathsf{E}}_{ij} = 1$. Finally, we note that rotations about the particle's axis are trivial, since the particle is axisymmetric.

In case 2b (2-D tumbling), the motion of the particle is more complex, but remains periodic, as illustrated in figure 2(b). From (3.7) it follows that the symmetry axis $\boldsymbol {p}$ rotates in a plane spanned by vectors $\boldsymbol {a},\boldsymbol {b}$ with period $T = 2{\rm \pi} /\omega$. Thus the rotation $\boldsymbol{\mathsf{Q}}(t) = \boldsymbol{\mathsf{Q}}_2\boldsymbol{\mathsf{Q}}_1$ of the body frame $\boldsymbol{\mathsf{R}}(t) = \boldsymbol{\mathsf{Q}}\boldsymbol{\mathsf{R}}_0$ can be composed of as a rotation $\boldsymbol{\mathsf{Q}}_1(t)$ about the axis $\boldsymbol {a}\times \boldsymbol {b}$ (mapping $\boldsymbol {p}_0$ onto $\boldsymbol {p}$), followed by a rotation $\boldsymbol{\mathsf{Q}}_2(t)$ about the axis $\boldsymbol {p} = \boldsymbol{\mathsf{Q}}_1\boldsymbol {p}_0$ by an angle

(3.13)\begin{equation} \theta_p(t) = \int_{0}^{t} \frac{1}{2} \boldsymbol{\omega}\boldsymbol{\cdot} \boldsymbol{p}(t') \mathrm{d}t', \end{equation}

relative to the plane normal. By inspection of (3.13) and (3.7), we see that $\theta _p(T) = 0$, since $\boldsymbol {p}(t) = -\boldsymbol {p}(t+T/2)$. Thus, $\boldsymbol{\mathsf{R}}(t)$ must be periodic. The average perceived velocity gradient can then be evaluated analogously to (3.9), but the resultant expression is much more complicated. It suffices to remark that the average strain $\overline{\boldsymbol{\mathsf{E}}}$ and vorticity $\overline{\boldsymbol{\omega}}$ components of the average perceived velocity gradient $\overline{\boldsymbol{\mathsf{A}}}$ must also satisfy (3.12), since in the body frame, the apparent rotation rate of the body must also be zero. It follows that in case 2b, as in case 1b, the average perceived velocity gradient may also be described by only three parameters, up to a trivial rotation and choice of scale.

In case 3 (3-D tumbling), the particle motion becomes fully three dimensional, as illustrated in figure 2(c). Only the motion of its symmetry axis is necessarily periodic; the equatorial axes $\boldsymbol {q}$ and $\boldsymbol {r}$ may precess around and do not necessarily trace a path with the same period. Thus, we cannot expect the flow in the particle frame to be time periodic, since $\boldsymbol {q}$ and $\boldsymbol {r}$ point in a new direction at the start of each cycle, and we cannot expect to apply (2.24) in this special case.

We recall that the derivation of (2.24) required pathlines of the flow to be open. Far from the particle, pathlines follow $\dot {\boldsymbol {y}} = \boldsymbol{\mathsf{G}}\boldsymbol{y}$, with solution $\boldsymbol {y} = \exp (\boldsymbol{\mathsf{G}}t)\boldsymbol {y}_0$. By a similar argument to that above, we see that when $\boldsymbol{\mathsf{G}}$ has eigenvalues $0,\pm \mathrm {i}\omega$, the pathlines are closed. This provides a necessary condition to apply (2.24). The 3-D tumbling orbits identified by Jeffery (Reference Jeffery1922) happen to correspond to this case, which further precludes application of (2.24) to the case of Jeffery orbits.

To summarise: by an analysis of the stable attractors of (3.4) we can construct five cases of the particle motion categorised by the eigenvalues of $\boldsymbol{\mathsf{K}}$ (3.5a–c) as shown in table 1. In cases 1a, 1b and 2a, the particle orients itself along a fixed axis corresponding to the eigenvector $\boldsymbol{\mathsf{K}}$ with largest real eigenvalue. In cases 2b and 3, the particle undergoes a limit cycle oscillation. In cases 1a, 1b, 2a and 2b, the relative flow field is steady or periodic. In cases 1a, 2a (spinning) the average perceived velocity gradient over one period is an axisymmetric strain, because the particle rotates steadily about its axis. In cases 1b and 2b (resting or 2-D tumbling), the average perceived velocity gradient satisfies (3.12), which can be specified in terms of three parameters up to a trivial rotation and choice of scale.

3.2. The fluid motion near the particle

In the body frame, the surface at $\xi = 0$ is stationary, so to leading order in $\xi$ the velocity is

(3.14)\begin{equation} \boldsymbol{u} = \xi \left.\frac{\partial \boldsymbol{u}}{\partial \xi}\right|_{\xi = 0} + O(\xi^2). \end{equation}

After differentiation of Jeffery's solution for the relative velocity field for an arbitrary ellipsoid (Jeffery Reference Jeffery1922), rewritten in the more compact matrix notation used by Kim & Karrila (Reference Kim and Karrila1991), we find that the velocity gradient normal to the surface is given by

(3.15)\begin{equation} \left.\frac{\partial \boldsymbol{u}}{\partial \xi}\right|_{\xi=0} = \boldsymbol{\Phi}\boldsymbol{h}_\xi - \boldsymbol{h}_\xi(\boldsymbol{h}_\xi \boldsymbol{\cdot} (\boldsymbol{\Phi}\boldsymbol{h}_\xi)) = \boldsymbol{w}, \end{equation}

where $\boldsymbol {h}_\xi = \boldsymbol{\mathsf{D}}\boldsymbol {x}/|\boldsymbol{\mathsf{D}}\boldsymbol{x}|$ is the unit vector surface normal, $\boldsymbol{\mathsf{D}}$ is a diagonal matrix whose entries are $a_i^{-2}$ and

(3.16)\begin{equation} \boldsymbol{\Phi} = \frac{3}{4{\rm \pi} a_1 a_2 a_3}\boldsymbol{\mathsf{S}}. \end{equation}

The expression for the stresslet $\boldsymbol{\mathsf{S}}$ is more involved. We remark here that it is a symmetric matrix with $\textrm {tr}(\boldsymbol{\mathsf{S}}) = 0$ whose elements are a linear combination of the components of the velocity gradient $\boldsymbol{\mathsf{A}}$ with coefficients determined by geometry-dependent ‘resistance functions’. Complete expressions for $\boldsymbol{\mathsf{S}}$ can be found in Kim & Karrila (Reference Kim and Karrila1991). Equation (3.15) is valid for the general case of torque-free, tri-axial ellipsoids. The action of a net torque upon the body adds an additional skew–symmetric component to (3.16) which is not treated here.

Equation (3.15) now defines the surface streamlines, which are everywhere tangent to the surface velocity gradient $\boldsymbol {w}$. The surface streamlines and their critical points are illustrated for an arbitrary linear shear in figure 1. From (3.15) we see that critical points occur where the surface normal $\boldsymbol {h}_\xi$ coincides with an eigenvector $\pm \boldsymbol {q}_i$ of the surface gradient tensor $\boldsymbol{\Phi}$. Since $\boldsymbol{\Phi}$ is a symmetric matrix, its eigenvalues are all real and its eigenvectors orthogonal. In general, $\boldsymbol{\Phi}$ has three distinct eigenvalues ordered $\phi _1 < \phi _2 < \phi _3$ and there are six critical points. In special cases, $\boldsymbol{\Phi}$ has a repeated eigenvalue and there is a locus of critical points.

The precise nature of the critical points can be seen by introducing the surface potential

(3.17)\begin{equation} \phi(\boldsymbol{x}) = \boldsymbol{h}_\xi \boldsymbol{\cdot} (\boldsymbol{\Phi}\boldsymbol{h}_\xi) = \frac{\boldsymbol{x}^\textrm{T}\boldsymbol{\mathsf{D}}\boldsymbol{\Phi} \boldsymbol{\mathsf{D}}\boldsymbol{x}}{\boldsymbol{x}^\textrm{T}\boldsymbol{\mathsf{D}}^2\boldsymbol{x}}, \end{equation}

which has the property that

(3.18)\begin{equation} \boldsymbol{\nabla} \phi = \frac{2\boldsymbol{\mathsf{D}}\boldsymbol{w}}{\boldsymbol{x}^\textrm{T}\boldsymbol{\mathsf{D}}^2\boldsymbol{x}}. \end{equation}

The gradient of $\phi$ measured along surface streamlines is $\boldsymbol {w}\boldsymbol {\cdot }\boldsymbol {\nabla } \phi > 0$ everywhere on the surface except at the critical points $\boldsymbol {w}=0$ where the surface streamlines terminate. In other words, the potential $\phi$ always increases as one moves along a surface streamline. The potential takes a minimum value of $\phi = \phi _1$ when $\boldsymbol {h}_\xi = \pm \boldsymbol {q}_1$ (red marker in figure 1), i.e. surface streamlines originate from a ‘source’ $\phi = \phi _1$. It takes a maximum value of $\phi = \phi _3$ when $\boldsymbol {h}_\xi = \pm \boldsymbol {q}_3$ (blue marker), i.e. surface streamlines terminate at a ‘sink’ $\phi = \phi _3$. Lastly, when the eigenvalues are distinct, all streamlines must pass through the contour $\phi = \phi _2$, except at points $\boldsymbol {h}_\xi = \pm \boldsymbol {q}_2$, which are saddle points (green marker). When there is a repeated eigenvalue, either $\phi _2 = \phi _1$ or $\phi _2 = \phi _3$, so there exists a locus of points where streamlines originate (or terminate). It should be noted that the definition of $\phi$ (3.17) and its properties extend also to torque-free, tri-axial ellipsoids.

3.3. Surface flux under spinning motion

We now proceed to evaluate the surface streamlines about a spheroid aligned with the axis of an axisymmetric straining flow. This configuration corresponds to the mean flow field about a spinning spheroid. In the body frame, the velocity gradient tensor is a diagonal matrix whose elements are ${\mathsf{A}}_{11}/2 = -{\mathsf{A}}_{22} = -{\mathsf{A}}_{33} = {\mathsf{E}}_3$. Likewise, the surface velocity gradient tensor $\boldsymbol{\Phi}$ is also a diagonal matrix with $\varPhi _{11}/2 = -\varPhi _{22} = -\varPhi _{33} = \beta E_3/2$, where the geometry-dependent prefactor $\beta$ is given by

(3.19)\begin{equation} \frac{1}{\beta} = \frac{3}{4} \int_{0}^{\infty} \frac{ac^2 t}{(a^2+t)^{3/2}(c^2+t)^2}\, \mathrm{d}t. \end{equation}

For this configuration, the surface streamlines are axisymmetric, originating at the ‘pole’ and terminating at the ‘equator’. Therefore, we can use an ellipsoidal polar coordinate system to describe the surface, identifying $\eta$ with the polar angle between the symmetry axis and a point on the surface and $\zeta$ with the azimuthal angle. We parametrise a point near the surface as

(3.20)\begin{equation} \boldsymbol{x} = \begin{bmatrix} a\cos\eta \\ c\sin\eta\cos\zeta \\ c\sin\eta\sin\zeta \end{bmatrix} +\xi\boldsymbol{h}_\xi, \end{equation}

so that the covariant coordinate vectors at the surface are

(3.21a–c)\begin{equation} \boldsymbol{h}_\xi = \frac{1}{h_\xi} \begin{bmatrix} c\cos\eta \\ a\sin\eta \cos\zeta \\ a\sin\eta \sin\zeta\end{bmatrix} ,\quad \boldsymbol{h}_\eta = \begin{bmatrix} -a \sin\eta \\ c\cos\eta \cos\zeta \\ c\cos\eta \sin\zeta \end{bmatrix}, \quad \boldsymbol{h}_\zeta = \begin{bmatrix} 0 \\ -c\sin\eta \sin\zeta \\ +c\sin\eta \cos\zeta \end{bmatrix}, \end{equation}

with $h_\xi$ chosen to ensure that $\boldsymbol {h}_\xi$ is a unit vector. Then it follows that

(3.22a,b)\begin{equation} u^\zeta = 0, \quad u^\eta = \frac{3}{2} \xi |\varPhi_{11}| \frac{ac \cos\eta\sin\eta}{(a^2\sin^2\eta + c^2\cos^2\eta)^{3/2}} = F\xi, \end{equation}

as required and

(3.23)\begin{equation} \rho = c \sin\eta(a^2 \sin^2\eta + c^2\cos^2\eta)^{1/2}. \end{equation}

Substituting (3.22a,b) and (3.23) into (2.24), we obtain

(3.24)\begin{align} \int_{\eta_0}^{\eta_1} {\rho}^{3/2}{F}^{1/2}\, \mathrm{d}\eta &= \int_{0}^{{\rm \pi}/2} \left( \frac{3}{2}\beta |{E}_{3}| {a}{c}^4 \cos\eta \sin^4\eta \right)^{1/2}\mathrm{d}\eta \nonumber\\ &= \left(\frac{{\rm \pi} {a}{c}^4 \beta |{E}_{3}|}{6}\right)^{1/2} \frac{\varGamma(\frac{7}{4})}{\varGamma(\frac{9}{4})}, \end{align}

and thus

(3.25)\begin{align} {Sh} &= 0.566 ({a}{c}^4 \beta)^{1/3} |E_3|^{1/3} {Pe}^{1/3} \nonumber\\ &= \alpha_{||}\left(\frac{|E_3|^* r}{\kappa}\right)^{1/3}, \end{align}

where $\alpha _{||}(\lambda ) = 0.566 ({a}{c}^4 \beta )^{1/3}$ represents the dependence of the surface flux upon geometry and $|E_3|^*r/\kappa$ is the Péclet number based on the strain perceived along the axis of rotation.

The geometry-dependent prefactor $\alpha _{||}$ has a relatively weak dependence upon the aspect ratio of the spheroid, varying between $0.762$ to $1.042$ over the interval $1/20 \le \lambda \le 20$. In contrast, from the definition of the characteristic shear rate $E^*$, $|E_3|$ may vary over the interval $0 < |E_3| \le 2/\sqrt {6}$, depending on the particular configuration of the background strain and the axis of the particle. Therefore, the alignment of the particle with the background velocity gradient plays a significant role in determining the surface flux for spinning particles. This is the phenomenon of the partial suppression of convection by rotation first identified by Batchelor (Reference Batchelor1979).

Some caution must be taken in utilising the result of (3.25). In our derivation of (2.24), we have assumed that the boundary layer thickness remains small in comparison to radius of curvature of the surface, so that cross-surface diffusion and higher-order convection terms are negligible. Yet, when the body is made infinitely slender, this assumption is violated. We expect that higher-order corrections to (2.24) are required for slender bodies at moderate Péclet number.

3.4. Surface flux under tumbling and resting motion

Under tumbling and resting motion, convenient expressions for the surface streamlines are no longer easy to find by hand. To proceed in this general case, we adopt a numerical approach to parametrise the surface in terms of coordinates $\boldsymbol {x} = \boldsymbol {x}(0, \eta , \zeta )$. Essentially, the task is to draw a set of $j = 1 \ldots n_\zeta$ surface streamlines covering the body, label each streamline with a unique $\zeta = \zeta _j$ and evaluate the position at $i = 1 \ldots n_\eta$ different locations $\eta = \eta _i$ along the streamline. Then we can create a $n_\eta \times n_\zeta$ mesh of points $\boldsymbol {x}_{i,j} = \boldsymbol {x}(0,\eta _i,\zeta _j)$ upon the surface to numerically approximate the metric $\rho$, which can be used to numerically integrate (2.24).

We shall now construct a suitable definition of the streamwise coordinate $\eta$. We require the surface streamlines be tangent to the surface velocity gradient $\boldsymbol {w}$ (3.15), so $\boldsymbol {h}_\eta$ must be of the form

(3.26)\begin{equation} \boldsymbol{h}_\eta = \frac{\mathrm{d}\boldsymbol{x}}{\mathrm{d}\eta} = \frac{\boldsymbol{w}}{\boldsymbol{w}\boldsymbol{\cdot} \boldsymbol{\nabla} \eta}, \end{equation}

which has $\boldsymbol {\nabla } \eta \boldsymbol {\cdot } \boldsymbol {h}_\eta = 1$ and $\boldsymbol {h}_\eta \boldsymbol {\cdot } \boldsymbol {h}_\xi = 0$, as required. Furthermore, we require that $\eta$ should increase monotonically along surface streamlines. We have seen in § 3.2 that the surface potential $\phi$ has this property. Therefore, we identify $\phi$ (3.17) with the streamwise coordinate $\eta$.

We require a definition of the $\zeta$ coordinate. Since $\zeta$ is constant along surface streamlines and every surface streamline passes through $\eta = \phi _2$, $\zeta$ can be thought of as a coordinate along the curve $\boldsymbol {x}_0(\zeta ) = \boldsymbol {x}(0, \phi _2, \zeta )$. Along $\eta = \phi _2$, from (3.17) we derive that the unit surface normal satisfies

(3.27)\begin{equation} \boldsymbol{h}_\xi\boldsymbol{\cdot} \boldsymbol{q}_1 \pm \sqrt{\frac{\phi_2 - \phi_3}{\phi_2 - \phi_1}} (\boldsymbol{h}_\xi\boldsymbol{\cdot} \boldsymbol{q}_3) = 0, \end{equation}

so the constraint

(3.28)\begin{equation} \zeta = \boldsymbol{h}_\xi \boldsymbol{\cdot} \boldsymbol{q}_2, \end{equation}

describes a point along $\boldsymbol {x}_0(\zeta )$. The surface can be split into four quadrants, depending upon the basin of attraction of the surface streamlines. To wit, the behaviour in the limits $\boldsymbol {h}_\xi \rightarrow \pm \boldsymbol {q}_1$ as $\eta \rightarrow \phi _1$ and $\boldsymbol {h}_\xi \rightarrow \pm \boldsymbol {q}_3$ as $\eta \rightarrow \phi _3$ forms our classification. Therefore, in each quadrant, the coordinates $(\eta ,\zeta ) \in [\phi _1, \phi _3] \times [-1, 1]$ uniquely define a point on the surface. This definition is general for torque-free, tri-axial ellipsoids.

We now outline the procedure to evaluate (2.24) numerically. For each surface quadrant, we choose a set of points $\boldsymbol {x}_{0,j} = \boldsymbol {x}(0, \phi _2, \zeta _j)$ which lie on the ellipsoid surface $\xi = 0$ and satisfy $\eta (\boldsymbol {x}) = \phi _2$ (3.17). We numerically integrate (3.26) from the initial condition $\boldsymbol {x}=\boldsymbol {x}_{0,i}$ at $\eta = \phi _2$ to $\eta = \eta _j$, which yields a mesh of points $\boldsymbol {x}_{i,j} = \boldsymbol {x}(0,\eta _i,\zeta _j)$ upon the particle surface. Measuring the surface area $\delta {\mathsf{S}}_{ij}$ of the region enclosed over $[\eta _i,\eta _{i+1}] \times [\zeta _i,\zeta _{i+1}]$, we approximate the surface area density for this surface element as

(3.29)\begin{equation} \rho_{ij} \approx \delta {\mathsf{S}}_{ij} (\eta_{i+1}-\eta_i)(\zeta_{i+1}-\zeta_i), \end{equation}

which is, roughly speaking, a ‘cell average’ of $\rho$. The velocity component $F$ (2.8) is evaluated at $\boldsymbol {x}_{i,j}$ from (3.17) and (3.15). Then, the integral (2.24) is evaluated as a Riemann sum over the surface elements.

A technical point remains that $\eta _i$ and $\zeta _j$ should be chosen so that the surface is densely covered in mesh points $\boldsymbol {x}_{i,j}$. To achieve this, we generate a uniform sampling of seed points on the surface. These seed points can be integrated (3.26) numerically towards the curve $\boldsymbol {x}_0$ to construct $\zeta _j$. This guarantees a satisfactory coverage of the surface by the streamlines. The $\eta _i$ can be chosen as

(3.30)\begin{equation} \eta_i = \begin{cases} \phi_1 \cos^2\nu_i + \phi_2 \sin^2\nu_i & \text{ if } \nu_i < 0 \\ \phi_2 \cos^2\nu_i + \phi_3 \sin^2\nu_i & \text{ if } \nu_i > 0 \end{cases}, \end{equation}

for $\nu _i$ evenly distributed on the interval $[-{\rm \pi} /2,{\rm \pi} /2]$.

3.5. Surface flux in rotation-dominated flow

It is useful to consider the special case $|\boldsymbol {\omega }|\rightarrow \infty$ where the vorticity is large and vortex stretching is non-zero ($\boldsymbol {\omega }^\textrm {T}\boldsymbol{\mathsf{E}}\boldsymbol {\omega } \ne 0$). In this case, it can be shown that the eigenvalues of $\boldsymbol{\mathsf{K}}$ are complex, its eigenvectors lie parallel and perpendicular to the direction of the vorticity $\hat {\boldsymbol {\omega }} = \boldsymbol {\omega }/|\boldsymbol {\omega }|$ and the particle rotates with constant angular velocity $\boldsymbol {\varOmega } \rightarrow \boldsymbol {\omega }/2$. Therefore, the motion either corresponds to case 2a (spinning) or case 2b (tumbling). In the spinning case, the particle rotates with its symmetry axis parallel to the vorticity vector $\boldsymbol {p} = \hat {\boldsymbol {\omega }}$. In the tumbling case, the particle rotates with its symmetry axis always orthogonal to the vorticity vector, e.g. $\boldsymbol {r} = \hat {\boldsymbol {\omega }}$. The motion of the body frame is therefore analogous to (3.8a–c).

The configuration can be inferred from the exact eigenvalue relationship

(3.31)\begin{equation} \lambda_1 \lambda_2 \lambda_3 ={-}2\sigma(\sigma^2 + \omega^2) = \frac{\gamma^3}{3}\textrm{tr}(\boldsymbol{\mathsf{E}}^3) + \frac{\gamma}{4} \boldsymbol{\omega}^\textrm{T}\boldsymbol{\mathsf{E}}\boldsymbol{\omega}, \end{equation}

where $\gamma = (\lambda ^2-1)/(\lambda ^2+1)$ is the shape co-factor. In the limit $|\boldsymbol {\omega }|\rightarrow \infty$, $\sigma \rightarrow -\gamma E_\omega /2$, where $E_{\omega } = \hat {\boldsymbol {\omega }}^\textrm {T} \boldsymbol{\mathsf{E}} \hat {\boldsymbol {\omega }}$ is the strain rate perceived in the direction of vorticity. Therefore, following § 3.1, we identify that the particle is aligned in the parallel configuration when $\gamma E_\omega > 0$ and the orthogonal configuration when $\gamma E_\omega < 0$. It follows that, as in (3.9), the average perceived velocity gradient is

(3.32)\begin{gather} \overline{\boldsymbol{\mathsf{A}}} = E_{\omega} \begin{bmatrix} 1 & 0 & 0 \\ 0 & -\frac{1}{2} & 0 \\ 0 & 0 & -\frac{1}{2} \end{bmatrix}\text{ when } \gamma E_\omega > 0 \textrm{ or } E_{\omega} \begin{bmatrix} -\frac{1}{2} & 0 & 0 \\ 0 & -\frac{1}{2} & 0 \\ 0 & 0 & 1 \end{bmatrix} \textrm{ when } \gamma E_\omega < 0. \end{gather}

In both cases, the average perceived velocity gradient is an axisymmetric strain. However, the alignment of the symmetry axis of the spheroid with this strain depends upon the sign of the shape co-factor and vortex stretching. As a result, we evaluate the surface flux as

(3.33)\begin{equation} {Sh} = \left\{\begin{matrix} \alpha_{||} {Pe}_{\omega}^{1/3} & \gamma E_\omega > 0 \\ \alpha_{{\perp}} {Pe}_{\omega}^{1/3} & \gamma E_\omega < 0 \end{matrix}\right. , \end{equation}

where ${Pe}_{\omega } = E_\omega ^* r/ \kappa$ is the Péclet number based on the vortex stretching, $\alpha _{||}(\lambda )$ is given by (3.25) and $\alpha _\perp (\lambda )$ is obtained using the numerical procedure outlined in § 3.4.

We have plotted the geometry-dependent prefactors $\alpha _{||}$ and $\alpha _{\perp }$ in figure 3. The marker shows Batchelor's result ${Sh} = 0.968 {Pe}_\omega ^{1/3}$ for the case of a sphere in rotation-dominated flow (Batchelor Reference Batchelor1979). We observe that, for the parallel-aligned configuration $\alpha _{||}$, the variation in the prefactor with $\lambda$ is relatively modest, corresponding to a variation in the surface flux of between $-21.4\,\%$ and $+7.7\,\%$ relative to that of a sphere with equivalent surface area. In contrast, there is a stronger variation observed for the orthogonal configuration $\alpha _{\perp }$, which exhibits an equivalent variation of $-10.5\,\%$ to $+53\,\%$ over the range shown. From (3.33), we see that the surface flux is proportional to the lower branches of the two black curves in vortex stretching $E_\omega > 0$ and the upper branches in vortex compression $E_\omega < 0$. It follows that the sign of the vortex stretching can influence the surface flux. In particular, the surface flux to prolate spheroids is significantly increased under vortex compression.

Figure 3.

Variation in the mass transfer coefficient of a spheroid of varying aspect ratio but constant surface area in axisymmetric straining flow (black lines) and uniform flow (blue line). The black circle shows Batchelor's result for a sphere in axisymmetric strain (Batchelor Reference Batchelor1979), whilst the black diamond shows the equivalent result for a sphere in uniform flow (Acrivos & Taylor Reference Acrivos and Taylor1962).

The shape dependence for spheroids in axisymmetric strain may be contrasted to the shape dependence observed for axisymmetric, uniform flow around a fixed spheroid shown in figure 3 (Acrivos & Taylor Reference Acrivos and Taylor1962; Sehlin Reference Sehlin1969; Dehdashti & Masoud Reference Dehdashti and Masoud2020). Here, the surface flux exhibits the same scaling ${Sh} = \alpha _U {Pe}_U^{1/3} + O(1)$, where ${Pe}_U=U_\infty ^* r/\kappa$ and $U_\infty ^*$ is the magnitude of the relative velocity (slip velocity) between the free stream and particle. Whilst it is of limited value to compare the absolute values of $\alpha$, some insight can be obtained by comparing the relative variation of each function. We observe that for a spherical particle with fixed translation velocity and surface area, flattening or elongating the particle results in a reduction in the surface flux. Likewise, for a spherical particle in rotation-dominated vortex stretching, flattening or elongating the particle also reduces the surface flux. However, in rotation-dominated vortex compression, flattening or elongating increases the surface flux. This observation is relevant to chain formation by marine diatoms, where each cell in a chain must experience an increased nutrient flux per unit area to benefit despite increased competition for nutrients by its neighbours (Pahlow et al. Reference Pahlow, Riebesell and Wolf-Gladrow1997).

One may also observe that rotation-dominated straining flow becomes considerably more effective than uniform flow at transferring solute from the particle surface at large aspect ratios. Of course, this result must depend upon the relative orientation of the free stream and particle axis, which is not varied here. Nonetheless, similar comparisons have found utility in determining when sinking or swimming may become a useful strategy for phytoplankton to increase their nutrient flux in turbulent water (Karp-Boss et al. Reference Karp-Boss, Boss and Jumars1996).

3.6. Further extensions

Two further generalisations of the surface coordinate system are to cases with non-zero body forces and torques. This would be necessary, for instance, to capture gyrotactic effects in the nutrient uptake of phytoplankton (Guasto et al. Reference Guasto, Rusconi and Stocker2012) or the behaviour of inertial particles. Such an extension can be accommodated by a suitable modification of the surface coordinate system, e.g. the inclusion of a body torque adds a skew–symmetric component to $\boldsymbol{\Phi}$ in (3.15). However, in this case, one would also expect the orientation dynamics (and therefore the mean flow around the particle) to change, which would also affect the mean surface flux via the convection suppression effect.