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Mass and entropy transport in a suspension of rigid particles

D. Lhuillier

To cite this version:

D. Lhuillier. Mass and entropy transport in a suspension of rigid particles. Journal de Physique, 1986,

47 (10), pp.1687-1696. �10.1051/jphys:0198600470100168700�. �jpa-00210365�

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1687

Mass and entropy transport in a suspension of rigid particles

D. Lhuillier

Laboratoire de Mécanique Théorique (*), Université P. et M. Curie, 4 place Jussieu, 75230 Paris Cedex 05,

France

(Requ le 3 mars 1986, accepté le 26 juin 1986)

Résumé.

2014

En utilisant la thermodynamique des phénomènes irréversibles, on fait une analyse du transport de

masse et d’entropie dans une suspension. La méthode utilisée est une extension de celle appliquée par Einstein et Batchelor à l’étude de la diffusion brownienne. On montre que le couplage (dû aux relations de symétrie d’Onsager) qui existe pour un mélange à deux composants, subsiste encore pour une suspension, mais qu’il est

cette fois dû au rôle simultané joué dans les deux transports par la vitesse relative entre phases. Les résultats

les plus remarquables sont : i) l’absence d’effet Soret lié à la tension interfaciale si les particules suspendues

sont rigides ; ii) la dépendance du coefficient de diffusion avec les masses volumiques de chacune des phases ; iii) une forme correcte de la force de Coriolis agissant dans le mouvement relatif ; iv) la possibilité pour la diffusion de Faxen (diffusion dans les gradients de vitesse inhomogènes) de jouer un rôle important pour peu que la sédimentation soit négligeable.

Abstract.

-

Mass and entropy transport in a suspension are analysed in the framework of irreversible

thermodynamics. Our approach extends the one used by Einstein and Batchelor for the study of Brownian diffusion. We show that the well-known coupling (due to the Onsager symmetry relations) which occurs in a two-component mixture, also occurs in a two-phase suspension, as a consequence of the joint role played by

the relative velocity in mass and entropy transport. Most noticeable results are i) if the suspended particles are rigid, surface tension cannot lead to any thermo-diffusion (Soret effect) ; ii) the general expression for the

diffusion constant depends on the densities of the two phases ; iii) in a rotating suspension, the Coriolis force

acting on the relative motion is not the one commonly found in the literature and iv) diffusion by non- homogeneous velocity gradients (Faxen’s diffusion) may become important whenever sedimentation is

negligible.

J. Physique 47 (1986) 1687-1696 OCTOBRE 1986,

Classification

Physics Abstracts

05.60

-

47.55K

1. Introduction.

The transport properties of a suspension of particles

have recently received a lot of attention. These studies have dealt not only with momentum transport in shear flow but also with mass transport in relation with sedimentation [1, 2] and concentration diffusion

[3, 4]. At variance, the thermo-diffusion problem

has not yet received a definite answer. One knows

that in a two-component system (defined as one in

which the « particles » have atomic size), the mass

flux is coupled to the entropy flux. What remains of that coupling for a dispersed two-phase system in which each particle contains a lot of atoms ? It is the

purpose of this paper to give an answer for rigid particles, and to reconsider mass and entropy trans- port in suspensions with the help of irreversible

thermodynamics. Our chief aim is the study of

thermo-diffusion or Soret effect but, as we shall see,

our analysis also brings out new results concerning

(*) associ6 au CNRS, U.A. 229.

concentration diffusion as well as diffusion in rota-

ting systems.

2. Mass and entropy diffusion in a two-component mixture

Irreversible thermodynamics provides us with a description of mass and entropy diffusion in a multi- component mixture [5]. The main results in the case

of two components (labelled 1 and 2) are reminded

below.

When no chemical reaction occurs, the mass of each component is separately conserved, hence

where Vk is the mass-weighted average velocity of

component k. Defining the barycentric velocity V

and the mass p per unit volume of the mixture by

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198600470100168700

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the above equations can be rewritten as

where J is the mass diffusion flux defined as

The entropy S per unit volume of the mixture evolves according to

where is the entropy diffusion flux and 0’ is the entropy production which reads

In this expression, U k is the chemical potential of component k, and T is the mixture temperature. In the framework of (linear) irreversible thermodyna- mics, the condition of positive entropy production is

satisfied with

and

The Onsager symmetry principle implies

and imposes a coupling between J and X. A simple

dimensional analysis of the phenomenological coeffi-

cients L allows to rewrite the diffusive fluxes as

and

Here kT is the (positive) coefficient of thermal

conductivity, while 0 is another positive quantity

with the dimension of a time. The third coefficient

s has the dimension of a specific entropy. Its presence in both J and 1; is a consequence of the

Onsager symmetry but neither its sign nor magnitude

are restricted by thermodynamics.

3. Two-phase mixtures versus two-component mixtu-

res.

Consider a mixture which appears as particles of

component 1 surrounded by component 2. If the

smallest particles contain so many atoms that their

continuum-mechanical description is justified (parti-

cle size larger than 0.1 um approximately), one speaks of the mixture as a dispersed two-phase mixture ; on the other hand, if all particles are

reduced to atoms, one speaks of a two-component mixture, the description of which was given above.

The continuum description of a two-phase mixture

uses averages over small volumes containing many particles, while the description of a two-component mixture involves averages over tiny volumes contai-

ning many atoms. The main difference between the

dynamics of two-phase and two-component mixtures lies in the average relative velocity between species 1

and 2. In a two-phase mixture, the large size of the

particles allows for a long-lived relative velocity. In

other words, the relative velocity is raised to the status of a state variable : it appears in the Gibbs relation and obeys an equation of motion.

4. Mass and entropy diffusion in a simple two-phase

mixture.

In a two-phase mixture the mass conservation is

expressed with equations similar to (1), i.e. it has

exactly the same form as for a two-component mixture. In particular, the mass diffusion flux is still

given by (2). The only difference comes from the definition of V, and V2 which are now the mass- weighted averages over a volume containing many

particles.

The entropy equation must have the same form as

written in (3) since this equation stems from galilean

invariance only. Nevertheless, a more detailed expression for the entropy flux can be obtained if

one notices that the overall entropy flux of a two- phase mixture can be written as

where s gathers all the non-convective contributions

and sk stands for the specific entropy of phase k.

Writting this flux as the sum

where

one deduces the important result

Hence, a part of X is linked to the relative velocity

while the whole of J is proportional to it (cf. (2)).

As far as mass and entropy equations are concer-

ned, the differences between a two-component and a

two-phase mixture are not very striking. We now

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1689

analyse more specific features of a two-phase mix-

ture, namely the evolution equation for the relative

velocity and the expression of the Gibbs relation.

The evolution in time of the relative velocity

is described by a Galilean-invariant equation

where F and R are the yet unknown force and stress

acting in the relative motion while p* is the related inertia defined as

where flk;n is the average kinetic energy of the mixture. The above equation (9) was recently studied

in the case of extremely high Reynolds numbers, Le.

when the flow around each particle may be approxi-

mated by the Euler equation [6]. Here we are

interested in the opposite situation of very low relative Reynolds numbers, when the Stokes equa- tions are relevant and all inertia terms are negligible.

In this low - W regime, the average kinetic energy is

merely

and consequently

Hence, for low enough relative velocity, equation (9) is nothing but an evolution equation for the mass

diffusion flux J (such an equation was considered

earlier in the frame of extended thermodynamics [7]). We shall later determine the low-W expressions

for F and R.

The second important difference between a two-

phase and a two-component mixture is the Gibbs relation. From the « microscopic » Gibbs relation (i.e. the classical one, valid on a scale much smaller than the particle size) and the above expression for

the kinetic energy, one can get the so-called mesos-

copic relation or Gibbs relation averaged over a

volume containing many particles. With U;nt standing

for the average internal energy (and including the

kinetic energy of relative motion) one gets

where P k and Tk are the average pressure and

temperature of phase k, while ak is its volume fraction. Since particles and fluid occupy the whole available space

We shall henceforth suppose that the particles are rigid. disappear The ratio from the p 1 a set is then of independant constant and variables. a 1 must

This requires the mixture to be permanently in equilibrium regarding a 1 and this amounts to

or equivalently

This condition of rigidity is easy to understand since any difference between the average pressures would

ultimately lead to an expansion or contraction of the

particles [8] and break the rigidity assumption.

Besides rigidity we make a second assumption and

suppose that the average temperature of the particles

is always equal to the average temperature of the surrounding fluid. This implies that the rate of change of the liquid temperature in the particles

frame is always much smaller than the characteristic time for heat exchanges, i. e.

where vTl stands for the thermal diffusivity of the particles while a is the particle size.

The two above assumptions are rewritten as

and

where P and T are henceforth referred to as the pressure and temperature of the mixture.

For a suspension of rigid particles with high enough heat factor VT1/ a2, the Gibbs relation is thus

simplified from (11) to

where the overall entropy S was already defined in

(7). Combining the above Gibbs relation with the

evolution equations, one gets the following entropy

production :

(5)

Let us report to § 9 the discussion concerning the R : VW and viscous dissipation terms. Compared to (4) it

looks as if an extra term linked to W has appeared. But W cannot play simultaneously the role of a

thermodynamic force and the role of a flux (remember the W-dependence of J and I exhibited in (2) and (8)). In fact, one must gather all the W-dependent terms and the above entropy production must be

rewritten as

It will be positive provided

and

where kT is the thermal conductivity of the suspension and 0 the relaxation time of the relative velocity

motion. If we now suppose that inertia in relative motion is negligible, and that the role of R is temporarily neglected (cf. § 9), equation (9) amounts to

And from (2), (8) and (13) one gets for the diffusion fluxes

and

These expressions are quite similar to the expressions (5) and (6) for a two-component mixture. However,

we now interpret 0 as the relaxation time for the relative velocity and we get for s the simple interpre-

tation

But while the presence of s in both (5) and (6) was a

consequence of the Onsager symmetry, the presence

of sl - s2 in both (15) and (16) is a consequence of the joint role of the relative velocity in the mass and entropy transport. We can go further by noticing

that the Gibbs-Duhem relation for the pure phase k

reads

where p 2 is the mass per unit volume of pure phase k, i.e.

Since both phases have locally thd same pressure and

temperature one finds

which means that the diffusive mass flux (15) is proportional to the pressure gradient only. In other words, mass diffusion is reduced to a baro-diffusion.

Sedimentation is nothing but a special case corres-

ponding to a hydrostatic pressure field

and accordingly

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1691

It is clear that the relaxation time depends on the particle volume fraction. To agree with Batchelor’s notation we now write

The interpretation of K ( a,) is readily got: if

sedimentation occurs with no net volume flux, i.e. if

then, combining (21) and (22), one sees that the particles fall (or rise) with a velocity

where

is the single particle falling (or rising) speed.

Let us stress that (15) and (19) imply the absence of any Soret effect (dependence of J on VT) or

concentration-diffusion (dependence of J on V « 1).

One could suggest that this is due to our neglect of

surface tension between the two components, and to

our neglect of the configuration entropy of the

particles. Let us examine these two points successi- vely.

5. Influence of surface tension

In a two-component mixture the difference of inte- ractions between the couples of atoms 1-1, 2-2 and 1-

2 manifests itself as an energy of mixing. In the

continuum description of a two-phase mixture, the

same phenomenon is taken into account in a slightly

different way: one says that the particles interact

with the surrounding fluid through short-range forces

that can be accounted for with a surface energy y

depending on the mean temperature Ti of the

interface. If ai i stands for the amount of interface per unit volume of the mixture, the thermodynamic

relations of the interface between components 1 and 2 are

and

where Ui and Si are the internal energy and entropy of the interfaces per unit volume of the mixture.

According to our previous assumptions, the ave-

rage temperature Ti cannot be different from the

common average temperature of the two compo- nents, hence

Moreover, if the particles are spheres of radius a and with a constant mass, we have

and

In this case a is completely determined by pi and

aI’ and it is not hard to see that the above

thermodynamic relations can be rewritten as

and

Everything appears as if the particles « dressed » by

surface tension could be considered as « bare »

particles with a chemical potential

instead of and a pressure

instead of

Moreover, the interface entropy stemming from the

surface tension is obviously convected with the parti-

cles and the diffusive entropy flux now appears as

instead of (8). Thus, when surface tension is taken into account, the specific entropy of the particles

becomes

instead of

As a consequence, the thermodynamic force that will enter the mass diffusion flux is no more (19) but

According to the Gibbs-Duhem relations (18) and (24) this force is

But the assumption of rigid particles now implies

instead of

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The average pressure P of the mixture is thus

and the mass diffusion flux is, as in the case of bare

particles, proportional to the gradient of pressure

only. At first sight it is rather surprising that surface

tension does not lead to any Soret effect. This is due to the mutual cancellation of two VT forces. The first comes from the gradient of chemical potential

and is the one most frequently invoked in the

literature. The second one comes from the transport of the interface entropy by the particles and seems to

have been overlooked up to now. The sum of these two forces amounts to a gradient of pressure, V ( 2 y /a ) . But if one takes into account the relation (27) between pressures which is a conse- quence of the rigidity assumption, the resulting force

is exactly the same as for particles without surface tension. The absence of Soret effect is thus clearly

associated with the rigidity of the particles. Since the thermodynamic description of a suspension with

deformable particles is much more involved, we postpone it to a forthcoming paper.

6. The entropy of configuration.

In a two-component mixture, a part of the total entropy is due to the many microstates having the

same average concentration, but differing from each

other by the spatial distribution of the two chemical

species. A suspension also has a configuration

entropy, but linked to the particles instead of the atoms, and defined as the logarithm of the number of different spatial configurations compatible with a given volume fraction. It vanishes not only for zero particle concentration but also when the particles are closed-packed since only one configuration is possi-

ble in that case.

Let us call AS the configuration entropy per unit volume of the mixture. To AS corresponds an excess

free enthalpy

Any correct expression for AG must satisfy the well-

known extensivity requirement

where Att k is the excess chemical potential. Since

the number of different configurations cannot depend on the pressure or the temperature but only

on the number of particles and on their volume

fraction, the only way to write AS in a form

compatible with (28) is

where f and 9 are two functions of the volume fraction. Hence, the excess chemical potentials asso-

ciated with the configuration entropy take the special

form

and

Besides (29), the configuration entropy must also satisfy a second property, namely

To see what it means, we combine (29) and (31) to

get

which, for a constant temperature, implies

This is nothing but a condition of no net force acting

on the mixture, as was written in a slightly different

form in equation (3.13) of [3]. Thus (31) means that

the configuration entropy plays no role in the barycentric motion of the mixture. But as we shall

soon see, it plays a prominent role in the relative motion and hence in diffusion. Before considering

that matter in more detail, let us establish a relation

that will be useful later on ; from (30) and (32)

follows

where

is the excess chemical potential per particle of mass

ml

=

4,7r a p 1/3. It may be helpful at this point to

have explicit expressions for f and 9. In principle,

the configuration entropy of a suspension can be

deduced from the entropy of a hard-sphere liquid.

The problem is that no analytical expression for that entropy has yet been found in the whole range 0 a, - a m, where a. is the close-packed volume

fraction. Nevertheless, two limiting situations have

been thoroughly investigated :

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1693

1) the dilute limit (a, a.) where the virial

expension method (cf [3] and references therein)

leads to

where kB is the Boltzmann constant.

2) the high-density limit (al c= a m where the analog of the virial series is an expansion in the relative free volume [9] with the result

The factor 3 in the above results must be replaced by D in a D-dimensional space.

Besides these exact results, one can also get an approximate expression for AS with the so-called lattice model in which the whole available space is divided into cells that can be occupied by one particle .at most.

The resulting expression for AS, supposed to be valid whatever is the concentration appears as

where nl is the number of particles per unit volume and nm its maximum value. This result can be transformed into a form similar to (29) with

The lattice-model expression for AS gives exact results for a one-dimensional space only. For our three-

dimensional space the lattice-model results for dilute and concentrated suspensions are a bit different from

the exact hard-sphere results. Anyway, the lattice model has the merit of giving easily a not so bad expression of the configuration entropy for arbitrary concentrations.

7. Role of configuration entropy in mass and entropy transport.

The entropy of the whole mixture is no longer (7) but

and the only modification brought to the Gibbs relation (12) is the replacement of ILk by ILk + 4ILk. A

second important modification concerns the entropy transport and is linked to the velocity with which the

configuration entropy is convected. Among the possible assumptions, there is only one which leads to sound

consequences : we shall suppose that the part of AS proportional to pl (resp. P 2) moves with V, (resp. V2).

This means that the overall entropy flux is now

where we made use of the property (29). As a consequence, the diffusive part of the entropy flux is now

instead of (8). Taking into account the above modifications brought by the configuration entropy to the

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chemical potentials and to the entropy transport, the force acting in the relative motion is no longer (13) but

If we again neglect inertia in relative motion and take result (30) into account we deduce

It is thus clear that the configuration entropy is responsible for the concentration dependent part of J. But again there is not Soret effect, due to the

mutual cancellation of two VT forces. This cancella- tion comes from the proportionality of the excess

chemical potentials J1¡.L and J1¡.L 2 with the tempera- ture, cf. (30). For particles interacting with each

other through long-range forces, the configuration

entropy will be replaced by a configuration free

energy that will depend non linearly on the tempera-

ture. In this case one can expect a Soret effect even

for rigid particles.

The usual definition of the diffusion coefficient D is

Comparing with (35) and taking (33) into account,

we get the remarkably simple result, similar to Einstein’s for Brownian diffusion.

If we now consider the expression for the relaxation time given in (22) together with the definition (33) of

the excess chemical potential per particle, we can.

rewrite the diffusion coefficient as

At first sight, the P 2 0 p factor seems to contradict

Batchelor’s result (6.5) in [3]. In fact Batchelor’s definition of the diffusion constant refers to the

special case of batch sedimentation for which (23)

holds and consequently

Hence, for batch sedimentation, the effective diffu-

sion constant is

and we recover Batchelor’s result. Anyway, the general expression is (36) or (37) and expression (38)

is restricted to a particular (although important)

case.

By the way, let us comment on a statement made

by Batchelor in [3]. In this fundamental paper it is said that a force per unit volume acting on fluid and particles alike produces no relative motion. This statement is obviously in error since only a force per unit mass acting on fluid and particles alike has that property (think of gravity for instance). If the

external forces per unit mass were different, say g, and g2, the right-hand side of (9) would have been modified into

and a part of J would have been proportional to

g, - g2. As a result Batchelor’s proposal (3.14) for

the effective force on a particle should be written as

and not

It happens that the missing factor p0 compensates

for the p2/p factor linking Db and D, and the final

result got by Batchelor for Db is correct.

8. Intluence of rotation.

When written in a frame rotating with angular velocity n relative to a Galilean frame, the equation (9) for the relative velocity is transformed into

And when neglecting both inertia and the role of R, this equation merges into

when (10) is taken into account. We deduce from

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1695

(13) and (19) that the relative velocity is now given by

with 6 given in (22). And if we also neglect inertia

and viscous shear stress in the overall momentum

equation, we get

where V is the barycentric velocity. A settling

process in a rotating system involves the solution of

(39) and (40) compatible with the two mass conserva-

tion equations [2]. Notice that the so-called Coriolis force is 2 ft x V for the « true » velocity V, but that it is Q x W for a relative (i. e. Galilean-invariant) velocity, and not 2 n x W as often found in the literature.

9. Faxen’s diffusion.

It is worth noticing that another kind of mass

diffusion is possible in a suspension, namely what

can be called Faxen’s diffusion : it results from the relative motion imposed on a particle moving in a non-homogeneous velocity gradient. Faxen’s result for an isolated particle can be written with our

notations as

and it is possible to propose a generalisation of this

result to non-dilute suspensions, again with the help

of irreversible thermodynamics.

-To do this, we notice that when the stress

R is taken into account, the entropy production

involves a R : V W term and because of a thermody-

namic coupling with the V V force occurring in the

viscous dissipation term, we can write

where 17 2 is the carrier fluid viscosity while m and n

are two unknown functions of the volume fraction.

When inertia in relative motion may be neglected,

the former result (14) is transformed into

where F given in (13). If we notice that a continuum

description of the suspension implies

where a is the particle size, it is not difficult to

convince oneself that the V W part of R is always negligible as compared to F, and consequently (41)

amounts to

Extracting W from that equation, the mass diffusion

flux becomes

instead of (15). The new contribution to J is the non- dilute form of Faxen’s diffusion. From the expression (22) for 0 it is clear that this term is all the more

important than the particle size is larger, but cer- tainly requires the absence of any sedimentation

(i. e. Po

=

p) to be observed.

10. Conclusions.

If one may neglect inertia in relative motion, the general features of mass and entropy transport in suspensions are rather simple. Except for Faxen’s diffusion which is specific of large particles, the general form of the mass and entropy fluxes was

shown to be the same for a suspension and a two- component mixture. The Onsager symmetry mani- fests itself in a suspension as a consequence of the

joint role played by the relative velocity in both mass

and entropy transport. It was possible to conclude

that for a Soret effect to be observed, the particles

should be deformable or interact through long-range

forces (other than hydrodynamic forces). In particu- lar, there is no Soret effect in a suspension of rigid particles. We have also reconsidered the concentra- tion-diffusion in suspensions with the help of the so-

called configuration entropy, and we showed that the true diffusion constant depends on the particle

and fluid densities, a result that can prove important

for diffusion in flows with non-zero volume flux.

Lastly a new and correct expression was given for

the Coriolis force in the relative motion ; it remains

to find a situation where this term is not negligible !

Acknowledgments.

-

I would like to thank

D. Levesque and J. J. Weiss (LPTHE Orsay) for

helpful discussions on the hard-sphere liquid.

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References

[1] BATCHELOR, G. K., J. Fluid. Mech. 52 (1972) 245.

[2] SCHNEIDER, W., in Lecture Notes in Physics 235, Meier G. and Obermeier F. eds. (Springer- Verlag, Berlin) 1985, p. 326.

[3] BATCHELOR, G. K., J. Fluid Mech. 74 (1976) 1.

[4] RUSSEL, W. B., Ann. Rev. Fluid. Mech. 13 (1981) 425.

[5] LANDAU, L. and LIFCHITZ, E., Mécanique des fluides (Mir, Moscou) 1971, ch. 6.

[6] LHUILLIER, D., Int. J. Multiph. Flow 11 (1985) 427.

GEURST, J. A., Physica A 129 (1985) 233.

[7] MÜLLER, I., in Lecture Notes in Physics 199, J.

Casas-Vasquez, D. Jou and G. Lebon eds.

(Springer-Verlag, Berlin) 1984, p. 32.

[8] LHUILLIER, D., J. Physique 46 (1985) 1325.

[9] SALSBURG, Z. W. and WOOD, W. W., J. Chem. Phys.

37 (1962) 798.

ALDER, B. J., HOOVER, W. G. and YOUNG, D. A.,

J. Chem. Phys. 49 (1968) 3688.

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