Non-existence of mean-field models for particle orientations in suspensions Richard M. Höfer1 Amina Mecherbet1 and Richard Schubert2

2025-05-02 0 0 681.25KB 18 页 10玖币
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Non-existence of mean-field models for particle
orientations in suspensions
Richard M. Höfer1, Amina Mecherbet1, and Richard Schubert2
1Institut de Mathématiques de Jussieu – Paris Rive Gauche, Université Paris Cité, France
2Institute for Applied Mathematics, University of Bonn, Germany
October 28, 2022
Abstract
We consider a suspension of spherical inertialess particles in a Stokes flow on the torus
T3
. The
particles perturb a linear extensional flow due to their rigidity constraint. Due to the singular
nature of this perturbation, no mean-field limit for the behavior of the particle orientation can
be valid. This contrasts with widely used models in the literature such as the FENE and Doi
models and similar models for active suspensions. The proof of this result is based on the study
of the mobility problem of a single particle in a non-cubic torus, which we prove to exhibit a
nontrivial coupling between the angular velocity and a prescribed strain.
1 Introduction
It is well known that inertialess rigid particles suspended in a fluid change the rheological properties
of the fluid flow. For passive non-Brownian particles this accounts to an increased viscous stress.
In more complex models like active (self-propelled) particles or non-spherical Brownian particles,
an additional active or elastic stress arises that renders the fluid viscoelastic. Over the last years,
considerable effort has been invested into the rigorous derivation of effective models for suspensions.
This has been quite successful regarding the derivation of effective fluid equations in models when
only a snapshot in time is studied for a prescribed particle configuration or for certain toy models
that do not take into account the effects of the fluid on the particle evolution (see e.g. [HM12;NS20;
HW20;GH20;GM22;DG20;GH21;DG21;Gir22;HLM22]).
Much less is known regarding the rigorous derivation of fully coupled models between the fluid
and dispersed phase, although a number of such models have been proposed a long time ago and
some of them have been studied extensively in the mathematical literature. These models typically
consist of a transport or Fokker-Planck type equation for the particle density coupled to a fluid
equation incorporating the effective rheological properties.
The rigorous derivation of such models is so far limited to sedimenting spherical particles where
the transport-Stokes system has been established in [Höf18;Mec19] to leading order in the particle
hoefer@imj-prg.fr
mecherbet@imj-prg.fr
schubert@iam.uni-bonn.de
1
arXiv:2210.15382v1 [math.AP] 27 Oct 2022
volume fraction. This system reads
tρ+ (u+g)· ∇ρ= 0,
u+p=gρ, div u= 0,
where
ρ
(
t, x
)is the number density of particles,
gR3
is the constant gravitational acceleration.
Here, the gravity is dominating over the change of the rheological properties of the fluid, which only
appears as a correction to the next order in the particle volume fraction
φ
. More precisely, as was
shown in [HS21], a more accurate description is given by the system
tρ+ (u+g)· ∇ρ= 0,
div((2 + 5φρ)Du) + p=gρ, div u= 0,(1.1)
where Du = 1/2(u+ (u)T)denotes the symmetric gradient.
For non-spherical particles, the increase of viscous stress depends on the particle orientations (see
e.g. [HW20] for a rigorous result in the stationary case). Moreover, elastic stresses are observed for
non-spherical Brownian particles as well as active stresses for self-propelled particles, both depending
on the particle orientation. Therefore, it is necessary to consider models for the evolution of particle
densities
f
that include the particle orientation. In the simplest case of identical axisymmetric
particles, the particle orientation can be modeled by a single vector
ξS2
. The model corresponding
to (1.1) then reads
tf+ (u+g)· ∇f+ divξ1
2curl uξ+BPξDf= 0,
u+pdiv(φM[f]Du) = gρ, div u= 0.(1.2)
Here,
Pξ
denotes the orthogonal projection in
R3
to the subspace
ξ
and
B
is the Bretherton
number that depends only on the particle shape (
B
= 0 for spheres,
B
= 1 in the limit of very
elongated particles, see e.g. [Gra18, Section 3.8]). Moreover
M
[
f
]is a 4-th order tensor depending
on the particle shape and given in terms of moments of f.
A widely used model for Brownian suspensions of rod-like (Bretherton number B= 1) particles
at very small particle volume fraction
φ
is the so called Doi model (see e.g. [DE88;Con05;HO06;
LM07;Con+07;CM08;ZZ08;OT08;CS09;CS10;BT12;BT13;HT17;La19]) that reads (in the
absence of fluid inertia)
tf+ div(uf) + divξ(Pξxf ) = 1
Deξf+λ1
De divx((Id +ξξ)xf),
u+pdiv σ=h, div u= 0
σ=σv+σe=φM[f]Du +λ2φ
De ˆS2
(3ξξId)fdξ.
(1.3)
Here,
De
is the Deborah number,
λ1, λ2
are constants that depend on the particle shape and
h
is some given source term. Neglecting the effect of the fluid on the particles, the elastic stress
σe
in the Doi model has been recently derived in [HLM22]. There are very similar models for active
suspensions (the Doi-Saintillan-Shelley model) and flexible particles, most prominently the FENE
model. Well-posedness and behavior of solutions to such models have been studied for example in
[JLL02;JLL04;Jou+06;LL07;SS08b;SS08a;LL12;CL13;Mas13;Sai18;CDG22;AO22].
The main purpose of this paper is to draw attention to the limitations of such fully coupled
models like
(1.2)
and
(1.3)
regarding the modeling of the particle orientations through the term
2
divξ
(
Pξxf
)(respectively
divξ
((1
/
2
curl uξ
+
BPξD
)
f
)for
B6
= 1). This term derives from
the change of orientation for the particles according to the gradient of the fluid velocity. However,
at least partially, this fluid velocity is arising as a perturbation flow due to the presence of the
particles themselves that cause the viscous and elastic stresses
σv
and
σe
. These perturbations are
typically of order
φ
. On the microscopic level, the perturbed fluid velocity is very singular. More
precisely, to leading order, it behaves like the sum of stresslets. At the i-th particle, it is given by
upert
N(Xi)X
j6=i
Φ(XiXj) : Sj
where the sum runs over all particles
j
different from
i
,Φis the fundamental solution of the Stokes
equation and
Sj
are moments of stress induced at the
j
-th particle due to the rigidity constraint
(and possibly activeness or flexibility). Consequently, the change of orientation behaves like
˙
ξi=Pξ
iξi· ∇upert
N(Xi)Pξ
iξiX
j6=i
2Φ(XiXj) : Sj
As Φis homogeneous of degree
1, this behavior is too singular to expect the “naive” mean-field
limit to be true that would lead to the term
divξ
(
Pξxf
)(respectively
divξ
((1
/
2
curl uξ
+
BPξD
)
f
)for
B6
= 1) in the models
(1.2)
and
(1.3)
. These models therefore do not seem to
describe correctly the behavior of the particle orientations to first order in the particle volume
fraction
φ
. Instead, it seems necessary to include terms that depend on the 2-point correlation
function for an accurate description up to order φ.
This is reminiscent of the second order correction in
φ
of the effective viscous stress
σv
(see [GH20;
GM22;DG21]). For the evolution of the particle orientation, this phenomenon already appears at
the first order, since the particle orientations are only sensitive to the gradient of the fluid velocity.
In this paper, we will make these limitations rigorous for a toy model. More precisely, we consider
a model example in which we show the non-existence of any mean field model that incorporates the
change of orientations to the leading order in the perturbation field of the fluid. This model example
consists of a suspension of spherical particles in a background flow which is a linear extensional flow.
In a bounded domain R3, the problem would read
u+p= 0,div u= 0 in \SiBi,
u(x) = φ1Ax on ,
Du = 0 in SiBi,
ˆBi
σ[u]ndS=ˆBi
(xXi)σ[u]ndS= 0 for all 16i6N.
where
Bi
=
BR
(
Xi
)denote the spherical particles and
ASym0
(3) is a symmetric tracefree matrix.
The rescaling with the volume fraction
φ
=
NR3
is introduced in order to normalize the perturbation
fluid velocity field uper induced by the particles.
For mathematical convenience, we consider the analogous problem on the torus
T3
. We attach
(arbitrary) orientations
ξiS2
to the spheres and show that no mean-field limit can exist by proving
that for periodically arranged particles on
Z3
, the particles do not rotate at all, while for particles
arranged periodically on (2Z)×Z2, the particles do rotate with a fixed rate.
1.1 Statement of the main results
We will work on the toroidal domains
T= (R/Z)3,TL= (R/2LZ)3,¯
TL= (R/4LZ)×(R/2LZ)2.
3
Furthermore we set
B=B1(0), BR=BR(0),
and for definiteness
A=
0 1 0
1 0 0
0 0 0
.
Theorem 1.1.
For 0
< R <
1
/
2and Ω =
T1
or Ω =
¯
T1
, let
uH1
(Ω) be the unique weak solution
to the problem
u+p= 0,div u= 0 in \BR,
Du =Ain BR,
ˆ
udx= 0,
ˆBR
σ[u]ndS=ˆBR
xσ[u]ndS= 0.
(1.4)
(i) If Ω = T1, then curl u(0) = 0.
(ii) If Ω = ¯
T1. then there exists ¯c > 0such that
curl u(0) R3
16 ¯ce3
6CR4(1.5)
for a constant Cindependent of R.
Observe that the factor 16 in (1.5) corresponds to the volume of ¯
T1.
As a consequence of Theorem 1.1 we show the negative result stated in Corollary 1.2 below, that
we outlined in the introduction. We will use the following notation. For
NN
, which we think of
as the number of particles in a unit cell, we denote by
φ=NR3
the volume fraction of the particles. Both
R
and
φ
may implicitly depend on
N
. We will make this
dependence explicit by a subscript
N
wherever we feel it is necessary for clarity. For
R >
0and
NN, let XiT,16i6Nbe such that
dmin = min
i6=j|XiXj|>2R. (1.6)
This ensures that the balls
Bi=BR(Xi)
do not intersect nor touch each other. Moreover, for 1
6i6N
, let
ξ0
iS2
. The associated initial
empirical density f0
N∈ P(R3×S2)is given by
f0
N=1
NX
i
δXiδξ0
i.
4
摘要:

Non-existenceofmean-eldmodelsforparticleorientationsinsuspensionsRichardM.Höfer*1,AminaMecherbet„1,andRichardSchubert…21InstitutdeMathématiquesdeJussieuParisRiveGauche,UniversitéParisCité,France2InstituteforAppliedMathematics,UniversityofBonn,GermanyOctober28,2022AbstractWeconsiderasuspensionofsph...

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