Chemotaxis-fluid systems with logarithmic sensitivity and slow consumption global generalized solutions and eventual smoothness

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arXiv:2211.01019v1 [math.AP] 2 Nov 2022
Chemotaxis(-fluid) systems with logarithmic sensitivity
and slow consumption: global generalized solutions and
eventual smoothness
Mario Fuest
Leibniz Universität Hannover,
Institut für Angewandte Mathematik,
Welfengarten 1, 30167 Hannover, Germany
Abstract
We consider the system
nt+u· ∇n= ∆nχ∇ · (n
cc),
ct+u· ∇c= ∆cnf(c),
ut+ (u· ∇)u= ∆u+P+nφ, ∇ · u= 0,
in smooth bounded domains Ω RN,NN, for given f0, φand complemented with initial and
homogeneous Neumann–Neumann–Dirichlet boundary conditions, which models aerobic bacteria in a fluid
drop. We assume f(0) = 0 and f(0) = 0, that is, that fdecays slower than linearly near 0, and construct
global generalized solutions provided that either N= 2 or N > 2 and no fluid is present.
If additionally N= 2, we next prove that this solution eventually becomes smooth and stabilizes in the
large-time limit. We emphasize that these results require smallness neither of χnor of the initial data.
Key words: chemotaxis, fluid, logarithmic sensitivity, generalized solutions, eventual smoothness
AMS Classification (2020): 35K55 (primary); 35B40, 35B65, 35D99, 35Q35, 92C17 (secondary)
1 Introduction
This article is concerned with the chemotaxis–Navier–Stokes system with logarithmic sensitivity
nt+u· ∇n= ∆nχ∇ · (n
cc) in ×(0,),
ct+u· ∇c= ∆cnf(c) in ×(0,),
ut+ (u· ∇)u= ∆u+P+nφ, ∇ · u= 0 in ×(0,),
νn=νc= 0, u = 0 on ×(0,),
(n, c, u)(·,0) = (n0, c0, u0) in Ω,
(1.1)
e-mail: fuest@ifam.uni-hannover.de, corresponding author
1
variants of which have been proposed in [32] to model the behavior of aerobic bacteria interacting with a fluid by
means of transportation and buoyancy. Apart from random motion (term ∆n) the bacteria with density nmay
also partially orient their movement towards higher concentrations of oxygen with density c(term χ·(n
cc),
where χ > 0 is given), a mechanism called chemotaxis. The oxygen diffuses (term ∆c) and is consumed by
the bacteria (term nf (c), where fis a given nonnegative function) and both the bacteria and the oxygen
are transported by a fluid with velocity field u(terms +u· ∇nand +u· ∇c), which in turn is given by the
Navier–Stokes equation with an inhomogeneity accounting for buoyancy effects, i.e. the observation that water
with bacteria is heavier than without (term +nφ, where φis a given gravitational potential). The modelling
in [32] is motivated by experiments performed in [7]; for an alternative derivation of such systems based on a
multiscale approach see [1].
The mathematical analysis of such models has first focussed on variants with linear taxis sensitivity, i.e. with
χ·(n
cc) in the first equation replaced by χ·(nc), for which global classical [4] and weak solutions [8, 36]
have been constructed for small and large data, respectively. Beyond that, many more results on chemotaxis–
fluid systems (for instance also covering situations where the signal is produced rather than consumed) are
available; we refer to [2, Section 4.6] for a recent overview.
The reason behind considering a logarithmic sensitivity in (1.1) is to account for the so-called Weber–Fechner
law of stimulus perception, an idea already present in earlier models by Keller and Segel [18] (see also [29] and
[15, Section 2.2]).
From a mathematical point of view, the logarithmic sensitivity poses two main challenges: First, it destroys
the (quasi-) energy structure crucially made use of for instance in [8] and [36] inter alia for linear sensitivity
functions as cf(c) cannot be concave near c= 0 for nonnegative smooth fwith f(0) = 0 (cf. the discussion in
[8, p. 1638]). Second, the consumption term in the second equation in (1.1) may force cto become very small,
which means that the factor 1
cin the taxis term may become very large. In fact, even local-in-time positive
lower bounds for cappear to be unavailable without relying on (generally not available) upper bounds for n—in
contrast to logarithmic chemotaxis systems with signal production where even time-independent lower bounds
have been derived, see for instance [10, Lemma 2.2].
Even without fluid interaction, global classical solutions of (1.1) have only been constructed under smallness
conditions [35] or for related, more regular systems (in [20] with nonlinear diffusion enhancement, in [23] with
saturated taxis sensitivity, and in [21] with weaker consumption terms, i.e. for nf(c) replaced by nβcfor
some β(0,1)).
Main result I: Global generalized solutions. The lack of unconditional global existence results for classical
solutions is not entirely surprising. Systems including cross-diffusive terms such as χ·(n
cc) in (1.1) generally
have quite low regularity properties. Indeed, the probably most prominent representative of such models, the
classical Keller–Segel system
(nt= ∆n− ∇ · (nc),
ct= ∆cc+n
admits classical solutions blowing up in finite time in both two- [14, 26] and higher-dimensional [37] settings—as
do many variants of this system, see for instance [28] for blow-up in a parabolic–elliptic system with logarithmic
sensitivity and the recent survey [22] for further examples. This makes it necessary to consider weaker solution
concepts when studying global solvability of cross-diffusive systems and while sometimes switching to usual
weak formulations suffices, one often needs to consider even more general concepts; see [9, Section 1.2] for a
more thorough discussion of various notions of solvability.
Such generalized solutions have also been obtained for (1.1) with f(c) = cboth in the two-dimensional setting
with fluid ([24]; see also the precedents [33] for the chemotaxis–Stokes system, i.e. (1.1) without the nonlinear
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convection term (u· ∇)uin the fluid equation, and [40] for the fluid-free case) and higher dimensional fluid-free
radially symmetric settings ([43]).
Our first main result expands on these findings and states that (1.1) possesses global generalized solutions if
either N= 2 or if N3 and there is no fluid present, and if fdoes not only fulfill
fC1([0,)) with f(0) = 0 and f > 0 in (0,) (1.2)
but also
f(0) = 0.(1.3)
By (1.2), the condition (1.3) is equivalent to limsց0f(s)
s= 0; that is, (1.3) requires superlinear decay of fnear
0, which reflects that oxygen is consumed more slowly if nearly none is left. We remark that (1.3) is not fulfilled
for the most typical choice f(c) = cbut, for instance, for f(c) = c2.
Theorem 1.1. Let RN,N2, be a smooth, bounded domain, χ > 0and φW2,(Ω), and assume
(1.2),(1.3) and
n0L1(Ω) with n0>0a.e. and ln n0L1(Ω),
c0L(Ω) with c0δfor some δ > 0,
u0L2(Ω; RN)with ∇ · u0= 0 in D(Ω).
(1.4)
If
N= 2 or (u00and φ0),(1.5)
then there exists a global generalized solution (n, c, u)of (1.1) in the sense of Definition 3.1 below which has the
property that u0if u00and φ0.
The main novelty of Theorem 1.1 is the fluid-free higher dimensional case. Indeed, for χ= 1, more regular initial
data and f(c) = cthe two-dimensional setting with fluid has already been treated in [24] and the challenges
caused by large χ, less regular initial data and more general fare relatively limited. (In fact, the main reason
to include the two-dimensional existence result here is so that we can refer to it in Theorem 1.2 below.)
On the other hand, new ideas are necessary for N3. While quasi-energy functionals quickly give a priori
bounds for (weighted) gradients of all components of solutions to approximative systems (see Lemma 3.5 and
Lemma 3.6), they are only strong enough to imply uniform integrability of nεf(cε) in the two-dimensional
setting (where such an estimate follows for instance from Heihoff’s inequality [13, (1.2)]). However, such an
a priori estimate turns out to be crucial for undertaking the limit processes in the weak formulations for the
first and second solution components; see the discussion at the beginning of Subsection 3.4 for a more thorough
discussion of this point. One way to obtain uniform integrability of nε(and hence also of nεf(cε)) is to modify
the system by adding a superlinear degradation term to the first equation in (1.1). This observation stands as
the core of [9, Section 7], where recently global generalized solution for the corresponding problem have been
constructed (cf. also the precedent [19] for quadratic dampening terms).
However, as we aim to prove a global existence result for (1.1) without any dampening terms and also for
N3, these ideas alone are evidently insufficient for our purpose. Fortunately, we can adapt an idea recently
introduced in [16]: The crucial a priori estimate, uniform boundedness of RT
0Rnεf(cε)|ln(nεf(cε))|, follows
eventually from considering the time evolution of the functional R(ln nε)cε, see Lemma 3.9 and the discussion
directly preceding that lemma.
Additionally relying on (1.3), we are then also able to favourably bound ln cεon sets where cεis small (cf.
Lemma 3.11), which allows us to obtain strong convergence of ln cεin Lemma 3.12. Combined, these bounds
and convergence properties then make it possible to pass to the limit in each term of the weak formulations for
the approximate problems, allowing us to prove Theorem 1.1 in Subsection 3.5.
3
Main result II: Eventual smoothness and stabilization in the two-dimensional setting. A natural next step
is to analyze the behavior of the solution given by Theorem 1.1 for large times with respect to both eventual
regularization and convergence in the large-time limit. These two points are actually related: Both bounds
in comparatively strong topologies and smallness of certain quantities may be key in favourably estimating
worrisome terms in energy functionals, which, depending on the functional, in turn may imply stronger a priori
estimates or convergence (see also the discussion after Theorem 1.2 below).
Indeed, for certain relatives of (1.1) with scalar nonsingular taxis sensitivity, both convergence to homoge-
neous steady states (see for instance [17, 38] for the two-dimensional as well as [4, 5] for the small-data three-
dimensional setting and [41] for results regarding weak solutions) and eventual smoothness properties (see e.g.
[30] for the fluid-free three-dimensional case and [34] for a three-dimensional chemotaxis–Navier–Stokes system
with superlinear degradation) have been shown. Moreover, for tensor-valued taxis sensitivities, global general-
ized solutions have been constructed in planar domains ([12]; see also [39] for a precedent dealing with a Stokes
fluid), whose large-time and eventual regularity properties have been analysed in [13].
Regarding chemotaxis-fluid systems with logarithmic sensitivity, the results appear to be limited to two-
dimensional settings: For Stokes fluids, [33] shows convergence towards homogeneous steady states while [3]
asserts eventual smoothness provided Rn0is sufficiently small. Moreover, under a similar smallness condition,
both convergence and eventual smoothness are obtained in [24] for the full Navier–Stokes equation.
Our second main result is then able to give an affirmative answer to the question whether similar relaxation
properties are also exhibited by the global generalized solution (potentially with large mass) constructed in
Theorem 1.1.
Theorem 1.2. Suppose in addition to the assumption of Theorem 1.1 that N= 2. Then the solution given by
Theorem 1.1 eventually becomes smooth in the sense that there are t>0and PC1,0(×[t,)) such that
n, c C2,1(×[t,)), u C2,1(Ω ×[t,); R2)
and that (n, c, u, P )is a classical solution of (1.1) in ×[t,); that is, that the first four equations therein
are fulfilled pointwise in ×[t,).
Moreover, this solution stabilises in the large time limit. More precisely,
lim
t→∞ kn(·, t)n0kC2(Ω) +kc(·, t)kC2(Ω) +ku(·, t)kC2(Ω)= 0,(1.6)
where n0=1
||Rn0.
This theorem relates to [24, Theorem 1.2] which proves eventual smoothness by requiring smallness of Rn0
instead of (1.3). A key ingredient to both results is the energy functional (4.1), which is conditional in the sense
that it only decreases throughout evolution if certain conditions are met, namely that the functional is already
sufficiently small at some time t00. That this functional indeed dissipates under certain conditions is verified
in Lemma 4.1, where we already rely on (1.3).
In order to actually make use of this conditional energy structure we then need to show that various quantities
become small at some point in time. The starting point is the quasi-energy inequality (3.15) holding for
approximate solutions (nε, cε, uε), ε(0,1). Its right-hand side χ2Rnεc1
εf(cε) becomes small if f(cε) = cε
and Rnε=Rn0is small; this is a core idea of [24, Lemma 5.2]. Not wanting to impose a smallness condition
of the initial data, we are forced to argue differently. A key observation is that nεc1
εf(cε) can be controlled
favourably for cεbounded away from 0 while for small cεthe key condition (1.3) shows that the respective term
becomes small as well. Thus, splitting the right-hand side of (3.15) in integrals over suitable subdomains allows
us to obtain smallness of the first part of the conditional energy functional, see Lemma 4.2 and Lemma 4.3.
4
For the remaining term, we crucially rely on the inequalities (2.3) and (2.4) recently derived by Heihoff in [13].
They improve on related inequalities by getting rid of an additional additive L1term on the right-hand side,
which make them favourably applicable also for large Rn0, see Lemma 4.4.
Finally, the bounds implied by the conditional energy functional serve as a starting point for a bootstrap
procedure sketched in Lemma 4.6, which provides further estimates sufficiently strong to arrive at Theorem 1.2
in Subsection 4.4.
Main result III: Global existence of classical solutions under smallness conditions. As a byproduct of the
arguments developed for proving Theorem 1.2, we immediately obtain global classical solutions emanating from
initial data already satisfying the conditions for the conditional energy functional.
Theorem 1.3. Let R2be a smooth, bounded domain, χ > 0and φW2,(Ω), suppose that fcomplies
with (1.2) and (1.3) and let m0>0. There exists η > 0such that whenever
(n0, c0, u0)C0(Ω) ×W1,q(Ω) × D(Aβ)for some q > 2and β(1
2,1),
where Adenotes the Stokes operator, are such that n0>0and c0>0in ,
Z
n0=m0kc0kL(Ω) m0
and
Z
n0ln n0
n0
+Z
c2
0+Z
|∇c0|2
c2
0
+Z
|u0|2η,
then there exists a global classical solution (n, c, u, P )of (1.1), which moreover satisfies (1.6).
Plan of the paper. We first collect some useful general inequalities in Section 2 before proving Theorem 1.1
in Section 3 and Theorem 1.2 as well as Theorem 1.3 in Section 4; we refer to the beginning of the later two
sections for a discussion of the finer structure. Let us here just point directly to the most crucial new steps:
Lemma 3.9 asserts uniform integrability of nεf(cε) and key ideas relying on (1.3) are employed in Lemma 3.11,
Lemma 4.1 and Lemma 4.2.
Notation. Let Ω RN,NN, be a smooth, bounded domain. Throughout the article, we abbreviate
ϕ:=1
||Rϕfor ϕL1(Ω), set L2
σ(Ω; RN):={ϕL2(Ω) : ∇ · ϕ= 0 in D(Ω) }, where D(Ω) is the
space of distributions on Ω, as well as W1,2
0(Ω; RN):=W1,2
0(Ω; RN)L2
σ(Ω; RN). We further denote by
Pthe Helmholtz projection on L2(Ω; RN) and by Athe Stokes operator P∆ on L2(Ω; RN) with domain
W2,2(Ω; RN)W1,2
0(Ω; RN), and often write L2(Ω) instead of L2(Ω; RN) etc. when the codomain can be
inferred from the context. Moreover, uppercase constants Ciare unique throughout the article while lowercase
constants ciare “local” to each proof.
2 Preliminaries: The Csiszár–Kullback and Heihoff inequalities
This preliminary section is concerned with multiple estimates regarding Rϕln ϕ
ϕand R
|∇ϕ|2
ϕ2for positive
functions ϕ. First, we recall the classical Csiszár–Kullback inequality which gives a nontrivial lower bound for
the former term.
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摘要:

arXiv:2211.01019v1[math.AP]2Nov2022Chemotaxis(-fluid)systemswithlogarithmicsensitivityandslowconsumption:globalgeneralizedsolutionsandeventualsmoothnessMarioFuest∗LeibnizUniversitätHannover,InstitutfürAngewandteMathematik,Welfengarten1,30167Hannover,GermanyAbstractWeconsiderthesystemnt+u·∇n=∆n−χ∇·...

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