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On anisotropic parabolic equations with a nonlinear convection term depending on the spatial variable
Advances in Difference Equations volume 2019, Article number: 27 (2019)
Abstract
Consider an anisotropic parabolic equation with a nonlinear convection term depending on the spatial variable. If the diffusion coefficients are degenerate, in general, the boundary trace cannot be defined for the weak solution. The existence and the uniqueness of weak solution are researched without the boundary value condition. Moreover, a general method to prove stability of weak solutions independent of the boundary value condition is introduced for the first time.
1 Introduction
In this paper, the anisotropic parabolic equation
is considered, where Ω is a bounded domain in \(\mathbb{R}^{N}\) with a \(C^{2}\) smooth boundary ∂Ω, \(p_{i}>1\), \({Q_{T}} = \varOmega \times(0,T)\), \(a_{i}(x) \in C^{1}(\overline{\varOmega})\), \(b_{i}(\cdot, x, t)\in C(\overline{Q_{T}})\).
Equation (1.1) arises in the mathematical modeling of various physical processes such as flows of incompressible turbulent fluids or gases in pipes, and processes of filtration in glaciology [1,2,3]. A particular case of Eq. (1.1) is the usual non-Newtonian fluid equation,
which has been researched far and widely, one can refer to [4,5,6] and the references therein. In recent years, there are more and more mathematicians interested in the anisotropic parabolic equations
one can refer to [7,8,9,10,11,12,13,14].
In this paper, we suppose that
then Eq. (1.1) is always degenerate on the boundary. To study the well-posedness of the solutions of Eq. (1.1), the initial value
is always indispensable. Moreover, the usual boundary value condition
may be invalid. This is due to the fact that the weak solution of Eq. (1.1) may lack the enough regularity to be defined the trace on the boundary [15]. Accordingly, one has tried to study the uniqueness of weak solution only depending on the initial value condition (1.4) [16, 17]. In fact, for a degenerate parabolic equation, that the boundary value (1.5) may be overdetermined is well known, one can refer to [18,19,20,21,22,23,24,25,26,27]. But how to impose a suitable boundary value condition instead of (1.5) has been a difficult and interesting unsolved problem for a long time.
Inspired by [15,16,17,18,19,20,21,22,23,24,25,26,27], we may conjecture that the degeneracy of \(a_{i}(x)\) on the boundary may take the place of the usual boundary value condition (1.5). In other words, the stability of weak solutions can be proved without the condition (1.5). Comparing with our previous work [16, 17], not only the anisotropic case is more complicated than the isotropic case, but also the nonlinear convection term \(\sum_{i=1}^{N}\frac{\partial b_{i}(u,x,t)}{\partial x_{i}}\) adds difficulties. We employ some special techniques to overcome these difficulties. Moreover, we will introduce a general method to study the stability of weak solutions for a parabolic equation without the boundary value condition.
2 Definitions and main results
We denote
In the first place, we introduce definition of weak solutions.
Definition 2.1
A function \(u(x,t)\) is said to be a weak solution of Eq. (1.1) with the initial value (1.4), if
and for any function \(\varphi \in C_{0}^{1}(Q_{T})\),
The initial value is satisfied in the following sense:
Definition 2.2
The function \(u(x,t)\) is said to be the weak solution of Eq. (1.1) with the initial boundary values (1.4)–(1.5) if u satisfies Definition 2.1, and the boundary value condition (1.5) is satisfied in the sense of trace.
Theorem 2.3
If \(p_{-}>2\), \(a_{i}(x)\in C^{1}(\overline{\varOmega })\) satisfies (1.3), \(b_{i}(s,x,t)\) is a \(C^{1}\) function on \(\mathbb {R}\times\overline{ \varOmega}\times[0,T]\),
either
or
then Eq. (1.1) with initial value (1.4) has a weak solution.
Theorem 2.4
Let \(p_{-}>2\), for every \(1\leq i\leq N\), either condition (2.5) be true, or \(\int_{\varOmega}a_{i}^{-\frac{1}{p_{i}-1}}(x)\,dx<\infty\) and condition (2.6) be true, \(a_{i}(x)\in C^{1}(\overline{\varOmega})\) satisfy (1.3), \(b_{i}(s, x, t)\) be a \(C^{1}\) function on \(\mathbb{R}\times\overline{ \varOmega}\times[0,T]\). Then the initial boundary value problem (1.1)–(1.4)–(1.5) has a solution.
If \(b_{i}\equiv0\), then only if \(p_{-}>1\) and \(\int_{\varOmega }a_{i}^{-\frac{1}{p_{i}-1}}(x)\,dx<\infty\), Theorem 2.3 and Theorem 2.4 are still true. However, if \(b_{i}\equiv0\) is not valid, when \(p_{-}>1\), then it is difficult to prove that \(u_{t}\in L^{2}(Q_{T})\). If we do not require \(u_{t}\in L^{2}(Q_{T})\), in other words, if we admit \(u_{t}\) belonging to another kind of Banach space, then the conditions (2.5) and (2.6) may not be necessary, one can refer to our previous work [28]. Moreover, the condition (2.6) (also the condition (2.9)) reflects that there are some relationships between the diffusion coefficient and the convection term. At least, one of our motivations on condition (2.6) (also the condition (2.9)) initially comes from the study of a model of strong degenerate parabolic equation arising in mathematical finance [29], which has the form
and satisfies
where \(\varOmega\subset\mathbb{R}^{2}\) is a bounded domain with the smooth boundary ∂Ω. From this, one can see that there are some relationships between the diffusion coefficient and the convection term.
Since we mainly are concerned about how the degeneracy of the coefficient \(a_{i}(x)\) affects the uniqueness or the stability of weak solutions, we have no intention to make a deep research on the existence. The main results of this paper are the following stability theorems.
Theorem 2.5
Let \(p_{-}>1\), for \(1\leq i\leq N\), \(a_{i}(x)\in C^{1}(\overline{\varOmega})\) satisfy (1.3), \(\int_{\varOmega}a_{i}^{-\frac {1}{p_{i}-1}}(x)\,dx<\infty\) and \(b_{i}(s,x,t)\) be a Lipchitz function \(\mathbb{R}\times\overline{ \varOmega}\times[0,T]\). If u and v are two solutions of Eq. (1.1) with the same homogeneous boundary value condition
and with different initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively, then
Roughly speaking, the condition \(\int_{\varOmega}a_{i}^{-\frac {1}{p_{i}-1}}(x)\,dx<\infty\) can guarantee that the boundary value condition (1.5) is true in the sense of trace. If this condition is invalid, for example,
and
that whether Theorems 2.4–2.5 are true or not is an open problem. Fortunately, by adding some restrictions on \(a_{i}(x)\) and \(b_{i}(s,x,t)\), we are able to prove the following stability of weak solutions without any boundary value condition, no matter whether \(\int_{\varOmega }a_{i}^{-\frac{1}{p_{i}-1}}(x)\,dx<\infty\) or not.
Theorem 2.6
Let \(p_{-}>1\), \(a_{i}(x)\in C^{1}(\overline{\varOmega })\) satisfy (1.3), \(b_{i}(s,x, t)\) be a Lipschitz function on \(\mathbb {R}\times\overline{ \varOmega}\times[0,T]\). Let u and v be two solutions of (1.1) with the initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively. If \(b_{i}(s,x,t)\) satisfies
and, for η small enough,
then the stability (2.8) is true.
Here, \(\varOmega_{\eta}=\{x\in\varOmega: (\prod_{j=1}^{N} a_{j}(x))>\eta\}\).
Comparing Theorem 2.6 with Theorem 2.5, we find that, in some cases, the degeneracy of \(a_{i}(x)\) on the boundary can take the place of the usual boundary value condition (1.5). Even, for some given kind of the weak solutions, the condition (2.10) may not be necessary. For example, we have the following result.
Theorem 2.7
Let \(p_{-}>1\), \(a_{i}(x)\in C^{1}(\overline{\varOmega })\) satisfy (1.3), \(b_{i}(s,x, t)\) be a Lipschitz function on \(\mathbb {R}\times\overline{ \varOmega}\times[0,T]\). Let u and v be two solutions of (1.1) with the initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively, and for η small enough,
If \(b_{i}(s,x,t)\) satisfies (2.9), then the stability (2.8) is true.
However, for some weak solutions, condition (2.9) may not be necessary. In fact, if the convection term is independent of the diffusion coefficient, we have the following result.
Theorem 2.8
Let \(p_{-}>1\), \(a_{i}(x)\in C^{1}(\overline{\varOmega })\) satisfy (1.3), \(b_{i}(s,x, t)\) be a Lipschitz function on \(\mathbb {R}\times\overline{ \varOmega}\times[0,T]\). If u and v are two solutions of Eq. (1.1) with the initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively, then, for any \(\varOmega_{1}\subset\subset\varOmega\),
which implies that the uniqueness of weak solution is true.
Actually, by the general method introduced in the last section of this paper, many kinds of stability theorems of weak solutions can be found.
3 The weak solutions dependent on the initial value
We consider the following regularized problem:
Here, \(u_{\varepsilon0} \in C^{\infty}_{0}(\varOmega)\), \(|u_{\varepsilon 0}|_{L^{\infty}(\varOmega)}\leq|u_{0}|_{L^{\infty}(\varOmega)}\), \(\vert \nabla u_{\varepsilon0} \vert \) converges to \(|\nabla u_{0}(x)|\) in \(L^{p_{+}}(\varOmega)\). It is well known that the above problem has an unique weak solution \(u_{\varepsilon}\in L^{\infty}(0,T; W_{0}^{1,\vec {p}}(a_{i}(x), \varOmega))\) [5, 30].
By the maximum principle [5], there is a constant c only dependent on \({ \Vert {{u_{0}}} \Vert _{{L^{\infty}}(\varOmega)}}\) but independent on ε, such that
Multiplying (3.1) by \(u_{\varepsilon}\) and integrating it over \(Q_{T}\), then
If \(\int_{\varOmega}a_{i}^{-\frac{2}{p_{i}-2}}(x)\,dx<\infty\), we know that \(\int_{\varOmega}a_{i}^{-\frac{1}{p_{i}-1}}(x)\,dx<\infty\), then
If the condition (2.6) is true, then
clearly. Accordingly, by (3.4), we have
For any \(\varOmega_{1}\subset\subset\varOmega\), since \(p_{-}=\min\{p_{i}\} >2\), \(a_{i}(x)\) satisfies (1.3),
by (3.5),
where \(c(\varOmega_{1})\) represents the constant depending upon the compact subset \(\varOmega_{1}\), but it may be different from one to another.
Multiplying (2.5) by \(u_{\varepsilon t}\), integrating it over \(Q_{T}\), it yields
Noticing that
then
If \(\int_{\varOmega}a_{i}^{-\frac{2}{p_{i}-2}}(x)\,dx<\infty\),
by the Hölder inequality
If \(|b_{is}(s,x,t)|\leq ca_{i}^{\frac{2}{p_{i}}}(x)\), \(p_{i}\geq2\), then by the Young inequality
Combining (3.7)–(3.10), we have
by the above inequality, we have
Now, by (3.4), (3.5), (3.6) and (3.11), there exist a function u and an n-dimensional vector function \(\overrightarrow{\zeta}= ({\zeta _{1}}, \ldots,{\zeta_{n}})\) satisfying \(u_{\varepsilon}\rightarrow u\) a.e. in \(Q_{T}\), and
It is easy to show that
for any \(\varphi\in C_{0}^{1}(Q_{T})\).
Now, we will prove that
for any given function \(\varphi_{1} \in C_{0}^{1} ({Q_{T}})\). In detail, we notice that, for any function \(\varphi \in C_{0}^{1} ({Q_{T}})\),
Let \(\varepsilon\rightarrow0\). Then
Let \(0 \leqslant\psi \in C_{0}^{\infty}({Q_{T}})\) and \(\psi=1\) on \(\operatorname{supp}\varphi_{1}\). Let \(v \in {L^{\infty}}({Q_{T}})\), \(a_{i}(x) \vert v_{x_{i}} \vert ^{p_{i}} \in {L^{1}}({Q_{T}})\). One has
By choosing \(\varphi = \psi u_{\varepsilon}\) in (3.15),
Let \(\varepsilon\rightarrow0\). Then
Let \(\varphi=\psi u\) in (3.16). We get
Thus
Let \(v=u- \lambda\varphi_{1}\), \(\lambda>0\). Then
If \(\lambda\rightarrow0\), then
Moreover, if \(\lambda<0\), similarly we can get
Thus
Noticing that \(\psi= 1\) on \({\operatorname{supp}}\varphi_{1}\), then (3.14) holds.
At last, we are able to prove (2.3) as in [31], then u is a solution of Eq. (1.1) with the initial value (1.4) in the sense of Definition 2.1. Thus we have Theorem 2.3.
Now, by a similar method as in [32], we can prove the following.
Lemma 3.1
If \(\int_{\varOmega}a_{i}^{-\frac {1}{p_{i}-1}}(x)\,dx<\infty\), u is a weak solution of Eq. (1.1) with the initial condition (1.4). Then, for any given \(t\in[0,T)\),
For simplicity, we omit the details of the proof of Lemma 3.1 here. By (3.23) and the fact \(\iint_{Q_{T}}|u_{t}|\,dx\,dt\leq c\), we know that \(u\in BV(Q_{T})\), \(C_{0}^{\infty}(Q_{T})\) is dense in \(BV(Q_{T})\) and the trace of u on the boundary ∂Ω can be defined in the traditional way. By Theorem 2.3 and Lemma 3.1, we clearly have Theorem 2.4.
4 The stability of the initial boundary value problem
In order to prove the stability of the weak solutions, for small \(\eta >0\), let
Obviously, \(h_{\eta}(s)\in C(\mathbb{R})\), and
Clearly, if we denote \(H_{\eta}(s)=\int_{0}^{s}S_{\eta}(\tau)\,d\tau\), then we have
Lemma 4.1
Let \(p_{-}>1\), for \(1\leq i\leq N\), \(\int_{\varOmega }a_{i}^{-\frac{1}{p_{i}-1}}(x)\,dx<\infty\) and
If u and v are two solutions of Eq. (1.1) with the same homogeneous value condition
and with different initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively, then
Proof
Let u and v be two weak solutions of Eq. (1.1). Since \(\int_{\varOmega}a_{i}^{-\frac{1}{p_{i}-1}}(x)\,dx<\infty\), by Lemma 3.1, \(u,v\in BV(Q_{T})\) we can choose \(\varphi=\chi_{[\tau,s]}S_{\eta }(u - v)\) as the test function. Here \(\chi_{[\tau,s]}\) is the characteristic function of \([\tau, s]\subset(0, T)\). Then
As usual, one has
Since \(\iint_{Q_{T}}|u_{t}|\,dx\,dt\leq c\), \(\iint_{Q_{T}}|v_{t}|\,dx\,dt\leq c\), using the dominated convergence theorem, one has
where \(H_{\eta}(u-v)(x,s)=H_{\eta}(u(x,s)-v(x,s))\).
Moreover, since \(b_{i}(s,x,t)\) satisfies the condition (4.3), one has
Now, let \(\eta\rightarrow0\) in (4.5). By (4.6)–(4.8), one has
Let \(\tau\rightarrow0\). Then
Lemma 4.1 is proved. □
In fact, the condition (4.3) in Lemma 4.1 is not the optimal. Without the condition (4.3), we have Theorem 2.5.
Proof of Theorem 2.5
From the above proof of Lemma 4.1, we only need to prove that
without the condition (4.3). In detail, we have
If the set \(\{\varOmega: |u-v|=0\}\) has zero a measure, then
If the set \(\{\varOmega: |u-v|=0\}\) only has a positive measure, then by, \(a_{i}^{-\frac{1}{p_{i}-1}}\in L^{1}(\varOmega)\),
Thus, we have the conclusion. □
5 The global stability without the boundary value condition
Proof of Theorem 2.6
Let u and v be two weak solutions of Eq. (1.1) with the initial values \(u_{0}(x)\), \(v_{0}(x)\), respectively.
Let \(\varOmega_{\eta}= \{x\in\varOmega:\prod_{i=1}^{N}a_{i}(x)>\eta \}\), and
Let us recall
where k is a constant such that \(\int_{\mathbb{R}^{N}}J(x)\,dx=1\). The usual mollifier is defined as
for small \(\varepsilon>0\). Let
for any \(f(x)\in L^{1}_{\mathrm{loc}}(\overline{\varOmega})\).
Let \(\phi_{\eta\varepsilon}(x)\) be the mollified function of \(\phi _{\eta}(x)\). We can choose \(\chi_{[\tau,s]}\phi_{\eta\varepsilon }(x)S_{\eta}(u - v)\) as the test function. By the process of taking the limit, \(\varepsilon\rightarrow0\), we can choose \(\chi_{[\tau ,s]}\phi_{\eta}(x)S_{\eta}(u - v)\) as the test function finally. Then
Let us observe every term on the left-hand side of (5.2).
For the first term, using the dominated convergence theorem, we have
For the second term, we have
For the third term, obviously, \(\phi_{\eta x_{i}}=\frac{1}{\eta} (\prod_{j=1}^{N} a_{j}(x) )_{x_{i}}\) when \(x\in\varOmega\setminus \varOmega_{\eta}\), in the other places, it is identical to zero. By the condition (2.10), we have
Then
For the fourth term, since \(b_{i}(s,x,t)\) satisfies the condition (2.9), we have
as before.
Finally, for the fifth term, by the condition (2.10), we have
since \(u,v\in L^{\infty}(Q_{T})\).
Now, let \(\eta\rightarrow0\) in (5.2). Then
where \(l<1\).
Let \(\kappa(s)=\int_{\varOmega}|u(x,s)-v(x,s)|\,dx\). Without loss of the generality, we may assume that there exists \(\tau \in[0, T)\), \(\kappa(\tau)>0\). Then, for any \(s> \tau\), \(\int_{\tau }^{s}k(t)\,dt>0\). If we denote
then \(\tau<\tau_{0}\leq s\), and
By \(u,v\in L^{\infty}(Q_{T})\), there exists a constant \(C>0\) such that
using the Gronwall inequality, we easily get
then, by the arbitrariness of Ï„,
 □
Proof of Theorem 2.7
Similar to the proof of Theorem 2.6, we have (5.1)–(5.4). Now, by the condition (2.11), we have
Last but not least, since \(a_{i}(x)\in C^{1}(\overline{\varOmega})\), \(a_{i}(x)=0\) when \(x\in\partial\varOmega\), we have
According to the definition of \(\varOmega_{\eta}\), we have
Now, let \(\eta\rightarrow0\) in (5.2). Then
By the arbitrariness of Ï„,
 □
6 The uniqueness of the solution
Theorem 2.6 and Theorem 2.7 both imply that the uniqueness of the weak solution is true, their proofs are based on the condition (2.9). Actually, without the condition (2.9), we still can prove the uniqueness of the solution without any boundary value condition.
Theorem 6.1
Let \(p_{-}>1\), \(a_{i}(x)\in C^{1}(\overline{\varOmega })\) satisfy (1.3), \(b_{i}(s,x, t)\) be a Lipschitz function on \(\mathbb {R}\times\overline{ \varOmega}\times[0,T]\). If u and v are two solutions of Eq. (1.1) with the initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively, then there exists a positive constant \(\beta_{j}\geq2\) such that
In particular, for any small enough constant \(\delta>0\),
where \(\varOmega_{\delta}= \{x\in\varOmega: \prod_{j=1}^{N} a_{j}^{\beta_{j}}(x)>\delta \}\).
Proof
Let u and v be two solutions of Eq. (1.1) with the initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively. By the process of taking the limit, we may choose \(\varphi=\chi_{[\tau,s]}\prod_{j=1}^{N}a_{j}^{\beta_{j}}(u-v)\) as a test function. Denoting that \(Q_{\tau s}=\varOmega\times[\tau, s]\), then
In the first place, we have
and
Here, we have used the fact that \(|a_{x_{i}}|\leq c\). Now, we choose \(\beta_{i}\geq2\). If \(p_{i}\geq2\),
If \(1< p_{i}<2\), by the Hölder inequality
Combining (6.5)–(6.7), we obtain
where \(l<1\).
In the second place,
For the first term on the right-hand side of (6.7), since \(\beta_{j}\geq 2\), \(| a_{jx_{i}}|\leq c\), by the Hölder inequality,
For the second term on the right-hand side of (6.9), since \(\beta _{i}\geq1\), denoting \(p_{i}'=\frac{p_{i}}{p_{i}-1}\) as usual, we have
By this inequality, we have
If \(p_{i}>2\), then \(1< p_{i}'<2\). By the Hölder inequality,
If \(1< p_{i}\leq2\), then \(p_{i}'\geq2\),
Combining (6.11)–(6.13), we have
where \(l<1\).
Moreover,
According to (6.3), (6.4), (6.8), (6.10), (6.14) and (6.15), we have
where \(l<1\). By (6.16), we easily show that
Thus, by the arbitrariness of Ï„, we have
By (6.18), we clearly have (6.1) and (6.2). The proof is complete. □
By this theorem, Theorem 2.8 is true.
7 The general method to prove the stability of weak solutions
We can generalize the method used in Sect. 6 to prove various kinds of stability of weak solutions.
Let \(\chi(x)\) be a \(C^{1}(\overline{\varOmega})\) function satisfying
Theorem 7.1
Let \(p_{-}\geq2\), \(a_{i}(x)\in C^{1}(\overline {\varOmega})\) satisfy (1.3), \(b_{i}(s,x, t)\) is bounded when s is bounded and \((x,t)\in\varOmega\times[0,T)\). If there exist constants \(0<\sigma_{i}<1\), \(0<\delta_{i}<1\), and there exists \(\chi(x)\) satisfying (7.1) and
Let u and v are be solutions of Eq. (1.1) with the initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively. Then, for any \(\varOmega_{1}\subset \subset\varOmega\),
Here, \(p_{i}'=\frac{p_{i}}{p_{i}-1}\) as usual.
Proof
Let u and v be two solutions of Eq. (1.1) with the initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively. By the process of taking the limit, we may choose \(\varphi=\chi_{[\tau,s]}\chi (x)(u-v)\) as a test function. Denoting \(Q_{\tau s}=\varOmega\times[\tau , s]\), then
In the first place, we have
and using (7.2) we deduce that
In the second place,
For the first term on the right-hand side of (7.7), since \(b_{i}(u,x,t)\) and \(b_{i}(v,x,t)\) are bounded when \(u\in L^{\infty }(Q_{T})\), \(v\in L^{\infty}(Q_{T})\), and by that \(p_{-}\geq2\) implies \(p_{i}'-\frac{2\delta_{i}}{(2-\delta _{i})(p_{i}-1)}\geq0\), by the Hölder inequality, using (7.2), we have
For the second term on the right-hand side of (7.7), by this inequality and the condition (7.3), we have
Moreover,
According to (7.4)–(7.10), we have
where \(l<1\). By (7.11), we easily can show that
By the arbitrariness of Ï„, then
Since (7.1), by (7.13), the inequality (7.3) is true clearly.
One can see that the condition \(p_{-}\geq2\) is only used to estimate (7.8). We are sure that it can weakened to \(p_{-}>1\). For example, if there exists constant \(\gamma_{i}>0\) such that
then we obtain
where \(l<1\). Thus, we still have the conclusion of Theorem 7.1. □
However, we are not ready to discuss how to weaken the condition \(p_{-}\geq2\) again in what follows. We prefer to explain the importance of Theorem 7.1. That is, if we choose various kinds of functions \(\chi(x)\), we can obtain the corresponding stability theorems. Let us give some examples.
If we choose \(\chi(x)=\prod_{i=1}^{N}a^{\beta}_{i}(x)\), we have a similar conclusion to Theorem 2.8. By the process of taking the limit, we can choose \(\chi(x)=d^{\alpha}(x)\), where \(\alpha>0\) is a constant, \(d(x)=\operatorname{dist}(x, \partial\varOmega)\) is the distance function from the boundary. Then we have the following theorem.
Theorem 7.2
Let \(p_{-}\geq2\), \(a_{i}(x)\in C^{1}(\overline {\varOmega})\) satisfy (1.3), \(b_{i}(s,x, t)\) is bounded when s is bounded and \((x,t)\in\varOmega\times[0,T)\). Assume \(\alpha>1\), and assume there exist constants \(0<\sigma_{i}<1\),
Let u and v are be solutions of Eq. (1.1) with the initial values \(u_{0}(x)\) and \(v_{0}(x)\), respectively. Then, for any \(\varOmega_{1}\subset \subset\varOmega\),
Proof
Since \(\chi(x)=d^{\alpha}(x)\), \(\alpha>1\), for any \(0<\sigma_{i}<1\), it is not difficult to show the inequality (7.1) is true. Then we have the conclusion. □
As long as one wants, one can choose other types of the functions \(\chi (x)\), e.g. \(\chi(x)=\sum_{i=1}^{N} a_{i}(x)\), \(\chi(x)=e^{a_{i}(x)}-1\) for any given \(i\in\{1,2,\ldots, N\}\), or \(\chi(x)=\max\{a_{i}(x)\}\), to obtain the corresponding stability theorems.
8 Conclusion
The anisotropic parabolic equations considered in this paper arise from many applied fields such as non-Newtonian fluid theory, reaction–diffusion problems. If the convection term depends on the diffusion coefficient which is degenerate on the boundary, then the stability of weak solutions may be proved without any boundary value condition. If the convection term is independent of the diffusion coefficient, the uniqueness of the weak solution is still true only if the convection function \(b_{i}(u,x,t)\) is bounded when \(|u|\leq c\). Moreover, a general method to prove the stability of the weak solutions without the boundary value condition is introduced for the first time in this paper. We believe such a method can be used in many kinds of parabolic equations, especially those lacking the regularity for the trace on the boundary to be defined.
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The paper is supported by Natural Science Foundation of Fujian province, supported by the Open Research Fund Program form Fujian Engineering and Research Center of Rural Sewage Treatment and Water Safety, supported by Science Foundation of Xiamen University of Technology, China.
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Zhan, H. On anisotropic parabolic equations with a nonlinear convection term depending on the spatial variable. Adv Differ Equ 2019, 27 (2019). https://doi.org/10.1186/s13662-019-1969-8
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DOI: https://doi.org/10.1186/s13662-019-1969-8