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On local existence of the VlasovFokkerPlanck equation in a 2D anisotropic space
Boundary Value Problems volume 2013, Article number: 233 (2013)
Abstract
We are concerned with local existence of the VlasovFokkerPlanck equation in a 2D anisotropic space ${L}_{x}^{p}{L}_{v}^{1}$ in a bounded domain with respect to the space variable. The energy method is used to construct the result and the Hardy inequality is used to estimate the electric field.
1 Introduction
Through this paper, as in the title, when anisotropic space is mentioned, we mean that the space variable x and the velocity variable v have different regularities, such as integrability and differentiability. Firstly, we would like to give a review which has close relationship with our paper. As to a classical solution, it is worthy to mention the paper of Yang and Yu [1]. They constructed the globalintime classical solutions to the VlasovMaxwellFokkerPlanck system near Maxwellian using an approach by combining the compensating function and energy method. For the system of (1.1) in the whole space, there are many results about weak solutions. We refer to them as follows. Triolo [2] obtained the global (local) existence in 1 and 2dimension (3dimension) for the Cauchy problem of the VlasovPoissonFokkerPlanck equation under the initial value ${f}_{0}\in {L}^{1}\cap {L}^{\mathrm{\infty}}\cap {C}^{0}({\mathbb{R}}^{n}\times {\mathbb{R}}^{n})$, $n=1,2,3$. Neunzert and some other authors [3] considered the modified VlasovFokkerPlanck equation problem, under the condition that the initial value ${f}_{0}\in {L}^{\mathrm{\infty}}({\mathbb{R}}^{2}\times {\mathbb{R}}^{2})$ has compact support in v, they got a solution which is a probability measure. Zheng and Majda [4] gave the existence of a global weak solution of the VlasovFokkerPlanck system under the measurevalued initial data. Degond [5] obtained the existence of solution which has the same regularity as the initial value
The author required that ${f}_{0}$ has the same index of differentiability and integrability with respect to variables x and v, i.e., they are isotropic. Comparing with [5], we do not need ${f}_{0}$, $D{f}_{0}$ to be bounded, continuous to offset, we cannot obtain the global existence even in a 2D space because of the difficulty to get the Gronwall inequality which can be solved in $t\in [0,\mathrm{\infty})$. Roughly speaking, the essential difficult point lies in that ${\parallel {\mathrm{\nabla}}_{x}{E}^{n}\cdot {\mathrm{\nabla}}_{v}{f}^{n+1}\parallel}_{{L}_{x}^{p}{L}_{v}^{1}}$ is in proportion to ${\parallel f\parallel}_{{L}_{x}^{p}{L}_{v}^{1}}^{2}$, which is superlinear.
In this paper, we consider the initial boundary problem with 0 boundary value (see (1.1)). The problem about general boundary value [6, 7] is so tough that we are going to consider it in the next paper. Moreover, we focus on the case in which the initial value ${f}_{0}$ has different regularities with respect to the x and v variables, i.e., they have different integral and differential indices. An anisotropic space is natural since the variables x and v need not to have the same regularity. For instance, Strain [8] considered the anisotropic space ${\dot{B}}_{2}^{\varrho ,\mathrm{\infty}}{L}_{v}^{2}$ when he studied the optimal decay rate of the solution to the hard and soft potential Boltzmann equation.
Before narrating the main theorem, we would like to introduce some notations.
Notation

(i)
$f(x,v,t)$, $x\in \mathrm{\Omega}\subset {\mathbb{R}}^{2}$ with $\partial \mathrm{\Omega}\in {C}^{1}$, $v\in {\mathbb{R}}^{2}$, $t>0$, the distribution function of the particles, where Ω is a bound open set with a ${C}^{1}$ boundary (for Definition see p.626 of [9]).

(ii)
${L}_{x}^{p}{L}_{v}^{1}$ is a space in which the elements are given the norm ${({\int}_{\mathrm{\Omega}}{\parallel f\parallel}_{{L}_{v}^{1}}^{p}\phantom{\rule{0.2em}{0ex}}dx)}^{\frac{1}{p}}$, $1\le p<\mathrm{\infty}$, here ${L}_{v}^{1}$ is the Lebesgue space with the norm given by ${\parallel f\parallel}_{{L}_{v}^{1}}:={\int}_{{\mathbb{R}}^{2}}f\phantom{\rule{0.2em}{0ex}}dv$.

(iii)
${L}^{2}([0,T]\times {\mathrm{\Omega}}_{x},{H}^{1}({\mathbb{R}}_{v}^{2}))$ is a space given the norm ${({\int}_{[0,T]\times {\mathrm{\Omega}}_{x}}{\parallel f\parallel}_{{H}_{v}^{1}}^{2}\phantom{\rule{0.2em}{0ex}}dt\phantom{\rule{0.2em}{0ex}}dx)}^{\frac{1}{2}}$, here ${H}_{v}^{1}$ is the Sobolev space with respect to v.
Now we are ready to state our main theorem.
In the theorem, we denote respectively by $E(x,t)$, $\rho (x,t)$ the electric field and the electric charge. $\sigma >0$ is a diffusion coefficient which is very small in physical situations.
Theorem 1.1 Suppose ${f}_{0}\in {L}^{2}(\mathrm{\Omega}\times {\mathbb{R}}_{v}^{2})$ and ${\parallel {f}_{0}\parallel}_{{L}_{v}^{1}}{}_{\partial \mathrm{\Omega}}=0$. Also, we assume that ${f}_{0}$ is nonnegative and
Here $p=\frac{4}{3}$. Then the VlasovFokkerPlanck system with bounded domain
admits a solution in the interval $[0,T)$, i.e., $f(x,v,t)\in {L}_{\mathrm{loc}}^{\mathrm{\infty}}([0,T),{L}_{x}^{p}{L}_{v}^{1})$. Here we mean the boundary value in the sense of trace (see p.259 of [9]). Moreover, we have that ${\mathrm{\nabla}}_{x}f,{\mathrm{\nabla}}_{v}f\in {L}_{\mathrm{loc}}^{\mathrm{\infty}}([0,T),{L}_{x}^{p}{L}_{v}^{1})$. The solution is unique.
The arrangement of this paper is the following. In Section 2, we cite or prove some lemmas which will be used in the proof of Theorem 1.1. In Section 3, we give the proof of the main theorem in several steps.
2 Some lemmas
Consider the linear equation, i.e.,
Next we introduce some lemmas, which are modified versions of the lemmas in Appendix A in [5] and will be used in the proof of Theorem 1.1 in Section 3. We only point out the differences, the details can be found in the reference.
Lemma 2.1 Assume
where $p>2$. Then equation (2.1) has a unique solution f in a class of functions Y defined according to
Proof Since $E(x,t)\in {L}_{t}^{\mathrm{\infty}}{L}_{x}^{p}$, $\int \int {\mathrm{\nabla}}_{v}\phi \cdot E\phi \phantom{\rule{0.2em}{0ex}}dx\phantom{\rule{0.2em}{0ex}}dv$ exists for any $\phi \in \mathcal{D}$, which implies $\int {\mathrm{\nabla}}_{v}\phi \cdot E\phi \phantom{\rule{0.2em}{0ex}}dv=0$.
On the other hand, since $f\in {L}^{2}([0,T]\times {\mathrm{\Omega}}_{x},{H}^{1}({\mathbb{R}}_{v}^{2}))$, we have $\mathrm{\forall}x\in \mathrm{\Omega}$, ${\mathrm{\nabla}}_{v}f\in {L}^{2}([0,T],{H}^{1}({\mathbb{R}}_{v}^{2}))$, which implies $\mathrm{\forall}x\in \mathrm{\Omega}$,
The other processes are similar. □
Remark 2.2 Similar to Lemma A.1 on p.535 of [5], we mean the initial condition that for any $u\in Y$, u admits trace value $u(x,v,0)\in {L}_{v}^{2}$ for a.e. $x\in \mathrm{\Omega}$.
Lemma 2.3 Assume in addition ${f}_{0}\in {L}_{x}^{p}{L}_{v}^{1}$; $U\in {L}_{t}^{1}{L}_{x}^{p}{L}_{v}^{1}$, then the solution defined in Lemma 2.1 belongs to ${L}^{\mathrm{\infty}}([0,T],{L}_{x}^{p}{L}_{v}^{1})$ and satisfies for $t\in [0,T]$ a.e.,
Proof Using quite a similar method to that on p.540 of [5], we get for a.e. x,
Taking the ${L}^{p}$ norm with respect to x yields the desired result. □
3 Proof of the main theorem
After the above preparation, we are in a position to prove our main theorem.
Proof To prove the theorem, we split the process into several steps. The first step is to construct the approximating solution sequence; in the second step, we prove the regularity of the solution we have obtained; and in the last step, we prove the uniqueness. To get the existence of a weak solution in the space ${L}_{x}^{p}$, it is natural to require ${f}^{n}$ to be a Cauchy sequence in the strong topology of ${L}_{x}^{p}$ and $E(t,x)$ to be bounded in ${L}_{x}^{{p}^{\prime}}$, here $\frac{1}{p}+\frac{1}{{p}^{\prime}}=1$. To estimate the ${L}^{{p}^{\prime}}$ norm of $E(t,x)$, we will use the Hardy inequality.
Step 1: We construct an iterative solution sequence to approximate the solution of the original equation.
Firstly, on the one hand, to guarantee the weak convergence, we need the weak convergence of ${E}^{n}$ in ${L}^{{p}^{\prime}}$, which in turn can be deduced by the boundedness of ${E}^{n}$ in ${L}^{{p}^{\prime}}$. By the Hardy inequality [10–12], we have
where
On the other hand, by Lemma 2.1 and Lemma 2.3, let ${f}^{0}=0$, we obtain a unique solution ${f}^{n+1}$ to (3.1). To pass to the limit in the system of (1.1), we need a strong convergence. In order to get this, we compute the Cauchy sequence as follows:
Here
Combining (3.2) with (3.3), we solve the indices $p=\frac{4}{3}$ and ${p}^{\prime}=4$. We claim that
uniformly in n. Thus,
By a process of induction, we obtain
which implies ${f}^{n}$ converges to some f in ${L}_{\mathrm{loc}}^{\mathrm{\infty}}([0,T),{L}_{x}^{p}{L}_{v}^{1})$.
Proof of the claim of (3.4).
A direct calculation by using the Hardy inequality yields
here $\frac{1}{q}+\frac{p}{2}=1+\frac{p}{{p}^{\prime}}$, $q>1$.
Differentiating equation (3.1) by ${D}_{x}$ and ${D}_{v}$, respectively, we get
Applying Lemma 2.3 to (3.6) yields
where $p>1$. Since
We require ${p}_{1}\le {p}^{\prime}$, $p<{p}^{\prime}$, this is an easy thing. Note that ${L}^{pq}(\mathrm{\Omega})\subset {L}^{p}(\mathrm{\Omega})$ and ${L}^{{p}_{2}}(\mathrm{\Omega})\subset {L}^{p}(\mathrm{\Omega})$. Plugging (3.8) and (3.9) into (3.7) yields
Next, we only have to solve the Gronwall inequalities in the form
These inequalities only hold in finite time, we denote the maximal existence time by T, i.e., for $t\in [0,T)$, there exists $\alpha (t)\in {L}^{\mathrm{\infty}}([0,T))$ such that
Therefore, the claim of (3.4) holds.
According to the standard weak convergence process, we conclude that f is a solution of the Cauchy problem of equations of (1.1).
Step 2: Regularity of the solution.
Denote ${D}_{x}$ or ${D}_{v}$ by D. Since ${f}^{n}\to f$ in ${L}_{x}^{p}{L}_{v}^{1}$, which deduces $D{f}^{n}\to Df$ in ${\mathcal{D}}^{\prime}({\mathrm{\Omega}}_{x}\times {\mathbb{R}}_{v}^{2})$, note that ${\parallel D{f}^{n}\parallel}_{{L}_{x}^{p}{L}_{v}^{1}}\le \text{const}$, we have ${\parallel Df\parallel}_{{L}_{x}^{p}{L}_{v}^{1}}\le {\parallel D{f}^{n}\parallel}_{{L}_{x}^{p}{L}_{v}^{1}}\le \text{const}$.
By property (i) of Proposition A.3 in [5], we conclude that ${f}^{n}$ is nonnegative. Moreover, ${f}^{n}\to f$, a.e. $(x,v)\in {\mathrm{\Omega}}_{x}\times {\mathbb{R}}_{v}^{2}$, since ${f}^{n}\to f$ in ${L}_{x}^{p}{L}_{v}^{1}$, which implies that f is nonnegative.
Step 3: Uniqueness of the solution.
The uniqueness is a direct consequence of
which in turn is a result of a very similar process to (3.5).
Next we are going to deal with the boundary, i.e., to show that the solution satisfied the boundary condition.
On the one hand, by Lemma 2.3, we have ${\parallel {f}^{n}\parallel}_{{L}_{v}^{1}}\le {\parallel {f}_{0}\parallel}_{{L}_{v}^{1}}$ for x a.e.; on the other hand, ${\parallel {f}^{n}(t,x,v)\parallel}_{{L}_{v}^{1}}\to {\parallel f(t,x,v)\parallel}_{{L}_{v}^{1}}$ for x a.e. Thus ${\parallel f(t,x,v)\parallel}_{{L}_{v}^{1}}\le {\parallel {f}_{0}\parallel}_{{L}_{v}^{1}}$ for x a.e., note the assumption of ${\parallel {f}_{0}\parallel}_{{L}_{v}^{1}}{}_{\partial \mathrm{\Omega}}=0$ in the sense of trace of ${L}_{x}^{p}$, we conclude in the sense of trace of ${L}_{x}^{p}$, since the boundary is ${C}^{1}$ and ${\parallel {f}^{n}\parallel}_{{L}_{v}^{1}}\in {W}_{x}^{1,p}$:
□
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Acknowledgements
The authors would like to thank the editors and the reviewers for providing us with valuable and detailed comments and suggestions which have brought great improvements to this manuscript. Also, they would like to thank Prof. C. J. Zhu (CCNU, School of Mathematics and Statistics) and Dr. H. Y. Wen (CCNU, School of Mathematics and Statistics) for helpful discussions and suggestions very much.
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Authors’ contributions
JCC is in charge of Section 2 and participated in the computation and discussion of the main theorem, Section 3. CH is responsible for the Section 3. This paper was finished under our joint efforts. We made many modifications and approve the final manuscript together. All authors read and approved the final manuscript.
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Keywords
 VlasovFokkerPlanck equation
 anisotropic space
 Hardy inequality
 energy method