Yuehong FENG(冯跃红)
College of Applied Sciences,Beijing University of Technology,Beijing 100022,China Laboratoire de Math´ematiques,Universit´e Blaise Pascal,Clermont-Ferrand,63000,France
Shu WANG(王术)
College of Applied Sciences,Beijing University of Technology,Beijing 100022,China
Xin LI(李新)
Department of Mathematics and Computer Science,Xinyang Vocational and Technical College,
Xinyang 464000,China
ASYMPTOTIC BEHAVIOR OF GLOBAL SMOOTH SOLUTIONS FOR BIPOLAR COMPRESSIBLE NAVIER-STOKES-MAXWELL SYSTEM FROM PLASMAS∗
Yuehong FENG(冯跃红)
College of Applied Sciences,Beijing University of Technology,Beijing 100022,China Laboratoire de Math´ematiques,Universit´e Blaise Pascal,Clermont-Ferrand,63000,France
E-mail:fengyuehong001@163.com
Shu WANG(王术)
College of Applied Sciences,Beijing University of Technology,Beijing 100022,China
E-mail:wangshu@bjut.edu.cn
Xin LI(李新)
Department of Mathematics and Computer Science,Xinyang Vocational and Technical College,
Xinyang 464000,China
E-mail:lixin91600@163.com
This paper is concerned with the bipolar compressible Navier-Stokes-Maxwell system for plasmas.We investigated,by means of the techniques of symmetrizer and elaborate energy method,the Cauchy problem in R3.Under the assumption that the initial values are close to a equilibrium solutions,we prove that the smooth solutions of this problem converge to a steady state as the time goes to the infinity.It is shown that the difference of densities of two carriers converge to the equilibrium states with the norm‖·‖Hs-1,while the velocities and the electromagnetic fields converge to the equilibrium states with weaker norms than‖·‖Hs-1.This phenomenon on the charge transport shows the essential difference between the unipolar Navier-Stokes-Maxwell and the bipolar Navier-Stokes-Maxwell system.
bipolar compressible Navier-Stokes-Maxwell system;plasmas;global smooth solutions;energy estimates;large-time behavior
2010 MR Subject Classification 35L45;35L60;35Q60
The Navier-Stokes-Maxwell system is used to simulate the transport of viscosity charged particles in plasmas[1,5,10,16,23].Usually,it takes the form of compressible Navier-Stokesequations forced by the electromagnetic fields,which is governed by the self-consistent Maxwell equations.In this paper,we consider the Cauchy problem for the bipolar compressible Navier-Stokes-Maxwell system:
for ν=e,i.Here qe=-1(qi=1)is the charge of electrons(ions).The unknowns are the density nν>0,the velocity uν=(uν1,uν2,uν3),the pressure function pνwith p′ν(nν)>0 for ν=e,i,the electric field E=(E1,E2,E3)and the magnetic field B=(B1,B2,B3).Moreover,the constants mν> 0,ην>0,λ>0,1γ=c= (ε0µ0)-1/2,ε0andµ0are the mass,the viscosity coefficient,the scaled Debye length,the speed of light,the vacuum permittivity and permeability,respectively.Throughout this paper,we set mν=ην=λ=γ=1 without loss of generality.This is not an essential restriction in the investigation of global existence of smooth solutions for system(1.1).
For smooth solutions with nν>0,the second equation of(1.1)is equivalent to
where hνis the enthalpy function defined by h′ν(nν)=1nνp′ν(nν).Since pνis strictly increasing on(0,∞),so is hν.
Then system(1.1)is equivalent to
Initial conditions are given as
which satisfy the compatibility conditions:
The bipolar compressible Navier-Stokes-Maxwellsystem(1.2)is a symmetrizable hyperbolic parabolic system for nν>0.Then,according to the result of Kato[11]and the pioneering work of Matsumura-Nishida[14,15],the Cauchy problem(1.2)-(1.3)has a unique local smooth solution when the initial data are smooth.Here we are concerned with stabilities of global smooth solutions to(1.2)-(1.3)around a constant state being a particular solution of(1.2).It is easy to see that this constant state is necessarily given by
Proposition 1.1(Local existence of smooth solutions,see[11,13-15])Assume(1.4)holds.Let s≥4 be an integer and¯n≥const.>0.Suppose(nν0-¯n,uν0,E0,B0)∈Hs?R3?with nν0≥2κ for some given constant κ>0.Then there exists T>0 such that problem(1.2)-(1.3)has a unique smooth solution satisfying nν≥κ in[0,T]×R3and
There are some mathematical investigations on the equations arising from plasmas.For one-dimensional isentropic Euler-Maxwell equations,Chen-Jerome-Wang[2]proved the global existence of weak solutions by using the compensated compactness method.For the threedimensional Euler-Maxwell equations,the existence of global smooth solutions with small amplitude to the periodic problem in the torus and to the Cauchy problem in R3is established by Ueda-Wang-Kawashima[26],Peng-Wang-Gu[22],Peng[18]and Xu[29],respectively.The decay rate of the smooth solution when time goes to infinity is discussed by Duan[4],Duan-Liu-Zhu[6],Feng-Wang-Kawashima[8],Wang-Feng-Li[27,28]and Ueda-Kawashima[25].For asymptotic limits with parameters,see[19-21,30]and references therein.For numerical analysis,see[3].In the case without damping,an additional relation B=∇×u was made in[9]to establish such a global existence result.Indeed,the variable B-∇×u is time invariant and the reduced linearized Euler-Maxwell system is of Klein-Gordon type,then its solution has a time decay of rate O(t-3/2).
For unipolar compressible Navier-Stokes-Maxwell system,by using the Green's function argument,Duan[5]proved the global existence and asymptotic behavior of smooth solutions around a steady state.For non-isentropic Navier-Stokes-Maxwell system,Feng-Peng-Wang[7]established the global existence and asymptotic behavior of smooth solutions,recently.To the authors'best knowledge,there are few analysis on the asymptotics and global existence for the bipolar Navier-Stokes-Maxwell system yet.The objective of this paper is to establish such a result.
The main results can be stated as follows.
Theorem 1.2(Global existence of smooth solutions) Let s≥4 be an integer.Assume(1.4)holds and¯n≥const.>0.Then there exist constants δ0>0 small enough,independent of any given time t>0,such that if
the Cauchy problem(1.2)-(1.3)has a unique global solution
Theorem 1.3(Large-time behavior of smooth solutions)Under the assumptions of Theorem 1.2,the global smooth solution satisfies
and
Remark 1.4 It should be emphasized that the velocity viscosity term of the bipolar Navier-Stokes-Maxwell system(1.2)plays a key role in the proof of Theorem 1.2.
Remark 1.5 Similarly,we may establish estimates(1.8)and(1.9)for the smooth solutions of the unipolar Navier-Stokes-Maxwell system.This implies the large-time behavior of the electromagnetic field in that case.
The proof of Theorem 1.2 and Theorem 1.3 based on techniques of symmetrizer and elaborate weighted energy method.It should be pointed out that the bipolar compressible Navier-Stokes-Maxwell system is much more complex than the unipolar compressible Navier-Stokes-Maxwell system.For example,Duan[5]introduced a new variable and reduced directly the unipolar Navier-Stokes-Maxwell system to a symmetric system by using a scaling technique. However,this technique doesn't work for the bipolar Navier-Stokes-Maxwell system due to the complexity of the coupled ions equations.To overcome this difficulty,we choose a new symmetrizer.Now,let us explain the main difference of proofs in the unipolar and bipolar Navier-Stokes-Maxwell systems.From(1.2),it is easy to see that∇uνis dissipative.By using the weighted energy method,we obtain an energy estimate for∇uνin L2?[0,T];Hs?R3??(see Lemma(2.4)).The key step for proving the global existence with asymptotic properties of solutions is to control nν-¯n in L2?[0,T];Hs?R3??.In the unipolar Navier-Stokes-Maxwell system[5],this is achieved in estimate
The rest of this paper is arranged as follows.In Section 2,we deal with the global existence for smooth solutions.The main goal is to prove Theorem 1.2 by establishing energy estimates. In Section 3,we complete the proof of Theorem 1.3 by establishing dissipations estimates for electromagnetic field,and the large-time behavior of the solutions is presented.
It is well known that the global existence of smooth solutions follows from the local existence and uniform estimates of solutions with respect to t.The main task of this section is devoted to the uniform estimates for proving Theorems 1.2.
2.1 Preliminary
We first introduce some notations for later use.The expression f~g means γg≤f≤1γg for a constant 0<γ<1.We denote by‖·‖sthe norm of the usual Sobolev space Hs(R3),andby‖·‖and‖·‖∞the norms of L2(R3)and L∞(R3),respectively.We also denote by<·,·>the inner product over L2(R3).For a multi-index α=(α1,α2,α3)∈N3,we denote
For α=(α1,α2,α3)and β=(β1,β2,β3)∈N3,β≤α stands for βj≤αjfor j=1,2,3,and β<α stands for β≤α and β/=α.
The Leibniz formulas
where Cβα>0 for β<α are constants.
The following Lemmas will be needed in the proof of Theorem 1.2.
Lemma 2.1(Moser-type calculus inequalities,see[12,13]) Let s≥1 be an integer. Suppose u∈Hs(R3),∇u∈L∞(R3)and v∈Hs-1(R3)∩L∞(R3).Then for all multi-index α with 1≤|α|≤s,one has∂α(uv)-u∂αv∈L2(R3)and
where
Furthermore,if s≥3,then the embedding Hs-1(R3)→L∞(R3)is continuous and we have
and for all smooth function f and u,v∈Hs(R3),
Lemma 2.2(see[7])For∇u∈H1,there exists a constant C>0 such that
Suppose(nν,uν,E,B)is a smooth solution of Cauchy problem for the bipolar Navier-Stokes-Maxwell system(1.2)with initial conditions(1.3)which satisfies(1.4).
Set
and
Using(2.1),system(1.2)can be written as
Furthermore,using(2.2),the Navier-Stokes equations of(2.3)can be rewritten as
with
where(e1,e2,e3)is the canonical basis of R3,I3is the 3×3 unit matrix,Vjdenotes the jth component of V∈R3.
It is clear that(2.4)for Uνis symmetrizable hyperbolic parabolic when nν=¯n+Nν>0. More precisely,since¯n≥const.>0 and we consider small solutions for which Nνis close to zero,we have nν=¯n+Nν≥const.>0.Let
Then
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Since Aν0is symmetric positively definite and˜Aνjis symmetric for all 1≤j≤3,system(2.4)is symmetrizable hyperbolic parabolic.
Let T>0 and W be a smooth solution of(2.3)defined on time interval[0,T]with initial data W0.This local solution is given by Proposition 1.1.From now on,we define
and by C >0 various constants independent of any time t and T.From the continuous embedding Hs(R3)→L∞?R3?for s≥2,there exists a constant Cm>0 such that
Moreover,by Lemma 2.1,for any smooth function g one has
Note that in the proof of Lemmas 2.3-2.5,we only suppose
2.2 Energy Estimates
In this subsection,we establish the classical energy estimate for W.The first lemma concerns the zero order energy estimate.
Lemma 2.3 Under the assumptions of Theorem 1.2,if ωT≤¯n
Proof Taking the inner product of(2.4)with 2Aν0(nν)Uνin L2?R3?yields the classical energy equality for Uν:
where
Since
using the first equation of(2.3),Lemma 2.2 and ωT≤¯n2Cm,we have
Then,
Now,let us estimate each term on the right hand side of(2.9).For the first term,using(2.5),(2.10),(2.11)and Lemma 2.2,we get
and then
For the last two terms,using(2.6),the fact that uν·(uν×B)=0 and an integration by parts,we have
Therefore,
On the other hand,a standard energy estimate for the Maxwell equations of(2.3)yields
Hence,the cancellation of the termneue-niui,Ein(2.12)and(2.13)exists.The sum of(2.12)and(2.13)for ν=e,i,we obtain
Therefore,(2.8)follows from integrating(2.14)over(0,t)with t∈[0,T].This completes the proof of Lemma 2.3. □
For Navier-Stokes equations in(2.3),we define the dissipation function Ds(t)by
Lemma 2.4 Under the assumptions of Theorem 1.2,if ωT≤¯n2Cm,it holds
Proof For α∈N3with 1≤|α|≤s.Applying∂αto(2.4)and multiplying the resulting equations by the symmetrizer matrix Aν0(nν),we have
where
Taking the inner product of(2.17)with 2∂αUνin L2(R3),we obtain
Using(2.10),(2.11)and the definition of,we have
Now,let us estimate each term on the right hand side of(2.19).For the first two terms,it follows from(2.18),(2.20)and Cauchy-Schwarz inequality that
For the last term,using(2.6),Leibniz formulas,Lemma 2.1 and Lemma 2.2,it holds
and
Then,
This inequality together with(2.19)and(2.21)yields
On the other hand,an easy high order energy estimate for the Maxwell equations of(2.3)gives
Due to the choice of symmetrizer)we see that the cancellation of the term
in(2.22)and(2.23)exists.It follows from(2.22)and(2.23)that
Noting the fact that
summing(2.24)for all α with 1≤|α|≤s,and then integrating over[0,t],together with(2.8),we get(2.16).This completes the proof of Lemma 2.4. □
Estimate(2.16)stands for the dissipation of∇uν.It is clear that this estimate is not sufficient to control the high order term on the right hand side of(2.16)and the dissipation estimates of Nνis necessary.
Lemma 2.5 Under the assumptions of Theorem 1.2,if ωT≤¯n
2Cm,there exist positive constants C1and C2,independent of t and T,such that
Proof For α∈N3with|α|≤s-1,applying∂αto the second equation of(2.3),and then taking the inner product of the resulting equation with∇∂αNνin L2?R3?,we have
where
Now,let us estimate each term in(2.26).First,noting thatand hνis a strictly increasing function on(0,+∞),we haveHence,
Next,using the first equation of(2.3)and an integration by parts,we get
When|α|=0,from Lemma 2.2 and Cauchy-Schwarz inequality,we have
And when|α|≥1,it follows similarly that
These last two inequalities together with(2.26)-(2.28)yields
Summing up this inequality for all|α|≤s-1 and choosing ε>0 small enough,so that the term ε||∂αNν||2can be controlled by that in the left hand side.Hence,integrating the resulting equation over[0,t],we have
Finally,
and
Therefore,together with(2.16),we obtain(2.25).This completes the proof of Lemma 2.5.□
Proof of Theorem 1.2 By Lemma 2.5,we find that if C2ωT<1,the integral term on the right hand side of(2.25)may be controlled by that of the left hand side.It follows that
Then,it suffices to choose a constant δ0small enough such that
3.1 Dissipation of the Electromagnetic Fields
The large time behavior of smooth solutions follows from uniform energy estimates of Nν,∇uν,∇E and∇2G with respect to T in L2([0,T];Hs′(R3))
for appropriate integers s′≥1.We establish these estimates in the following two lemmas.
Proof For α∈N3with 1≤|α|≤s-1,applying∂αto the second equation of(2.3)and taking the inner product of the resulting equations with∂αE in L2(R3),we have
where
and
Using the electric field equation in(2.3),Cauchy-Schwarz inequality and an integration by parts,we obtain
Similarly as before,we obtain
It follows from(3.2)-(3.4)that
Summing up this inequality for all α with 1≤|α|≤s-1 and taking ε>0 so small that the term ε‖∂αE‖2can be controlled by that in the left hand side,and then integrating the resulting equation over[0,t],using(2.25)and noting the fact that for all t∈[0,T],
we obtain(3.1).This completes the proof of Lemma 3.1. □
Lemma 3.2 Under the assumptions of Theorem 1.2,if if ωT≤¯n
2Cmfor all t∈[0,T],it holds
Proof For α∈N3with 1≤|α|≤s-2,applying∂αto the electric field equation in(2.3)and taking the inner product of the resulting equation with-∇×∂αB,we obtain
Note that for all t∈[0,T],
Let ε>0 be small enough,integrating(3.6)over[0,T]and summing for all 1≤|α|≤s-2,together with(3.1),we get(3.5).In this estimate we have used
for 1≤i≤3,due to the fact that∇·B=0 and∂i△-1∇is bounded from Lpto itself with 1<p<∞,see[24].This completes the proof of Lemma 3.2. □3.2 Proof of Theorem 1.3
Recall the following Lemma that is used in the following.
Lemma 3.3 Let f:(0,+∞)→ R be a uniformly continuous function such that f∈ThenIn particular,the conclusion holds when f∈L1(0,+∞)∩W1,+∞(0,∞).
Now let us establish the large time behavior of solutions and complete the proof of Theorem 1.3.From Lemma 2.5,there exists a constant δ0such that if ωT≤δ0,it holds
Since ne-ni=Ne-Niand∇nν=∇Nν,this together with(2.15)implies that
Using the Navier-Stokes equations in(2.3),we obtain
Then
which imply(1.6)-(1.7).
Similarly as before,from(3.5)and(3.7),we get
It follows from the Maxwell equations in(2.3)that
Therefore,
which implies(1.8).We further deduce that
Then
which implies(1.9).This completes the proof of Theorem 1.3. □
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∗Received October 30,2014;revised February 14,2015.The authors are supported by the Collaborative Innovation Center on Beijing Society-building and Social Governance,NSFC(11371042),BNSF(1132006),the key fund of the Beijing education committee of China and China Postdoctoral Science Foundation funded project.
Acta Mathematica Scientia(English Series)2015年5期