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      ASYMPTOTIC BEHAVIOR OF GLOBAL SMOOTH SOLUTIONS FOR BIPOLAR COMPRESSIBLE NAVIER-STOKES-MAXWELL SYSTEM FROM PLASMAS?

      2015-11-21 07:11:39YuehongFENG馮躍紅
      關(guān)鍵詞:李新保障機(jī)制管理體制

      Yuehong FENG(馮躍紅)

      College of Applied Sciences,Beijing University of Technology,Beijing 100022,China Laboratoire de Math′ematiques,Universit′e Blaise Pascal,Clermont-Ferrand,63000,F(xiàn)rance

      Shu WANG(王術(shù))

      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(馮躍紅)

      College of Applied Sciences,Beijing University of Technology,Beijing 100022,China Laboratoire de Math′ematiques,Universit′e Blaise Pascal,Clermont-Ferrand,63000,F(xiàn)rance

      E-mail:fengyuehong001@163.com

      Shu WANG(王術(shù))

      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

      1 Introduction

      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 andˉn≥const.>0.Suppose(nν0-ˉn,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],F(xiàn)eng-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,F(xiàn)eng-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 andˉn≥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-ˉn 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.

      2 Global Existence

      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=ˉn+Nν>0. More precisely,sinceˉn≥const.>0 and we consider small solutions for which Nνis close to zero,we have nν=ˉn+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≤ˉn

      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≤ˉn2Cm,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≤ˉn2Cm,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≤ˉn

      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 Large Time Behavior

      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≤ˉn

      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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      [14]Matsumura A,Nishida T.The initial value problem for the equation of motion of compressible viscous and heat-conductive fluids.Proc Japan Acad,Ser A,1979,55:337-342

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      [16]Markowich P,Ringhofer C A,Schmeiser C.Semiconductor Equations.Springer,1990

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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.

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