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Volume 2012, Article ID 212786,7pages doi:10.1155/2012/212786

Research Article

Regularizing Model for the 2D MHD Equations with Zero Viscosity

Ensil Kang

1

and Jihoon Lee

2

1Department of Mathematics, Chosun University, Gwangju 501-759, Republic of Korea

2Department of Mathematics, Sungkyunkwan University, Suwon 440-746, Republic of Korea

Correspondence should be addressed to Jihoon Lee,[email protected] Received 1 March 2012; Accepted 9 April 2012

Academic Editor: Narcisa C. Apreutesei

Copyrightq2012 E. Kang and J. Lee. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

We consider the regularity of two dimensional incompressible magneto-hydrodynamics equations with zero viscosity. We provide an approximating system to the equations and prove global-in- time existence of classical solution to this approximating system. By using approximating system, a priori estimates for the equations can be justified.

1. Introduction

In this paper, we are concerned with regularity problem of solutions to the 2-dimensional incompressible magnetohydrodynamicsMHDequations with zero viscosity

ut u· ∇u∇p b· ∇b, x∈R2, t >0, bt−Δb u· ∇b b· ∇u, x∈R2, t >0,

∇ ·u∇ ·b0, x∈R2, t >0,

1.1

where u u1, u2,b b1, b2, and p are fluid velocity vector field, magnetic field, and pressure function. The underlying idea of MHD is that dynamics of magnetic field induces the force on the fluid and, in turn, the motion of the conducting fluid affects the dynamics of magnetic field. MHD has many applications in electromagnetics, plasma theory, and cosmology. MHD equations describe the dynamics of the conducting fluids and thus, MHD equations are expressed as the combinations of the fluid equations and Maxwell system. We restrict our interest on the incompressible Euler equationwith Lorentz force of magnetic fieldas the fluid equation. This is the special case that the fluid viscosity is quite smaller

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than the magnetic diffusivity. Recall that magnetic Prandtl number is approximately the ratio of viscosity and magnetic diffusivity. So1.1represents the zero magnetic Prandtl number case. In physics, liquid metal usually has the small magnetic Prandtl number. For the two- dimensional incompressible MHD equations with positive viscosity and magnetic diffusivity, it is well known that there exists a unique global classical solution for every initial data u0, b0Hm with m ≥ 2 and∇ ·u0 ∇ ·b0 0see1,2 . But if viscosity of the fluid or the magnetic diffusivity is zero, then the global regularity issue for 2D remains as an open problem. For the case that viscosity is positive and the magnetic diffusivity is zero, then there are some studies on the regularity or blow-up criterion. We briefly recall a few of them. In 3 , the authors showed that ifT

0 ∇ ×ωLdt <∞, then the solutionu, bremain smooth on 0, T . In4 , the authors showed that ifT

0 ∇ ×bBMOdt <∞, then the solutionu, bremain smooth on0, T . In5 , it was shown that ifT

0bBMOdt < ∞, then the solutionu, b remain smooth on0, T . For the case that the viscosity is zero and the magnetic diffusivity is positive, that is, for the system1.1, we have better a prior estimates. In6–8 , the authors obtained the global existence of more regular weak solution, that is, we haveuL0, T;H1 andbL0, T;H1L20, T;H02for anyT >0.

But still the global existence of smooth solution is remained as a challenging open problem. Only some blow-up criterion for the system 1.1is known. In 7 , Cao and Wu showed that if for someT >0,

sup

q≥2

1 q

T

0

∇uLqdt <∞, 1.2

thenu, bremains smooth on0, T . Also Lei and Zhou8 obtained the regularity criterion in terms of theL10, T; BMO norm of∇ × ω. In6 , Kozono studied the stability of the solution to1.1 see9 also. And in10 , the authors studied the 2D incompressible MHD equations with horizontal dissipation and horizontal magnetic diffusion.

In this paper, we consider approximating system of1.1, which still preserves some properties of1.1. We consider

tu u· ∇u∇p −Δ−αb· ∇b,

tb u· ∇b−Δb b· ∇

−Δ−αu ,

∇ ·u∇ ·b0.

1.3

We study the regularity issue for1.3. We can rewrite1.3into the equations of the vorticity ω∂1u22u1and the current densityj∂1b22b1as follows:

ωt u· ∇ω −Δ−α

b· ∇j

, x∈R2, t >0, jt u· ∇j−Δj b· ∇−Δ−αω2b1

1 −Δ−α

1u12b2

1 −Δ−α

1u2

1b1

1 −Δ−α

2u11b2

1 −Δ−α

2u2, x∈R2, t >0.

1.4

We state our main results.

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Theorem 1.1. Assumeu0, b0H3 and ∇ ·u0 ∇ ·b0 0. Then for any T > 0 andα ∈ 0,1/2, there exists a unique solutionu, b∈L0, T;H3×L0, T;H3L20, T;H04of1.3.

Furthermore, there exist constantsCandDsatisfying

uL0,T;H3bL0,T;H3bL20,T;H40DeCT, 1.5

whereCandDdepend onu0H3,b0H3, andα.

2. Global-in-Time Existence of Smooth Solution

To proveTheorem 1.1, we present some regularity criterion for the solution to1.3. The proof is standard and very similar to the criterion in7,8 . But for the readers’ sake, we provide the sketch of the proof.

Proposition 2.1. Assume the initial datau0, b0H3,∇ ·u0 0 and∇ ·b0 0. Letu, bbe the corresponding solution of 1.3. If, for someT >0,

T

0

ωtLdt <∞, 2.1

thenu, bis regular on0, T , namely,u, b∈C0, T ;H3.

Proof. We provide brief sketch of proof. If we take3 operator on the fluid equations and magnetic field equations and take inner product with∇3uand ∇3b, respectively, then we obtain

1 2

d dt

3u2

L23b2

L2

4b2

L2

R23u· ∇u∇3u dx

R23−Δ−αb· ∇b∇3u dx

R23u· ∇b∇3b dx

R23

b· ∇−Δ−αu

3b dx.

2.2

There are some cancellation properties, that is,

R2u· ∇∇3u· ∇3u dx0,

R2−Δ−α b· ∇∇3b

3u dx

R2 b· ∇∇3b

3−Δ−αu dx

R2 b· ∇∇3−Δ−αu

3b dx.

2.3

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Using the previous cancellation, we have 1

2 d dt

3u2

L23b2

L2

4b2

L2C∇uL

3u2

L22b2

L2

. 2.4

Then recall the following Beale-Kato-Majda’s logarithmic inequality11 ,

∇uLL1ln1uH3. 2.5

We have the conclusion via Gronwall type inequality.

We provide the Proof ofTheorem 1.1.

Proof ofTheorem 1.1. For simplicity of the exposition, the calculations are presented on 0 smooth solutions. All the calculations can be justified by using continuation method of the local solutions. If we multiply both sides of the first and second equations of1.4byωand j, respectively, and integrate overR2, then we have

1 2

d

dtω2L2

R2b· ∇j·−Δ−αω dx, 1

2 d dtj2

L2∇j2

L2

R2b· ∇−Δ−αω·j dxC

R2|∇u||∇B|jdx

R2b· ∇−Δ−αω·j dxC∇uL2j2

L4.

2.6

Since we have

R2b· ∇−Δ−αω·j dx

R2b· ∇−Δ−αj·ω dx, 2.7 we obtain the following by adding the above inequalities:

1 2

d

dt ω2L2j2

L2

∇j2

L2C∇uL2j2

L4

L2j

L2∇j

L2

2L2j2

L2 1 2∇j2

L2.

2.8

By using Gronwall’s inequality, we have sup

0≤t≤T ωt2L2jt2

L2

T

0

∇jt2

L2dt

≤ ω02L2j02

L2

exp

C

T

0

j2

L2dt

.

2.9

Then we obtainωL0, T;L2andjL0, T;L2L20, T;H1.

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By standardLp,qestimate of the Stokes system or heat equationsee12,13 , we have t

0

∇jqLpdtC t

0

b· ∇

−Δ−αuq

LpdtCj0

H2, 2.10

for anyp, q∈1,∞. We also recall the following inequality:

b· ∇

−Δ−αu

Lp ≤ bL2puW1−2α,2p

0 . 2.11

SincejL0, T;L2L20, T;H1,bL0, T;L2pforp <∞. Then we have t

0

∇jq

LpdtC t

0

uq

W01−2α,2pdtC. 2.12

If we consider a usual trajectory map Xx, t such that dX/dtx, t uXx, t, t and Xx,0 x, then we can rewrite the first equation of1.4as

d

dtωXx, t, t −Δ−α∇ ·

bjXx, t, t

. 2.13

Thus we have

sup

0≤t≤TωLr ≤ ω0Lr t

0

bj

W1−2α,rdt, 2.14

for anyr∈1,∞ .

From the calculus inequality, we have bj

W1−2α,rC

bL2rj

W1−2α,2rbW1−2α,2rj

L2r

. 2.15

Forr∈2,∞andp≥2r/1αr, by Sobolev inequality, we have j

W1−2α,2rCj

W1,p0 Cj

L2. 2.16

For the caser∞, we choosepsuch thatαp >1, then we have j

W1−2α,∞Cj

W01,pCj

L2. 2.17

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Hence for anyr <∞andp≥2r/1αr, we have

sup

0≤t≤TωLr ≤ ω0Lr C T

0

bL2rj

W1−2α,2rbW1−2α,2rj

L2rdt

≤ ω0Lr C T

0

j

W01,pdtC

.

2.18

SincejL0, T;L2L20, T;H01, we have the finiteness ofbL0,T;L2rbL20,T;W1−2α,r jL20,T;H1

0in the above inequality.

If we use2.12, then for anyq∈1,∞, we have

sup

0≤t≤TωLrCCTq−1/q T

0

uq

W01−2α,2pdt 1/q

. 2.19

If we choosepsuch that 4r/1αr≤2p≤r/1αrwe can choose suchpifr≥3/5α, then for anyq∈1,∞, we have

sup

0≤t≤TωLrCCTq−1/q T

0

ωqLrdt 1/q

. 2.20

By using Gronwall’s inequality, we have sup

0≤t≤TωLrC, 2.21

for anyr∈3/5α,∞. In turn, it gives the bound of∇jLq0,t;Lpfor allp, q∈1,∞.

Forr∞andp >1/α, we have

sup

0≤t≤TωL≤ ω0LC T

0

bLj

W1−2α,∞bW1−2α,∞j

Ldt

≤ ω0LrC T

0

j

W01,pdtC

.

2.22

We already have the finiteness of∇jL10,T;Lp; this gives our conclusion byProposition 2.1.

Remark 2.2. With the similar arguments in the proof ofTheorem 1.1and this approximating system, we can prove rigorously that the solutionu, bto1.1satisfiesuL0, T;W1,p andbL0, T;W1,pLq0, T;W02,pfor anyT >0 andp, q∈2,∞×1,∞as the remark in8 .

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Acknowledgment

J. Lee’s work was partly supported by the National Research Foundation of Korea NRF- 2009-0072320.

References

1 G. Duvaut and J.-L. Lions, “In´equations en thermo´elasticit´e et magn´etohydrodynamique,” Archive for Rational Mechanics and Analysis, vol. 46, pp. 241–279, 1972.

2 M. Sermange and R. Temam, “Some mathematical questions related to the MHD equations,”

Communications on Pure and Applied Mathematics, vol. 36, no. 5, pp. 635–664, 1983.

3 J. Fan and T. Ozawa, “Regularity criteria for the magnetohydrodynamic equations with partial viscous terms and the Leray-α-MHD model,” Kinetic and Related Models, vol. 2, no. 2, pp. 293–305, 2009.

4 Y. Zhou and J. Fan, “A regularity criterion for the 2D MHD system with zero magnetic diffusivity,”

Journal of Mathematical Analysis and Applications, vol. 378, no. 1, pp. 169–172, 2011.

5 Z. Lei, N. Masmoudi, and Y. Zhou, “Remarks on the blowup criteria for Oldroyd models,” Journal of Differential Equations, vol. 248, no. 2, pp. 328–341, 2010.

6 H. Kozono, “Weak and classical solutions of the two-dimensional magnetohydrodynamic equations,”

The Tohoku Mathematical Journal, vol. 41, no. 3, pp. 471–488, 1989.

7 C. Cao and J. Wu, “Two regularity criteria for the 3D MHD equations,” Journal of Differential Equations, vol. 248, no. 9, pp. 2263–2274, 2010.

8 Z. Lei and Y. Zhou, “BKM’s criterion and global weak solutions for magnetohydrodynamics with zero viscosity,” Discrete and Continuous Dynamical Systems A, vol. 25, no. 2, pp. 575–583, 2009.

9 E. Casella, P. Secchi, and P. Trebeschi, “Global classical solutions for MHD system,” Journal of Mathematical Fluid Mechanics, vol. 5, no. 1, pp. 70–91, 2003.

10 C. Cao, D. Regmi, and J. Wu, “The 2D MHD equations with horizontal dissipation and horizontal magnetic diffusion,” preprint.

11 J. T. Beale, T. Kato, and A. Majda, “Remarks on the breakdown of smooth solutions for the 3D Euler equations,” Communications in Mathematical Physics, vol. 94, no. 1, pp. 61–66, 1984.

12 Y. Giga and H. Sohr, “AbstractLPestimates for the Cauchy problem with applications to the Navier- Stokes equations in exterior domains,” Journal of Functional Analysis, vol. 102, no. 1, pp. 72–94, 1991.

13 V. A. Solonnikov, “Estimates of the solutions of the nonstationary Navier-Stokes system,” Zapiski Nauˇcnyh Seminarov Leningradskogo Otdelenija Matematiˇceskogo Instituta im. V. A. Steklova Akademii Nauk SSSR, vol. 38, pp. 153–231, 1973.

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