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Article

A Blow-Up Criterion for the Density-Dependent Incompressible Magnetohydrodynamic System with Zero Viscosity

1
College of Sciences, Nanjing Forestry University, Nanjing 210037, China
2
Department of Applied Mathematics, Nanjing Forestry University, Nanjing 210037, China
3
Department of Mathematics, Hokkaido University, Sapporo 060-0810, Japan
*
Author to whom correspondence should be addressed.
Mathematics 2024, 12(10), 1510; https://doi.org/10.3390/math12101510
Submission received: 16 April 2024 / Revised: 9 May 2024 / Accepted: 11 May 2024 / Published: 12 May 2024

Abstract

:
In this paper, we provide a blow-up criterion for the density-dependent incompressible magnetohydrodynamic system with zero viscosity. The proof uses the L p -method and the Kato–Ponce inequalities in the harmonic analysis. The novelty of our work lies in the fact that we deal with the case in which the resistivity η is positive.

1. Introduction

Magnetohydrodynamics (MHD) is concerned with the study of applications between magnetic fields and fluid conductors of electricity. The application of magnetohydrodynamics covers a very wide range of physical objects, from liquid metals to cosmic plasmas.
We consider the following 3D density-dependent incompressible magnetohydrodynamic system:
t ρ + u · ρ = 0 ,
ρ t u + ρ ( u · ) u + π = rot b × b ,
t b + u · b b · u = η Δ b ,
div u = 0 , div b = 0 in R 3 × ( 0 , ) ,
lim | x | ( ρ , u , b ) = ( 1 , 0 , 0 ) ,
( ρ , u , b ) ( · , 0 ) = ( ρ 0 , u 0 , b 0 ) in R 3 .
The unknowns are the fluid velocity field u = u ( x , t ) , the pressure π = π ( x , t ) , the density ρ = ρ ( x , t ) , and the magnetic field b = b ( x , t ) . η > 0 is the resistivity coefficient. The term rot b × b in (2) is the Lorentz force with low regularity, and thus it is the difficult term.
For the case of b = 0 , there are many studies. Beirão da Veiga and Valli [1,2] and Valli and Zajaczkowski [3] proved the unique solvability, local in time, in some supercritical Sobolev spaces and Hölder spaces in bounded domains. It is worth pointing out that, in 1995, Berselli [4] discussed the standard ideal flow. Danchin [5] and Danchin and Fanelli [6] (see also [7,8]) proved the unique solvability, local in time, in some critical Besov spaces. Recently, Bae et al [9] showed a regularity criterion:
u L 1 ( 0 , T ; L ( R 3 ) ) .
This refined the previous blow-up criteria [5,6,7]:
ω : = rot u L 1 ( 0 , T ; B ˙ 2 , 1 d 2 ( R d ) ) ,
u L 1 ( 0 , T ; L ) and π L 1 ( 0 , T ; B , r s 1 ) , s 1 , 1 r .
In [10], the authors proved the local well-posedness of smooth solutions in Sobolev spaces. The aim of this article is to prove (7) for the system (1)–(6). We will prove the following.
Theorem 1.
Let 0 < inf ρ 0 ρ 0 C , ρ 0 H 2 , u 0 , b 0 H 3 with div u 0 = div b 0 = 0 in R 3 . Let ( ρ , u , b ) be the unique solution to the problem (1)–(6). If (7) holds true with some 0 < T < , then the solution ( ρ , u , b ) can be extended beyond T > 0 .
Remark 1.
In [8], Zhou, Fan and Xin showed the same blow-up criterion (8), which is refined by (7) for the ideal MHD system.
Remark 2.
When η = 0 , we are unable to show a similar result.
In the following proofs, we will use the bilinear commutator and product estimates due to Kato–Ponce [11]:
Λ s ( f g ) f Λ s g L p C ( f L p 1 Λ s 1 g L q 1 + g L p 2 Λ s f L q 2 ) ,
Λ s ( f g ) L p C ( f L p 1 Λ s g L q 1 + Λ s f L p 2 g L q 2 ) ,
with s > 0 , Λ : = ( Δ ) 1 2 and 1 p = 1 p 1 + 1 q 1 = 1 p 2 + 1 q 2 .

2. Proof of Theorem 1

We only need to prove a priori estimates.
First, thanks to the maximum principle, it is easy to see that
1 C ρ C .
We will use the identity
b · b + b × rot b = 1 2 | b | 2 .
Testing (2) by u, using (1), (4) and (13), we find that
1 2 d d t ρ | u | 2 d x = ( b · ) b · u d x .
Testing (3) by b and using (4), we obtain
1 2 d d t | b | 2 d x + η | b | 2 d x = ( b · ) u · b d x .
Summing up (14) and (15), we have the well-known energy identity
1 2 d d t ( ρ | u | 2 + | b | 2 ) d x + η | b | 2 d x = 0 ,
and hence
( | u | 2 + | b | 2 ) d x + 0 T | b | 2 d x d t C .
It is easy to deduce that
ρ L ρ 0 L exp 0 t u ( s ) L d s C .
Testing (3) by | b | q 2 b ( 2 < q < ) and using (4), we derive
1 q d d t b L q q + η | b | q 2 | b | 2 d x + η 1 2 | b | 2 · | b | q 2 d x = b · u · | b | q 2 b d x u L b L q q ,
and therefore
d d t b L q u L b L q ,
which gives
b L q b 0 L q exp 0 t u ( s ) L d s .
Taking q , one has
b L C .
(2) can be rewritten as
t u + u · u + 1 ρ π = 1 ρ rot b × b .
Testing (20) by π and using (4), it follows that
1 ρ | π | 2 d x = u · u · π d x + 1 ρ rot b × b · π d x C ( u · u L 2 + rot b × b L 2 ) π L 2 C ( u L 2 u L + b L b L 2 ) π L 2 ,
whence
π L 2 C u L + C b L 2 .
Taking rot to (20) and denoting the vorticity ω : = rot u , we obtain
t ω + u · ω = ω · u 1 ρ × π + rot rot b ρ × b .
Testing (22) by ω and using (4), (17) and (19), we compute
1 2 d d t | ω | 2 d x = ω · u · ω d x 1 ρ × π ω d x + rot rot b ρ × b · ω d x u L | ω | 2 d x + 1 ρ π L 2 ω L 2 + C ρ L b L b L 2 ω L 2 + C b L Δ b L 2 ω L 2 + C b L 4 2 ω L 2 C u L | ω | 2 d x + C π L 2 ω L 2 + C b L 2 ω L 2 + η 4 Δ b L 2 2 + C ω L 2 2 .
Here, we have used the Gagliardo–Nirenberg inequality
b L 4 2 C b L Δ b L 2 .
On the other hand, testing (3) by Δ b and using (4) and (19), we achieve
1 2 d d t | b | 2 d x + η | Δ b | 2 d x = j ( u · ) b j 2 b d x ( b · ) u · Δ b d x = j j u · b · j b d x b · u · Δ b d x C u L b L 2 2 + b L u L 2 Δ b L 2 η 4 Δ b L 2 2 + C u L b L 2 2 + C ω L 2 2 .
Here, we have used the inequality
u L r C ω L r with 1 < r < .
Summing up (23) and (25) and using (21) and the Gronwall inequality, we reach
ω L 2 + b L 2 C .
Taking div to (20) and using (4), we observe that
Δ π = f : = ρ div ( u · u ) + ρ 1 ρ · π ρ div rot b ρ × b ,
from which, with (17), (19), (21) and (27), we have
Δ π L 4 f L 4 C u L u L 4 + C ρ L π L 4 + C ρ L b L rot b L 4 + C Δ b L 4 b L + C b L 8 2 C u L ω L 4 + C π L 4 + C rot b L 4 + C Δ b L 4 C u L ω L 4 + C π L 2 4 7 Δ π L 4 3 7 + C rot b L 4 + C Δ b L 4 1 2 Δ π L 4 + C u L ω L 4 + C u L + C + C rot b L 4 + C Δ b L 4 ,
which yields
Δ π L 4 C u L ω L 4 + C u L + C + C rot b L 4 + C | Δ b L 4 .
Here, we have used the Gagliardo–Nirenberg inequalities
b L 8 2 C b L Δ b L 4 ,
π L 4 C π L 2 4 7 Δ π L 4 3 7 .
Testing (22) by | ω | 2 ω and using (4), (17), (19), (29), (30) and (31), we have
1 4 d d t ω L 4 4 C u L ω L 4 4 + C 1 ρ L π L 4 ω L 4 3 + C ( b L Δ b L 4 + b L 8 2 ) ω L 4 3 + C 1 ρ L b L rot b L 4 ω L 4 3 C u L ω L 4 4 + C π L 4 ω L 4 3 + C ( Δ b L 4 + rot b L 4 ) ω L 4 3 ,
which implies
d d t ω L 4 2 C u L ω L 4 2 + C ( u L + 1 + rot b L 4 + Δ b L 4 ) ω L 4 C u L ω L 4 2 + C ( u L + 1 + rot b L 4 ) ω L 4 + C ω L 4 2 + C Δ b L 4 2 ,
and thus
ω L 4 2 ω 0 L 4 2 + C 0 t [ ( u L + 1 ) ω L 4 2 + ( u L + 1 + rot b L 4 ) ω L 4 ] d s + 0 t Δ b L 4 2 d s .
On the other hand, using the L 2 ( 0 , T ; W 2 , 4 ) -theory of the heat equation, it follows that
0 t Δ b L 4 2 d s C + C 0 t u · b b · u L 4 2 d s C + C 0 t ( u L 2 b L 4 2 + b L 2 u L 4 2 ) d s C + C 0 t ( u L 6 4 3 u L 2 3 rot b L 4 2 + ω L 4 2 ) d s C + C 0 t ( u L 2 3 rot b L 4 2 + ω L 4 2 ) d s .
Here, we have used the inequality
b L p C rot b L p with 1 < p < .
Inserting (33) into (32), we have
ω L 4 2 C + C 0 t ( u L + ) ω L 4 2 d s + C 0 t ( u L + rot b L 4 ) ω L 4 d s + C 0 t u L 2 3 rot b L 4 2 d s .
Taking rot to (3) and denoting the current J : = rot b , we infer that
t J η Δ J + rot ( u · b b · u ) = 0 .
Testing (36) by | J | 2 J , using (17), (19) and (34), we derive
1 4 d d t J L 4 4 + η | J | 2 | J | 2 d x + η 1 2 | J | 2 · | J | 2 d x = ( b · u u · b ) rot ( | J | 2 J ) d x = ( b · u u · b ) ( | J | 2 rot J + | J | 2 × J ) d x b · u u · b L 4 J L 4 | J | · | J | L 2 C ( b L u L 4 + u L b L 4 ) J L 4 | J | · | J | L 2 η 2 | J | 2 | J | 2 d x + C ( ω L 4 2 + u L 2 J L 4 2 ) J L 4 2 ,
which implies
d d t J L 4 2 C ω L 4 2 + C u L 2 3 J L 4 2 .
Integrating the above inequality, one has
rot b L 4 2 C + C 0 t ( ω L 4 2 + u L 2 3 rot b L 4 2 ) d s .
Summing up (35) and (37), using the Gronwall inequality, we arrive at
u L 4 + b L 4 + 0 T Δ b L 4 2 d t C ,
u L + 0 T b L 2 d t C .
Applying Λ 3 to (1), testing by Λ 3 ρ and using (4) and (10), we obtain
1 2 d d t ( Λ 3 ρ ) 2 d x = ( Λ 3 ( u · ρ ) u · Λ 3 ρ ) Λ 3 ρ d x C ( u L Λ 3 ρ L 2 + ρ L Λ 3 u L 2 ) Λ 3 ρ L 2 .
Applying Λ 3 to (2), testing by Λ 3 u and using (1) and (4), we have
1 2 d d t ρ | Λ 3 u | 2 d x = ( Λ 3 ( b · b ) b · Λ 3 b ) Λ 3 u d x + b · Λ 3 b · Λ 3 u d x ( Λ 3 ( ρ t u ) ρ Λ 3 t u ) Λ 3 u d x ( Λ 3 ( ρ u · u ) ρ u · Λ 3 u ) Λ 3 u d x = : I 1 + I 2 + I 3 + I 4 .
Applying Λ 3 to (3), testing by Λ 3 b and using (4), we have
1 2 d d t | Λ 3 b | 2 d x + η | Λ 4 b | 2 d x = ( Λ 3 ( b · u ) b · Λ 3 u ) Λ 3 b d x + b · Λ 3 u · Λ 3 b d x ( Λ 3 ( u · b ) u · Λ 3 b ) Λ 3 b d x = : I 5 + I 6 + I 7 .
Summing up (41) and (42) and noting that I 2 + I 6 = 0 , we have
1 2 d d t ( ρ | Λ 3 u | 2 + | Λ 3 b | 2 ) d x + η | Λ 4 b | 2 d x = I 1 + I 3 + I 4 + I 5 + I 7 .
Using (10) and (11), we bound I 1 , I 4 , I 5 and I 7 as follows.
I 1 C b L ( Λ 3 b L 2 2 + Λ 3 u L 2 2 ) ; I 4 C ( ( ρ u ) L Λ 3 u L 2 + u L Λ 3 ( ρ u ) L 2 ) Λ 3 u L 2 C ( u L + 1 ) Λ 3 u L 2 2 + C u L ( Λ 3 u L 2 + u L Λ 3 ρ L 2 ) Λ 3 u L 2 C ( u L + 1 ) Λ 3 u L 2 2 + C u L Λ 3 ρ L 2 2 ; I 5 + I 7 C ( b L Λ 3 u L 2 + u L Λ 3 b L 2 ) Λ 3 b L 2 .
To bound I 3 , we proceed as follows.
I 3 C ( t u L Λ 3 ρ L 2 + ρ L Λ 2 t u L 2 ) Λ 3 u L 2 C u · u + 1 ρ π rot b ρ × b L Λ 3 ρ L 2 Λ 3 u L 2 + C Δ u · u + 1 ρ π rot b ρ × b L 2 Λ 3 u L 2 C ( u L + π L + b L ) Λ 3 ρ L 2 Λ 3 u L 2 + C u L Λ 3 u L 2 + Λ 2 π L 2 + π L 3 Λ 2 1 ρ L 6 + Δ 1 ρ L 6 rot b L 3 b L + b L Λ 3 b L 2 Λ 3 u L 2 C ( u L + π L + b L ) Λ 3 ρ L 2 Λ 3 u L 2 + C ( Λ 3 u L 2 + Λ 2 π L 2 + π L 3 Δ ρ L 6 + Δ ρ L 6 + Λ 3 b L 2 ) Λ 3 u L 2 C ( u L + π L + b L ) Λ 3 ρ L 2 Λ 3 u L 2 + C ( Λ 3 u L 2 + f L 2 + π L 3 Λ 3 ρ L 2 + Λ 3 ρ L 2 + Λ 3 b L 2 ) Λ 3 u L 2 .
On the other hand, we have
π L C π L 2 + C Δ π L 4 C u L + C + C Δ b L 4 ;
Δ π L 2 = f L 2 C ρ L u L 4 2 + C u L Λ 3 u L 2 + C ρ L 2 π L 2 + C Δ ρ L 6 π L 3 + C ρ L ( Δ b L 2 b L + b L 4 2 + ρ L b L 2 ) + C b L Λ 3 b L 2 + C Δ 1 ρ L 6 b L b L 3 C + C Λ 3 u L 2 + C 2 π L 2 + C Λ 3 ρ L 2 π L 3 + C Λ 3 b L 2 + C Λ 3 ρ L 2 1 2 f L 2 + C π L 2 + C + C Λ 3 u L 2 + C Λ 3 ρ L 2 + C Λ 3 b L 2 + C Λ 3 ρ L 2 π L 3 ,
which gives
f L 2 C + C u L + C Λ 3 ρ L 2 + C Λ 3 u L 2 + C Λ 3 b L 2 + C Λ 3 ρ L 2 ( π L 2 + Δ π L 4 ) C + C u L + C Λ 3 ( ρ , u , b ) L 2 + C Λ 3 ρ L 2 ( u L + 1 + Δ b L 4 ) .
Inserting the above estimates into (44), we obtain
I 3 C ( u L + 1 + b L + Δ b L 4 ) ( Λ 3 ρ L 2 2 + Λ 3 u L 2 2 ) + C Λ 3 ( ρ , u , b ) L 2 2 C ( u L + 1 + b L + Δ b L 4 ) Λ 3 ( ρ , u , b ) L 2 2 .
Inserting the above estimates of I 1 , I 3 , I 4 , I 5 and I 7 into (43), we have
1 2 d d t ( ρ | Λ 3 u | 2 + | Λ 3 b | 2 ) d x + η | Λ 4 b | 2 d x C ( u L + 1 + b L + Δ b L 4 ) Λ 3 ( ρ , u , b ) L 2 2 .
Summing up (40) and (46) and using the Gronwall inequality, we conclude that
Λ 3 ( ρ , u , b ) L 2 + 0 T | Λ 4 b | 2 d x d t C .
This completes the proof. □

3. Conclusions

In this paper, we prove a refined blow-up criterion for the inhomogeneous incompressible MHD system with zero viscosity, which is important and can be used for the simulation of MHD. For ρ = 1 and η = 0 , Caflisch et al. [12] showed the following regularity criterion:
rot u , rot b L 1 ( 0 , T ; L ) .
Since the problem is very challenging, we are unable to present further developments.

Author Contributions

Writing—original draft, K.S. and J.F.; Writing—review & editing, G.N. All authors have read and agreed to the published version of the manuscript.

Funding

J. Fan is partially supported by the NSFC (No. 11971234). The authors are indebted to the referees for their valuable suggestions.

Data Availability Statement

The data in this study are available from the corresponding author upon request.

Conflicts of Interest

The authors declare no conflict of interest.

References

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Shi, K.; Fan, J.; Nakamura, G. A Blow-Up Criterion for the Density-Dependent Incompressible Magnetohydrodynamic System with Zero Viscosity. Mathematics 2024, 12, 1510. https://doi.org/10.3390/math12101510

AMA Style

Shi K, Fan J, Nakamura G. A Blow-Up Criterion for the Density-Dependent Incompressible Magnetohydrodynamic System with Zero Viscosity. Mathematics. 2024; 12(10):1510. https://doi.org/10.3390/math12101510

Chicago/Turabian Style

Shi, Kunlong, Jishan Fan, and Gen Nakamura. 2024. "A Blow-Up Criterion for the Density-Dependent Incompressible Magnetohydrodynamic System with Zero Viscosity" Mathematics 12, no. 10: 1510. https://doi.org/10.3390/math12101510

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