Blow-up criteria for smooth solutions to the generalized 3D MHD equations
© Hu and Wang; licensee Springer 2013
Received: 22 April 2013
Accepted: 5 August 2013
Published: 21 August 2013
In this paper, we focus on the generalized 3D magnetohydrodynamic equations. Two logarithmically blow-up criteria of smooth solutions are established.
Here , and are non-dimensional quantities corresponding to the flow velocity, the magnetic field and the total kinetic pressure at the point , while and are the given initial velocity and initial magnetic field with and , respectively.
The GMHD equations is a generalized model of MHD equations. It has important physical background. Therefore, the GMHD equations are also mathematically significant. For 3D Navier-Stokes equations, whether there exists a global smooth solution to 3D impressible GMHD equations is still an open problem. In the absence of global well-posedness, the development of blow-up/ non blow-up theory is of major importance for both theoretical and practical purposes. Fundamental mathematical issues such as the global regularity of their solutions have generated extensive research and many interesting results have been established (see [1–5]).
When , (1.1) reduces to MHD equations. There are numerous important progresses on the fundamental issue of the regularity for the weak solution to (1.1), (1.2) (see [6–18]). A criterion for the breakdown of classical solutions to (1.1) with zero viscosity and positive resistivity in was derived in . Some sufficient integrability conditions on two components or the gradient of two components of and in Morrey-Campanato spaces were obtained in . A logarithmal improved blow-up criterion of smooth solutions in an appropriate homogeneous Besov space was obtained by Wang et al. . Zhou and Fan  established various logarithmically improved regularity criteria for the 3D MHD equations in terms of the velocity field and pressure, respectively. These regularity criteria can be regarded as log in time improvements of the standard Serrin criteria established before. Two new regularity criteria for the 3D incompressible MHD equations involving partial components of the velocity and magnetic fields were obtained by Jia and Zhou .
When , , (1.1) reduces to Navier-Stokes equations. Leray  and Hopf  constructed weak solutions to the Navier-Stokes equations, respectively. The solution is called the Leray-Hopf weak solution. Later on, much effort has been devoted to establish the global existence and uniqueness of smooth solutions to the Navier-Stokes equations. Different criteria for regularity of the weak solutions have been proposed and many interesting results have been obtained [21–25].
In the paper, we obtain two logarithmically blow-up criteria of smooth solutions to (1.1), (1.2) in Morrey-Campanato spaces. We hope that the study of equations (1.1) can improve the understanding of the problem of Navier-Stokes equations and MHD equations.
Now we state our results as follows.
then the solution can be extended beyond .
We have the following corollary immediately.
then the solution can be extended beyond .
We have the following corollary immediately.
The paper is organized as follows. We first state some preliminaries on function spaces and some important inequalities in Section 2. Then we prove main results in Section 3 and Section 4, respectively.
Before stating our main results, we recall the definition and some properties of the homogeneous Morrey-Campanato space.
where denotes the ball of center x with radius R.
where the infimum is taken over all possible decompositions.
Lemma 2.1 Let and p, q satisfy . Then is the dual space of .
The following lemma comes from .
where and .
The following inequality is the well-known Gagliardo-Nirenberg inequality.
with the following exception: if and is a nonnegative integer, then (2.2) holds only for a satisfying .
3 Proof of Theorem 1.1
In what follows, for simplicity, we set .
Gronwall’s inequality implies the boundedness of -norm of u and B provided that , which can be achieved by the absolute continuous property of integral (1.3). We have completed the proof of Theorem 1.1. □
4 Proof of Theorem 1.2
From (4.11), estimate for this case is the same as that for Theorem 1.1. Thus, Theorem 1.2 is proved. □
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