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Blow-up criterion for the compressible magnetohydrodynamic equations with vacuum

机译:真空可压缩磁流体动力学方程的爆破判据

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In this paper, the 3-D compressible magnetohydrodynamic (MHD) equations with initial vacuum or infinite electric conductivity is considered. We prove that the L-infinity norms of the deformation tensor D(u) and the absolute temperature theta control the possible blow-up (see [18,23]) of strong solutions, especially for the non-resistive MHD system when the magnetic diffusion vanishes. This conclusion means that if a solution of the compressible MHD equations is initially regular and loses its regularity at some later time, then the formation of singularity must be caused by losing the bound of D(u) or theta as the critical time approaches. The viscosity coefficients are only restricted by the physical conditions. Our criterion (see (1.17)) is similar to [17] for 3-D incompressible Euler equations and to [12] for 3-D compressible isentropic Navier-Stokes equations. (C) 2015 Elsevier Inc. All rights reserved.
机译:本文考虑具有初始真空或无限电导率的3-D可压缩磁流体动力学(MHD)方程。我们证明了变形张量D(u)的L-无穷大范数和绝对温度theta控制着强解的可能爆炸(参见[18,23]),尤其是对于非电阻MHD系统,当磁场扩散消失。该结论意味着,如果可压缩MHD方程的解最初是正则的,并且在以后的某个时间失去正则性,则奇异性的形成必定是由于随着临界时间的临近而失去了D(u)或theta的界线。粘度系数仅受物理条件的限制。我们的标准(请参阅(1.17))类似于[17]的3-D不可压缩的Euler方程和[12]的3-D可压缩的等熵Navier-Stokes方程。 (C)2015 Elsevier Inc.保留所有权利。

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