2020
DOI: 10.1002/mma.6596
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Regularity criteria for the 3D magnetohydrodynamics system involving only two velocity components

Abstract: This paper is dedicated to the regularity criteria of weak solutions to the three‐dimensional incompressible magnetohydrodynamics system in terms of only two velocity components. It is proved that the weak solution (u,b) is smooth on (0,T], provided that ∇u1,∇u2∈L43−2sfalse(0,T;trueB˙∞,∞−sfalse(ℝ3false)false).3emwith.3em0

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Cited by 8 publications
(3 citation statements)
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References 39 publications
(45 reference statements)
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“…Precisely, they showed if the velocity field satisfies 𝑢 ∈ 𝐿 then the weak solution of (1.1) is smooth on ℝ 3 × (0, 𝑇]. Then, this result was extended or improved by [10,43,44,51].…”
Section: Introduction and The Main Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Precisely, they showed if the velocity field satisfies 𝑢 ∈ 𝐿 then the weak solution of (1.1) is smooth on ℝ 3 × (0, 𝑇]. Then, this result was extended or improved by [10,43,44,51].…”
Section: Introduction and The Main Resultsmentioning
confidence: 99%
“…Precisely, they showed if the velocity field satisfies uLα,γ0.33emwith0.33em2αgoodbreak+3γgoodbreak≤1,0.33em0.33em3goodbreak<γgoodbreak≤,$$\begin{equation} u\in L^{\alpha ,\gamma }\text{ with }\frac{2}{\alpha }+\frac{3}{\gamma }\le 1,\text{ \ }3&lt;\gamma \le \infty , \end{equation}$$or uLα,γ0.33emwith0.33em2αgoodbreak+3γgoodbreak≤2,0.33em0.33em32goodbreak<γgoodbreak≤,$$\begin{equation} \nabla u\in L^{\alpha ,\gamma }\text{ with }\frac{2}{\alpha }+\frac{3}{ \gamma }\le 2,\text{ \ }\frac{3}{2}&lt;\gamma \le \infty , \end{equation}$$then the weak solution of (1.1) is smooth on R3×(0,T]$\mathbb {R}^{3}\times (0,T]$. Then, this result was extended or improved by [10, 43, 44, 51]. Global regularity can also be obtained by imposing conditions on the pressure [21, 40, 58].…”
Section: Introduction and The Main Resultsmentioning
confidence: 99%
“…Over the past decade, more and more researchers are interested in investigating the regularity criteria for the MHD equations in terms of partial components or partial derivatives of the velocity field, the magnetic field, or the pressure, see, for example, the literature 28‐39 . Ji‐Lee 37 obtained a regularity condition in terms of horizontal components of the velocity field and the magnetic field, that is, rightleftuhLp(0,T;Lq(3)),bhLs(0,T;Lt(3)),rightrightleft2p+3q=1,2s+3t=1,3<q,t, where fh:=false(f1,f2false).…”
Section: Introductionmentioning
confidence: 99%