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Shuai Xi

Publications and source records attributed to Shuai Xi.

3 recordsLinked to original sources

High Order Asymptotic Expansion at Infinity for Strong Solutions to Incompressible Navier-Stokes Equations

We discuss an interesting distinction between the incompressible Navier-Stokes equations (the velocity equations) and its vorticity form in whole space. We show that if the initial vorticity has a Gaussian bound then the bound is inherited up to the maximal lifespan of the strong solution. However, it turns out that the velocity equations don not share the same property. In fact, $L^p$-strong solutions to the velocity equations arising from ``well-localized" initial value generally behave at infinity like derivatives (of order $\geq3$) of the fundamental solution of Laplacian. To show this, a clean expansion up to maximal lifespan is derived : \begin{align} u(x,t)=-\nabla\sum_{|\alpha|=0}^{d-1}\frac{(-1)^{|\alpha|}}{\alpha !}\partial^\alpha\partial_{i,j}^2\Gamma(x)\int_0^t{\rm M}_{\alpha}^{i,j}(s){\rm d}s+O\big(|x|^{-2d-1}\big)\nonumber \end{align} where ${\rm M}_{\alpha}^{i,j}(t):=\int_{\mathbb R^d}y^\alpha u^i(y,t)u^j(y,t){\rm d}y$ and $\Gamma$ is the fundamental solution of Laplacian. This improves the first order expansion given by L. Brandolese and F. Vigneron \cite{BV07}.

math.AP

Global mild solutions to three-dimensional magnetohydrodynamic system in Morrey spaces

In this article, the Cauchy problem of three-dimensional (3-D) incompressible magnetohydrodynamic system was investigated. If the initial $\mathcal{M}^{1,1}$ norms of the vorticity $ω$ and the current density $j$ are both sufficiently small, then some uniform estimates with respect to time for the coupling terms between the fluid and the magnetic field can be established, which lead to a global-in-time well-posedness of mild solutions in Morrey spaces via some effective arguments.

math.AP

Blow-up criterion for the $3$D non-resistive compressible Magnetohydrodynamic equations

In this paper, we prove a blow-up criterion in terms of the magnetic field $H$ and the mass density $ρ$ for the strong solutions to the $3$D compressible isentropic MHD equations with zero magnetic diffusion and initial vacuum. More precisely, we show that the $L^\infty$ norms of $(H,ρ)$ control the possible blow-up (see \cite{olga}\cite{zx}) for strong solutions, which means that if a solution of the compressible isentropic non-resistive MHD equations is initially smooth and loses its regularity at some later time, then the formation of singularity must be caused by losing the bound of the $L^\infty$ norm of $H$ or $ρ$ as the critical time approaches.

math.AP