Jinkai Ni — Page 2 | Searcharxiv

arXiv2024

Global existence and time decay of strong solutions to a fluid-particle coupled model with energy exchanges

In this paper, we investigate a three-dimensional fluid-particle coupled model. % in whole space $\mathbb{R}^3$. This model combines the full compressible Navier-Stokes equations with the Vlasov-Fokker-Planck equation via the momentum and energy exchanges. We obtain the global existence and optimal time decay rates of strong solutions to the model in whole space $\mathbb{R}^3$ when the initial data are a small perturbation of the given equilibrium in $H^2$. We show that the $L^2$-norms of the solutions and their gradients decay as $(1+t)^{-3/4}$ and $(1+t)^{-5/4}$ respectively. Moreover, we also obtain the decay rates of solutions in $L^p$-norms for $p\in [2,\infty]$, and the optimal time decay rates of the highest-order derivatives of strong solutions which reads as $(1+t)^{-{7}/{4}}$ in $L^2$-norm. % Our decay rates are consistent with those of non-isentropic compressible Navier-Stokes equations. When the model is considered in a periodic domain, besides the global existence results, we show the strong solution decay exponentially. Our proofs rely on the energy method, Fourier analysis techniques, and the method of frequency decomposition. And some new ideas are introduced to achieve the desired convergence rates.

math.AP↗

arXiv2024

Global well-posedness and decay rates of strong solutions to the incompressible Vlasov-MHD system

In this paper, we study the global well-posedness and decay rates of strong solutions to an incompressible Vlasov-MHD model arising in magnetized plasmas. This model is consist of the Vlasov equation and the incompressible magnetohydrodynamic equations which interacts together via the Lorentz forces. It is readily to verify that it has two equilibria $(\bar f,\bar u,\bar B)=(0,0,0)$ and $( \tilde f,\tilde u,\tilde B)=(M,0,0)$, where $M$ is the global maxwellian. For each equilibrium, assuming that the $H^2$ norm of the initial data $(f_0,B_0,U_0)$ is sufficient small and $f_0(x,v)$ has a compact support in the position $x$ and the velocity $v$, we construct the global well-posedness and decay rates of strong solutions near the equilibrium in the whole space $\mathbb{R}^3$. And the solution decays polynomially. The global existence result still holds for the torus $\mathbb{T}^3$ case without the compact support assumption in $x$. In addition, the decay rates are exponential. Lack of dissipation structure in the Vlasov equation and the strong trilinear coupling term $((u-v)\times B)f$ in the model are two main impediments in obtaining our results. To surround these difficulties, we assume that $f_0(x,v)$ has a compact support and utilize the method of characteristics to calculate the size of the supports of $f$. Thus, we overcome the difficulty in estimating the integration $\int_{\mathbb{R}^3} \big((u-v)\times B\big)f\mathrm{d}v$ and obtain the global existence of strong solutions by taking advantage of a refined energy method. Moreover, by making full use of the Fourier techniques, we obtain the optimal time decay rate of the gradient of the solutions. This is the first result on strong solutions to the Vlasov-MHD model containing nonlinear Lorentz forces.

math.AP↗