Analysis of PDEs (math.AP)

Abstract: We consider the steady Stokes equations in a bounded domain with forcing in divergence form supplemented with no-slip boundary conditions. We provide a maximal regularity theory in Campanato spaces (inlcuding $\mathrm{BMO}$ and $C^{0,\alpha}$ for $0<\alpha <1$ as special cases) under minimal assumptions on the regularity of the underlying domain. Our approach is based on pointwise multipliers in Campanto spaces.

Abstract: This work deals with the non-cutoff Boltzmann equation with hard potentials, in both the torus $\mathbf{T}^3$ and in the whole space $\mathbf{R}^3$, under the incompressible Navier-Stokes scaling. We first establish the well-posedness and decay of global mild solutions to this rescaled Boltzmann equation in a perturbative framework, that is for solutions close to the Maxwellian, obtaining in particular integrated-in-time regularization estimates. We then combine these estimates with spectral-type estimates in order to obtain the strong convergence of solutions to the non-cutoff Boltzmannn equation towards the incompressible Navier-Stokes-Fourier system.

Abstract: We study the continuity of solutions to complex Monge-Ampere equations with prescribed singularities. This generalizes the previous results of DiNezza-Lu and the author. As an application, we can run the Monge-Ampere flow starting at a current with prescribed singularities.

Abstract: The Pauli-Poisswell equation for 2-spinors is the first order in $1/c$ semi-relativistic approximation of the Dirac-Maxwell equation for 4-spinors coupled to the self-consistent electromagnetic fields generated by the density and current of a fast moving electric charge. It consists of a vector-valued magnetic Schr\"odinger equation with an extra term coupling spin and magnetic field via the Pauli matrices coupled to 1+3 Poisson type equations as the magnetostatic approximation of Maxwell's equations. The Pauli-Poisswell equation is a consistent $O(1/c)$ model that keeps both relativistic effects magnetism and spin which are both absent in the non-relativistic Schr\"odinger-Poisson equation and inconsistent in the magnetic Schr\"odinger-Maxwell equation. We present the mathematically rigorous semiclassical limit $\hbar \rightarrow 0$ of the Pauli-Poisswell equation towards the magnetic Euler-Poisswell equation. We use WKB analysis which is valid locally in time only. A key step is to obtain an a priori energy estimate for which we have to take into account the Poisson equations for the magnetic potential with the current as source term. Additionally we obtain the weak convergence of the monokinetic Wigner transform and strong convergence of the density and the current density. We also prove local wellposedness of the Euler-Poisswell equation which is global unless a finite time blow-up occurs.

Abstract: We consider solutions satisfying the zero Neumann boundary condition and a linearized mean field game equation in $\Omega \times (0,T)$ whose principal coefficients depend on the time and spatial variables with general Hamiltonian, where $\Omega$ is a bounded domain in $\Bbb R^d$ and $(0,T)$ is the time interval. We first prove the Lipschitz stability in $\Omega \times (\varepsilon, T-\varepsilon)$ with given $\varepsilon>0$ for the determination of the solutions by Dirichlet data on arbitrarily chosen subboundary of $\partial\Omega$. Next we prove the Lipschitz stability for an inverse problem of determining spatially varying factors of source terms and a coefficient by extra boundary data and spatial data at intermediate time.