Forward self-similar solutions to the MHD equations: existence and pointwise estimates
Yifan Yang
TL;DR
The paper addresses forward self-similar solutions to the 3D incompressible MHD equations in $\mathbb{R}^3$ with initial data homogeneous of degree $-1$. It reduces the self-similar problem to a time-independent perturbed Leray system for profile fields and employs a blow-up argument together with the Leray–Schauder fixed-point theorem on invading domains to construct a global weak solution $(V,G)$, with pressure $P$ obtained from De Rham theory. Through energy methods and kernel-based perturbation analysis using the Oseen/heat kernels, it derives decay and pointwise estimates for the perturbation $(V,G)$ and for the velocity/magnetic fields $(u,b)$, including optimal rates under higher regularity of the initial data. The results yield a smooth, forward self-similar solution $(u,b)$ that converges to the heat-flow initial data in a weak sense and provides explicit decay profiles, contributing a rigorous large-data framework for self-similar MHD behavior. Uniqueness remains open, but the methodology enables potential extensions to half-space problems and related fluid–magnetic systems, with the kernel-based approach offering sharp pointwise controls.
Abstract
In this paper, we study the forward self-similar solutions to the three-dimensional Magnetohydrodynamic equations (MHD equations) in the whole space. By employing the Leray-Schauder theorem and blow-up argument, we construct a global-time forward self-similar solutions, which is smooth in $\R^{3}\times(0,\infty)$. Furthermore, by investigating the regularity of the weak solutions to the corresponding Leray system in the weighted Sobolev space, we can derive the pointwise estimate for the forward self-similar solution.
