Waiting Time Solutions in gas dynamics
Juhi Jang, Jiaqi Liu, Nader Masmoudi
TL;DR
The paper addresses waiting-time phenomena for the 1D compressible Euler equations with a vacuum boundary under the physical vacuum condition, for $\gamma\in(1,3)$. It develops a self-similar reduction using a two-parameter scaling and analyzes an associated ODE system in the $(U,H)$ plane, including a key special solution $H^{\text{sp}}(U)$. It proves the existence of a two-parameter continuum of self-similar waiting-time solutions, parameterized by $\mu\in(0,1)$ and $\gamma\in(1,3)$, featuring a stationary left vacuum boundary for $t<0$ that transitions to a moving boundary with a physical vacuum for $t>0$, after a finite waiting time. The construction relies on a detailed phase-portrait analysis and barrier arguments to connect critical points $C\to A\to E\to D\to B$, yielding Hölder regularity near the singular point and a Lipschitz discontinuity along the emergent sonic curve.
Abstract
In this article, we construct a continuum family of self-similar waiting time solutions for the one-dimensional compressible Euler equations for the adiabatic exponent $\ga\in(1,3)$ in the half-line with the vacuum boundary. The solutions are confined by a stationary vacuum interface for a finite time with at least $C^1$ regularity of the velocity and the sound speed up to the boundary. Subsequently, the solutions undergo the change of the behavior, becoming only Hölder continuous near the singular point, and simultaneously transition to the solutions to the vacuum moving boundary Euler equations satisfying the physical vacuum condition. When the boundary starts moving, a weak discontinuity emanating from the singular point along the sonic curve emerges. The solutions are locally smooth in the interior region away from the vacuum boundary and the sonic curve.
