Asymptotic stability of the equilibrium for the free boundary problem of a compressible atmospheric primitive model with physical vacuum

TL;DR

This paper proves the exponential convergence to equilibrium of solutions to a free boundary problem in compressible atmospheric models with physical vacuum, using a novel coordinate system and derivative estimates.

Contribution

It introduces a new coordinate system based on enthalpy and establishes stability results for the physical vacuum free boundary problem in atmospheric dynamics.

Findings

Global-in-time solutions converge exponentially to equilibrium.

The new coordinate system simplifies derivative estimates.

The model accounts for physical vacuum conditions at the boundary.

Abstract

This paper concerns the large time asymptotic behavior of solutions to the free boundary problem of the compressible primitive equations in atmospheric dynamics with physical vacuum. Up to second order of the perturbations of an equilibrium, we have introduced a model of the compressible primitive equations with a specific viscosity and shown that the physical vacuum free boundary problem for this model system has a global-in-time solution converging to an equilibrium exponentially, provided that the initial data is a small perturbation of the equilibrium. More precisely, we introduce a new coordinate system by choosing the enthalpy (the square of sound speed) as the vertical coordinate, and thanks to the hydrostatic balance, the degenerate density at the free boundary admits a representation with separation of variables in the new coordinates. Such a property allows us to establish horizontal derivative estimates without involving the singular vertical derivative of the density profile, which plays a key role in our analysis.