On the global stability and large time behavior of solutions of the Boussinesq equations

Fuente: arXiv
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Autori principali: Jiang, Song, Wang, Quan
Natura: Preprint
Pubblicazione: 2025
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author Jiang, Song
Wang, Quan
author_facet Jiang, Song
Wang, Quan
contents We study the two dimensional viscous Boussinesq equations, which model stratified flows in a circular domain under the influence of a general gravitational potential $f$. First, we show that the Boussinesq equations admit steady-state solutions only in the form of hydrostatic equilibria, $(\mathbf{u},ρ,p) = (0, ρ_s, p_s)$, where the pressure gradient satisfies $\nabla p_s = -ρ_s \nabla f$. Moreover, the relation between $ρ_s$ and $f$ is constrained by $(\partial_y ρ_s, -\partial_x ρ_s) \cdot (\partial_x f, \partial_y f) = 0$, which allows us to write $\nabla ρ_s = h(x,y) \nabla f$ for some scalar function $h(x,y)$. Second, we prove that any hydrostatic equilibrium $(0, ρ_s, p_s)$ is linearly unstable if $h(x_0, y_0) > 0$ at some point $(x, y) = (x_0, y_0)$. This instability coincides with the classical Rayleigh--Taylor instability. Third, by employing a series of regularity estimates, we reveal that although the presence of the Rayleigh--Taylor instability makes perturbations around the unstable equilibrium grow exponentially in time, the system ultimately converges to a state of hydrostatic equilibrium. The analysis is carried out for perturbations about an arbitrary hydrostatic equilibrium, covering both stable and unstable configurations. Finally, we derive a necessary and sufficient condition on the initial density perturbation under which the density converges to a profile of the form $-γf + β$ with constants $γ, β> 0$. This result underscores the system's inherent tendency to settle into a hydrostatic state, even in the presence of Rayleigh--Taylor instability.
format Preprint
id arxiv_https___arxiv_org_abs_2502_16226
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle On the global stability and large time behavior of solutions of the Boussinesq equations
Jiang, Song
Wang, Quan
Analysis of PDEs
We study the two dimensional viscous Boussinesq equations, which model stratified flows in a circular domain under the influence of a general gravitational potential $f$. First, we show that the Boussinesq equations admit steady-state solutions only in the form of hydrostatic equilibria, $(\mathbf{u},ρ,p) = (0, ρ_s, p_s)$, where the pressure gradient satisfies $\nabla p_s = -ρ_s \nabla f$. Moreover, the relation between $ρ_s$ and $f$ is constrained by $(\partial_y ρ_s, -\partial_x ρ_s) \cdot (\partial_x f, \partial_y f) = 0$, which allows us to write $\nabla ρ_s = h(x,y) \nabla f$ for some scalar function $h(x,y)$. Second, we prove that any hydrostatic equilibrium $(0, ρ_s, p_s)$ is linearly unstable if $h(x_0, y_0) > 0$ at some point $(x, y) = (x_0, y_0)$. This instability coincides with the classical Rayleigh--Taylor instability. Third, by employing a series of regularity estimates, we reveal that although the presence of the Rayleigh--Taylor instability makes perturbations around the unstable equilibrium grow exponentially in time, the system ultimately converges to a state of hydrostatic equilibrium. The analysis is carried out for perturbations about an arbitrary hydrostatic equilibrium, covering both stable and unstable configurations. Finally, we derive a necessary and sufficient condition on the initial density perturbation under which the density converges to a profile of the form $-γf + β$ with constants $γ, β> 0$. This result underscores the system's inherent tendency to settle into a hydrostatic state, even in the presence of Rayleigh--Taylor instability.
title On the global stability and large time behavior of solutions of the Boussinesq equations
topic Analysis of PDEs
url https://arxiv.org/abs/2502.16226