The $N$-dimensional gravity driven Muskat problem

Fuente: arXiv
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Autori principali: Matioc, Bogdan-Vasile, Prokert, Georg
Natura: Preprint
Pubblicazione: 2026
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author Matioc, Bogdan-Vasile
Prokert, Georg
author_facet Matioc, Bogdan-Vasile
Prokert, Georg
contents We study the Muskat problem, which describes the motion of two immiscible, incompressible fluids in a homogeneous porous medium occupying the full space ${\mathbb{R}^{N+1}}$, $N \geq 2$, driven by gravity. The interface between the fluids is given as graph of a function over $\mathbb{R}^N$. The problem is reformulated as a nonlinear, nonlocal evolution problem for this function, involving singular integrals arising from potential representations of the velocity and pressure fields. Using results from harmonic analysis, we demonstrate that the evolution is of parabolic type in the open set identified by the Rayleigh-Taylor condition. We use the abstract theory of such problems to establish that the Muskat problem defines a semiflow on this set in all subcritical Sobolev spaces $H^s(\mathbb{R}^N)$, $s>s_c$, where ${s_c=1+N/2}$ is the critical exponent. We additionally obtain parabolic smoothing up to ${\rm C}^\infty$.
format Preprint
id arxiv_https___arxiv_org_abs_2602_09786
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle The $N$-dimensional gravity driven Muskat problem
Matioc, Bogdan-Vasile
Prokert, Georg
Analysis of PDEs
35R37, 35K55, 35Q35, 42B20
We study the Muskat problem, which describes the motion of two immiscible, incompressible fluids in a homogeneous porous medium occupying the full space ${\mathbb{R}^{N+1}}$, $N \geq 2$, driven by gravity. The interface between the fluids is given as graph of a function over $\mathbb{R}^N$. The problem is reformulated as a nonlinear, nonlocal evolution problem for this function, involving singular integrals arising from potential representations of the velocity and pressure fields. Using results from harmonic analysis, we demonstrate that the evolution is of parabolic type in the open set identified by the Rayleigh-Taylor condition. We use the abstract theory of such problems to establish that the Muskat problem defines a semiflow on this set in all subcritical Sobolev spaces $H^s(\mathbb{R}^N)$, $s>s_c$, where ${s_c=1+N/2}$ is the critical exponent. We additionally obtain parabolic smoothing up to ${\rm C}^\infty$.
title The $N$-dimensional gravity driven Muskat problem
topic Analysis of PDEs
35R37, 35K55, 35Q35, 42B20
url https://arxiv.org/abs/2602.09786