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Main Authors: Li, Jinlu, Yu, Yanghai, Zhu, Neng
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2503.05069
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author Li, Jinlu
Yu, Yanghai
Zhu, Neng
author_facet Li, Jinlu
Yu, Yanghai
Zhu, Neng
contents In this paper, we consider the Cauchy problem for the 3D Euler equations with the Coriolis force in the whole space. We first establish the local-in-time existence and uniqueness of solution to this system in $B^s_{p,r}(\R^3)$. Then we prove that the Cauchy problem is ill-posed in two different sense: (1) the solution of this system is not uniformly continuous dependence on the initial data in the same Besov spaces, which extends the recent work of Himonas-Misiołek \cite[Comm. Math. Phys., 296, 2010]{HM1} to the more general framework of Besov spaces; (2) the solution of this system cannot be Hölder continuous in time variable in the same Besov spaces. In particular, the solution of the system is discontinuous in the weaker Besov spaces at time zero. To the best of our knowledge, our work is the first one addressing the issue on the failure of Hölder continuous in time of solution to the classical Euler equations with(out) the Coriolis force.
format Preprint
id arxiv_https___arxiv_org_abs_2503_05069
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle On the continuous properties for the 3D incompressible rotating Euler equations
Li, Jinlu
Yu, Yanghai
Zhu, Neng
Analysis of PDEs
In this paper, we consider the Cauchy problem for the 3D Euler equations with the Coriolis force in the whole space. We first establish the local-in-time existence and uniqueness of solution to this system in $B^s_{p,r}(\R^3)$. Then we prove that the Cauchy problem is ill-posed in two different sense: (1) the solution of this system is not uniformly continuous dependence on the initial data in the same Besov spaces, which extends the recent work of Himonas-Misiołek \cite[Comm. Math. Phys., 296, 2010]{HM1} to the more general framework of Besov spaces; (2) the solution of this system cannot be Hölder continuous in time variable in the same Besov spaces. In particular, the solution of the system is discontinuous in the weaker Besov spaces at time zero. To the best of our knowledge, our work is the first one addressing the issue on the failure of Hölder continuous in time of solution to the classical Euler equations with(out) the Coriolis force.
title On the continuous properties for the 3D incompressible rotating Euler equations
topic Analysis of PDEs
url https://arxiv.org/abs/2503.05069