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arXiv 2103.03474math.AP

具有非零涡量的三维可压缩 Euler 方程的延迟奇性形成

Delayed singularity formation for the three dimensional compressible Euler equations with non-zero vorticity

Fei Hou, Huicheng Yin

AI总结:

本文研究三维可压缩等熵 Euler 方程中非零初始涡量对光滑解寿命的影响,通过加权能量与衰减估计证明涡量大小可显著延迟奇性形成。

摘要:

对于静止状态存在大小为 $\ve$ 的初始扰动的三维可压缩等熵 Euler 方程,如果初始涡量大小为 $\dl$,其中 $0<\dl\le \ve$,且 $\ve$ 很小,我们证明:对于多方气体,光滑解的寿命为 $T_{\dl}=O(\min\{e^\frac{1}{\ve},\frac{1}{δ}\})$;而对于 Chaplygin 气体,寿命为 $T_{\dl}=O(\frac{1}{δ})$。例如,当选取 $\dl=e^{-\f{1}{\ve^2}}$ 时,尽管初始密度扰动和初始速度散度仅为 $O(\ve)$ 阶,但多方气体的 $T_{\dl}=O(e^{\f{1}{\ve}})$,Chaplygin 气体的 $T_{\dl}=O(e^{\f{1}{\ve^2}})$。我们的结果表明,只要初始数据充分接近常数,光滑解的存在时间就关键地取决于初始数据涡量的大小。本文的主要技术要素包括:引入若干适当加权的能量,推导解的逐点时空衰减估计,寻找替代速度的良好未知量,以及建立关于涡量所需的加权估计。

英文摘要:

For the 3D compressible isentropic Euler equations with an initial perturbation of size $\ve$ of a rest state, if the initial vorticity is of size $\dl$ with $0<\dl\le \ve$ and $\ve$ is small, we establish that the lifespan of the smooth solutions is $T_{\dl}=O(\min\{e^\frac{1}{\ve},\frac{1}δ\})$ for the polytropic gases, and $T_{\dl}=O(\frac{1}δ)$ for the Chaplygin gases. For example, when $\dl=e^{-\f{1}{\ve^2}}$ is chosen, then $T_{\dl}=O(e^{\f{1}{\ve}})$ for the polytropic gases and $T_{\dl}=O(e^{\f{1}{\ve^2}})$ for the Chaplygin gases although the perturbations of the initial density and the divergence of the initial velocity are only of order $O(\ve)$. Our result illustrates that the time of existence of smooth solutions depends crucially on the size of the vorticity of the initial data, as long as the initial data is sufficiently close to a constant. The main ingredients in the paper are: introducing some suitably weighted energies, deriving the pointwise space-time decay estimates of solutions, looking for the good unknown instead of the velocity, and establishing the required weighted estimates on the vorticty.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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