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Formation of singularities of spherically symmetric solutions to the 3D compressible Euler equations and Euler–Poisson equations

机译:三维可压缩欧拉方程与欧拉 - 泊松方程的球体对称解的奇异性

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摘要

By introducing a new averaged quantity with a fast decay weight to perform Sideris’s argument?(Commun Math Phys 101:475–485, 1985) developed for the Euler equations, we extend the formation of singularities of classical solution to the 3D Euler equations established in Makino et al. (Jpn J Appl Math 3:249–257, 1986) and Sideris (1985) for the initial data with compactly supported disturbances to the spherically symmetric solution with general initial data in Sobolev space. Moreover, we also prove the formation of singularities of the spherically symmetric solutions to the 3D Euler–Poisson equations, but remove the compact support assumptions on the initial data in Makino and Perthame (Jpn J Appl Math 7:165–170, 1990) and Perthame (Jpn J Appl Math 7:363–367, 1990). Our proof also simplifies that of Lei et al. (Math Res Lett 20:41–50, 2013) for the Euler equations and is undifferentiated in dimensions.
机译:通过以快速衰减重量引入新的平均数量来执行Sideris的论点?(为欧拉方程开发的Math Malt 101:475-485,1985),我们将经典解决方案的奇异性的形成扩展到建立的3D欧拉方程 makino等。 (JPN JP Appl Math 3:249-257,1986)和Sideris(1985)用于初始数据,具有紧凑支持的扰动,与SoboLev空间中的一般初始数据进行球体对称的解决方案。 此外,我们还证明了3D Euler-Poisson方程的球形对称解的奇点形成,但是除去了Makino和Hotthame中的初始数据上的紧凑载体假设(JPN J Appl Math 7:165-170,1990)和 截然不同(JPN J Appl Math 7:363-367,1990)。 我们的证据还简化了雷等人的证据。 (Math Res Lett 20:41-50,2013)用于欧拉方程,并在尺寸中无差别化。

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