Space-time decay rates of a two-phase flow model with magnetic field in R^3

Authors

  • Qin Ye Guangxi Normal Univ., Guilin, Guangxi, China
  • Yinghui Zhang Guangxi Normal Univ., Guilin, Guangxi, China

DOI:

https://doi.org/10.58997/ejde.2023.41

Keywords:

Compressible Euler equations; Two-phase flow model; Space-time decay rate; Weighted Sobolev space.

Abstract

We investigate the space-time decay rates of strong solution to a two-phase flow model with magnetic field in the whole space \(\mathbb{R}^3 \). Based on the temporal decay results by Xiao [24] we show that for any integer \(\ell\geq 3\), the space-time decay rate of \(k(0\leq k \leq \ell)\)-order spatial derivative of the strong solution in the weighted Lebesgue space \( L_\gamma^2 \) is \(t^{-\frac{3}{4}-\frac{k}{2}+\gamma}\). Moreover, we prove that the space-time decay rate of \(k(0\leq k \leq \ell-2)\)-order spatial derivative of the difference between two velocities of the fluid in the weighted Lebesgue space \( L_\gamma^2 \) is \(t^{-\frac{5}{4}-\frac{k}{2}+\gamma}\), which is faster than ones of the two velocities themselves.

For more information see https://ejde.math.txstate.edu/Volumes/2023/41/abstr.html

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2023-06-23

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Space-time decay rates of a two-phase flow model with magnetic field in R^3. (2023). Electronic Journal of Differential Equations, 2023(01-87), No. 41, 21-29. https://doi.org/10.58997/ejde.2023.41