Some Exact Blowup Solutions to the Pressureless Euler Equations in R^N
arXiv:0910.1272 · doi:10.1016/j.cnsns.2010.10.021
Abstract
The pressureless Euler equations can be used as simple models of cosmology or plasma physics. In this paper, we construct the exact solutions in non-radial symmetry to the pressureless Euler equations in % [c]{c}% ρ(t,\vec{x})=\frac{f(\frac{1}{a(t)^{s}}\underset{i=1}{\overset {N}{\sum}}x_{i}^{s})}{a(t)^{N}}\text{,}\vec{u}(t,\vec{x}% )=\frac{\overset{\cdot}{a}(t)}{a(t)}\vec{x}, a(t)=a_{1}+a_{2}t. \label{eq234}% where the arbitrary function and , and are constants\newline In particular, for , the solutions blow up on the finite time . Moreover, the functions (\ref{eq234}) are also the solutions to the pressureless Navier-Stokes equations.
7 pages Key Words: Pressureless Gas, Euler Equations, Exact Solutions, Non-Radial Symmetry, Navier-Stokes Equations, Blowup, Free Boundary
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Cited by in corpus (6)
- Self-Similar Solutions with Elliptic Symmetry for the Compressible Euler and Navier-Stokes Equations in R^{N}
- Blowup for the Euler and Euler-Poisson Equations with Repulsive Forces
- Exact, Rotational, Infinite Energy, Blowup Solutions to the 3-Dimensional Euler Equations
- Self-Similar Blowup Solutions to the 2-Component Degasperis-Procesi Shallow Water System
- Perturbational Blowup Solutions to the 2-Component Camassa-Holm Equations
- The Inviscid, Compressible and Rotational, 2D Isotropic Burgers and Pressureless Euler-Coriolis Fluids; Solvable models with illustrations