Abstract
Using recent developments in the theory of globally defined expanding compressible gases, we construct a class of global-in-time solutions to the compressible 3-D Euler–Poisson system without any symmetry assumptions in both the gravitational and the plasma case. Our allowed range of adiabatic indices includes, but is not limited to all γ of the form γ=1+1n, n∈ N\ { 1 }. The constructed solutions have initially small densities, a compact support, and they stay close to Sideris affine solutions of the Euler system. As t→ ∞ the density scatters to zero and the support grows at a linear rate in t.
Original language | English |
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Pages (from-to) | 475-505 |
Number of pages | 31 |
Journal | Communications in Mathematical Physics |
Volume | 370 |
Issue number | 2 |
Early online date | 26 Jul 2019 |
DOIs | |
Publication status | Published - 1 Sept 2019 |