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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 of the form , . The constructed solutions have initially small densities and a compact support. As the density scatters to zero and the support grows at a linear rate in .

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