Global solutions of the compressible Euler‐Poisson equations with large initial data of spherical symmetry
We are concerned with a global existence theory for finite‐energy solutions of the multidimensional Euler‐Poisson equations for both compressible gaseous stars and plasmas with large initial data of spherical symmetry. One of the main challenges is the strengthening of waves as they move radially in...
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Veröffentlicht in: | Communications on pure and applied mathematics 2024-06, Vol.77 (6), p.2947-3025 |
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