A Model of Radiational Gaseous Stars
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Publication:4560157
DOI10.1137/17M1133476zbMath1423.76392arXiv1612.07936MaRDI QIDQ4560157
Publication date: 5 December 2018
Published in: SIAM Journal on Mathematical Analysis (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1612.07936
PDEs in connection with fluid mechanics (35Q35) Gas dynamics (general theory) (76N15) Free boundary problems for PDEs (35R35) Celestial mechanics (70F15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Related Items (7)
Immediate Blowup of Entropy-Bounded Classical Solutions to the Vacuum Free Boundary Problem of Nonisentropic Compressible Navier–Stokes Equations ⋮ Local Existence and Uniqueness of Strong Solutions to the Free Boundary Problem of the Full Compressible Navier--Stokes Equations in three dimensions ⋮ Local well-posedness to the vacuum free boundary problem of full compressible Navier-Stokes equations in \(\mathbb{R}^3\) ⋮ On the expanding configurations of viscous radiation gaseous stars: thermodynamic model ⋮ The self-similar solutions to full compressible Navier–Stokes equations without heat conductivity ⋮ On the expanding configurations of viscous radiation gaseous stars: the isentropic model ⋮ Variational rotating solutions to non-isentropic Euler-Poisson equations with prescribed total mass
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