Variational rotating solutions to non-isentropic Euler-Poisson equations with prescribed total mass
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Publication:2082280
DOI10.1007/s11425-021-1859-8zbMath1498.35545arXiv1710.02915OpenAlexW3199602516MaRDI QIDQ2082280
Publication date: 4 October 2022
Published in: Science China. Mathematics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1710.02915
PDEs in connection with fluid mechanics (35Q35) Variational methods applied to PDEs (35A15) General theory of rotating fluids (76U05) Liquid crystals (76A15) Geodesy, mapping problems (86A30) PDEs in connection with astronomy and astrophysics (35Q85)
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Cites Work
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- Local well-posedness of the three dimensional compressible Euler-Poisson equations with physical vacuum
- Nonlinear asymptotic stability of the Lane-Emden solutions for the viscous gaseous star problem with degenerate density dependent viscosities
- An application of the Nash-Moser theorem to the vacuum boundary problem of gaseous stars
- Instability theory of the Navier-Stokes-Poisson equations
- Well-posedness for the motion of physical vacuum of the three-dimensional compressible Euler equations with or without self-gravitation
- A remark on the geometry of uniformly rotating stars
- On rotating star solutions to the non-isentropic Euler-Poisson equations
- The global branching of rotating stars
- Multiplicity of stationary solutions to the Euler--Poisson equations
- Nonlinear instability in gravitational Euler-Poisson systems for \(\gamma=\frac{6}{5}\)
- Nonlinear dynamical stability of Newtonian rotating and non-rotating white dwarfs and rotating supermassive stars
- Existence and nonlinear stability of rotating star solutions of the compressible Euler-Poisson equations
- The Chandrasekhar theory of stellar collapse as the limit quantum mechanics
- Asymptotic estimates for an axisymmetric rotating fluid
- The shape of axisymmetric rotating fluid
- Existence and dimensions of a rotating white dwarf
- On uniformly rotating stars
- On diameters of uniformly rotating stars
- Nonlinear stability of gaseous stars
- On rotating axisymmetric solutions of the Euler-Poisson equations
- Rotating fluids with self-gravitation in bounded domains
- Solutions of Euler-Poisson equations for gaseous stars
- On slowly rotating axisymmetric solutions of the Euler-Poisson equations
- Existence of magnetic compressible fluid stars
- On the expanding configurations of viscous radiation gaseous stars: thermodynamic model
- On spherically symmetric motions of a gaseous star governed by the Euler-Poisson equations
- Rapidly rotating stars
- Variational solutions of some nonlinear free boundary problems
- On nonlinear asymptotic stability of the Lane-Emden solutions for the viscous gaseous star problem
- Reduction and a Concentration-Compactness Principle for Energy-Casimir Functionals
- Nonlinear Instability Theory of Lane-Emden Stars
- Stability of Gaseous Stars in Spherically Symmetric Motions
- A Model of Radiational Gaseous Stars
- Steady States of Rotating Stars and Galaxies
- Nonlinear Stability of Expanding Star Solutions of the Radially Symmetric Mass‐Critical Euler‐Poisson System
- On the expanding configurations of viscous radiation gaseous stars: the isentropic model
- Existence of rotating planet solutions to the Euler-Poisson equations with an inner hard core
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