Structural stability of non-isentropic Euler-Poisson system for gaseous stars
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Publication:6667455
DOI10.1016/J.JDE.2024.11.010MaRDI QIDQ6667455
Chun-peng Wang, Ben Duan, Zhen Luo
Publication date: 20 January 2025
Published in: Journal of Differential Equations (Search for Journal in Brave)
PDEs of mixed type (35M10) Existence, uniqueness, and regularity theory for compressible fluids and gas dynamics (76N10) Nonlinear boundary value problems for nonlinear elliptic equations (35J66) PDEs in connection with astronomy and astrophysics (35Q85)
Cites Work
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- Nonlinear asymptotic stability of the Lane-Emden solutions for the viscous gaseous star problem with degenerate density dependent viscosities
- Well-posedness for the motion of physical vacuum of the three-dimensional compressible Euler equations with or without self-gravitation
- On rotating star solutions to the non-isentropic Euler-Poisson equations
- Euler-Poisson equations related to general compressible rotating fluids
- 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 shape of axisymmetric rotating fluid
- Minimization problems in \(L^1(\mathbb{R}^3)\)
- On uniformly rotating stars
- Stable steady states in stellar dynamics
- Nonlinear stability of gaseous stars
- Elliptic partial differential equations of second order
- 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
- Larson-Penston self-similar gravitational collapse
- Gravitational collapse for polytropic gaseous stars: self-similar solutions
- Continued gravitational collapse for Newtonian stars
- A class of global solutions to the Euler-Poisson system
- Rapidly rotating stars
- Some results on Newtonian gaseous stars -- existence and stability
- Variational solutions of some nonlinear free boundary problems
- Elliptic partial differential equations
- On The Euler-Poisson Equations of Self-Gravitating Compressible Fluids
- Linearized analysis of barotropic perturbations around spherically symmetric gaseous stars governed by the Euler–Poisson equations
- Global smooth solutions to Euler equations for a perfect gas
- Blowing up solutions of the euler-poisson equation for the evolution of gaseous stars
- Stability of Gaseous Stars in Spherically Symmetric Motions
- Steady States of Rotating Stars and Galaxies
- Nonlinear Stability of Expanding Star Solutions of the Radially Symmetric Mass‐Critical Euler‐Poisson System
- Continued Gravitational Collapse for Gaseous Star and Pressureless Euler--Poisson System
- Ellipsoidal figures of equilibrium—an historical account
- Existence of rotating planet solutions to the Euler-Poisson equations with an inner hard core
- Stability of rotating gaseous stars
- Existence of Rotating Stars with Variable Entropy
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