Nonlinear asymptotic stability of gravitational hydrostatic equilibrium for viscous white dwarfs with symmetric perturbations
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Publication:6619968
DOI10.1007/s00526-024-02831-4MaRDI QIDQ6619968
Yan-Lin Wang, Tao Luo, Huihui Zeng
Publication date: 16 October 2024
Published in: Calculus of Variations and Partial Differential Equations (Search for Journal in Brave)
Smoothness and regularity of solutions to PDEs (35B65) Asymptotic behavior of solutions to PDEs (35B40) PDEs in connection with fluid mechanics (35Q35) Stability in context of PDEs (35B35) Perturbations in context of PDEs (35B20) Free boundary problems for PDEs (35R35) Galactic and stellar dynamics (85A05) Existence, uniqueness, and regularity theory for compressible fluids and gas dynamics (76N10) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20) PDEs in connection with astronomy and astrophysics (35Q85)
Cites Work
- Unnamed Item
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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
- 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
- The density of white dwarf stars.
- Singular behavior of vacuum states for compressible fluids
- Nonlinear instability in gravitational Euler-Poisson systems for \(\gamma=\frac{6}{5}\)
- Local well-posedness of dynamics of viscous gaseous stars
- Nonlinear dynamical stability of Newtonian rotating and non-rotating white dwarfs and rotating supermassive stars
- Global behavior of spherically symmetric Navier-Stokes-Poisson system with degenerate viscosity coefficients
- 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
- The shape of axisymmetric rotating fluid
- Minimization problems in \(L^1(\mathbb{R}^3)\)
- Existence and dimensions of a rotating white dwarf
- On uniformly rotating stars
- On diameters of uniformly rotating stars
- Nonlinear stability of gaseous stars
- Compressible flow with vacuum and physical singularity.
- Global solutions to physical vacuum problem of non-isentropic viscous gaseous stars and nonlinear asymptotic stability of stationary solutions
- Solutions of Euler-Poisson equations for gaseous stars
- Compressible flow with damping and vacuum
- Well-posedness in smooth function spaces for the moving-boundary three-dimensional compressible Euler equations in physical vacuum
- Local well-posedness to the vacuum free boundary problem of full compressible Navier-Stokes equations in \(\mathbb{R}^3\)
- Larson-Penston self-similar gravitational collapse
- Continued gravitational collapse for Newtonian stars
- Almost global solutions to the three-dimensional isentropic inviscid flows with damping in a physical vacuum around Barenblatt solutions
- Local well-posedness of the vacuum free boundary of 3-D compressible Navier-Stokes equations
- A class of global solutions to the Euler-Poisson system
- Global resolution of the physical vacuum singularity for three-dimensional isentropic inviscid flows with damping in spherically symmetric motions
- Global behavior of compressible Navier-Stokes equations with a degenerate viscosity coefficient
- Variational solutions of some nonlinear free boundary problems
- On nonlinear asymptotic stability of the Lane-Emden solutions for the viscous gaseous star problem
- Global Existence of Smooth Solutions and Convergence to Barenblatt Solutions for the Physical Vacuum Free Boundary Problem of Compressible Euler Equations with Damping
- Nonlinear Instability Theory of Lane-Emden Stars
- Well-posedness of Compressible Euler Equations in a Physical Vacuum
- Well-posedness in smooth function spaces for moving-boundary 1-D compressible euler equations in physical vacuum
- Well-posedness for compressible Euler equations with physical vacuum singularity
- Stability of Gaseous Stars in Spherically Symmetric Motions
- The Highly Collapsed Configurations of a Stellar Mass
- The Maximum Mass of Ideal White Dwarfs
- Local Existence and Uniqueness of Strong Solutions to the Free Boundary Problem of the Full Compressible Navier--Stokes Equations in three dimensions
- 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
- Separable Hamiltonian PDEs and Turning Point Principle for Stability of Gaseous Stars
- Global finite-energy solutions of the compressible Euler-Poisson equations for general pressure laws with large initial data of spherical symmetry
- Global Solutions of the Compressible Euler-Poisson Equations with Large Initial Data of Spherical Symmetry
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