Expanding Solutions to Free Boundary 3D Spherically Symmetric Compressible Navier-Stokes-Poisson Equations near the Lane-Emden Stars

Fuente: arXiv
Guardado en:
Detalles Bibliográficos
Autor principal: Cao, Han
Formato: Preprint
Publicado: 2025
Materias:
Acceso en línea:
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
_version_ 1866908670808293376
author Cao, Han
author_facet Cao, Han
contents We consider the gravitational Navier-Stokes-Poisson equations with the equation of state $P(ρ)=Kρ^γ$, where $γ\in(\frac{6}{5},\frac{4}{3}]$, which models the viscous polytropic gaseous stars. We prove the existence of global weak solutions to the equations with constant viscosity and radially symmetric initial data. For $γ=\frac{4}{3}$, we require the initial data having mass less than the mass of the Lane-Emden stars; for $γ\in(\frac{6}{5},\frac{4}{3})$, we require that the initial data belong to an invariant set where initial initial data can be taken near the Lane-Emden stars. For $γ\in(\frac{6}{5},\frac{4}{3})$, we show that the invariant set contains some initial data that are not allowed in previous literature. We also prove the support of any strong solution expands to infinity for the Navier-Stokes-Poisson equations with constant viscosity and a class of density-dependent viscosity, which indicates the strong instability of Lane-Emden solutions for the Navier-Stokes-Poisson equations.
format Preprint
id arxiv_https___arxiv_org_abs_2511_18339
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Expanding Solutions to Free Boundary 3D Spherically Symmetric Compressible Navier-Stokes-Poisson Equations near the Lane-Emden Stars
Cao, Han
Analysis of PDEs
We consider the gravitational Navier-Stokes-Poisson equations with the equation of state $P(ρ)=Kρ^γ$, where $γ\in(\frac{6}{5},\frac{4}{3}]$, which models the viscous polytropic gaseous stars. We prove the existence of global weak solutions to the equations with constant viscosity and radially symmetric initial data. For $γ=\frac{4}{3}$, we require the initial data having mass less than the mass of the Lane-Emden stars; for $γ\in(\frac{6}{5},\frac{4}{3})$, we require that the initial data belong to an invariant set where initial initial data can be taken near the Lane-Emden stars. For $γ\in(\frac{6}{5},\frac{4}{3})$, we show that the invariant set contains some initial data that are not allowed in previous literature. We also prove the support of any strong solution expands to infinity for the Navier-Stokes-Poisson equations with constant viscosity and a class of density-dependent viscosity, which indicates the strong instability of Lane-Emden solutions for the Navier-Stokes-Poisson equations.
title Expanding Solutions to Free Boundary 3D Spherically Symmetric Compressible Navier-Stokes-Poisson Equations near the Lane-Emden Stars
topic Analysis of PDEs
url https://arxiv.org/abs/2511.18339