Non-relativistic limit analysis of the Chandrasekhar–Thorne relativistic Euler equations with physical vacuum
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Publication:5237783
DOI10.1142/S0218202519500155zbMath1428.35331arXiv1808.05856MaRDI QIDQ5237783
Pierangelo Marcati, La-Su Mai, Hai-liang Li
Publication date: 18 October 2019
Published in: Mathematical Models and Methods in Applied Sciences (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1808.05856
Smoothness and regularity of solutions to PDEs (35B65) Stability in context of PDEs (35B35) Gas dynamics (general theory) (76N15) Free boundary problems for PDEs (35R35) Euler equations (35Q31)
Related Items (8)
Free boundary value problem for damped Euler equations and related models with vacuum ⋮ \(L^1\) convergences and convergence rates of approximate solutions for compressible Euler equations near vacuum ⋮ Immediate Blowup of Entropy-Bounded Classical Solutions to the Vacuum Free Boundary Problem of Nonisentropic Compressible Navier–Stokes Equations ⋮ Quasi-Neutral Limit to Steady-State Hydrodynamic Model of Semiconductors with Degenerate Boundary ⋮ Well and ill-posedness of free boundary problems to relativistic Euler equations ⋮ Approximation and Existence of Vacuum States in the Multiscale Flows of Compressible Euler Equations ⋮ Newtonian limit for the relativistic Euler-Poisson equations with vacuum ⋮ Nonrelativistic limits for the 1D relativistic Euler equations with physical vacuum
Cites Work
- Well-posedness for the motion of physical vacuum of the three-dimensional compressible Euler equations with or without self-gravitation
- Special relativistic effects revealed in the Riemann problem for three-dimensional relativistic Euler equations
- Well-posedness of 1-D compressible Euler-Poisson equations with physical vacuum
- Blowup of smooth solutions for relativistic Euler equations
- Non-relativistic global limits of entropy solutions to the isentropic relativistic Euler equations
- Lagrangian formulation and a priori estimates for relativistic fluid flows with vacuum
- Non-relativistic global limits of entropy solutions to the extremely relativistic Euler equations
- A priori estimates for the free-boundary 3D compressible Euler equations in physical vacuum
- \(L^{1}\) stability of spatially periodic solutions in relativistic gas dynamics
- Non-relativistic global limits of weak solutions of the relativistic Euler equation
- Global solutions of the relativistic Euler equations
- Conservation laws for relativistic fluid dynamics
- On the relativistic Euler equation
- Relativistic Euler equations for isentropic fluids: stability of Riemann solutions with large oscillation
- Global entropy solutions to the relativistic Euler equations for a class of large initial data
- On spherically symmetric solutions of the relativistic Euler equation
- Local smooth solutions of the relativistic Euler equation
- Local smooth solutions of the relativistic Euler equation. II
- Well-posedness in smooth function spaces for the moving-boundary three-dimensional compressible Euler equations in physical vacuum
- 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
- Local existence for the free boundary problem for nonrelativistic and Relativistic compressible Euler equations with a vacuum boundary condition
- Approximate Solutions of the Einstein Equations for Isentropic Motions of Plane-Symmetric Distributions of Perfect Fluids
- Well-posedness for compressible Euler equations with physical vacuum singularity
- Global entropy solutions for isentropic relativistic fluid dynamics
- Conservation laws for the relativistic P-system
- A priori estimates for solutions to the relativistic Euler equations with a moving vacuum boundary
- Post-Newtonian Equations of Hydrodynamics and the Stability of Gaseous Masses in General Relativity
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