The Newtonian limit for perfect fluids
From MaRDI portal
Publication:2466825
DOI10.1007/s00220-007-0334-zzbMath1194.83018arXiv0810.3744OpenAlexW3098529974MaRDI QIDQ2466825
Publication date: 16 January 2008
Published in: Communications in Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0810.3744
PDEs in connection with fluid mechanics (35Q35) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) PDEs in connection with relativity and gravitational theory (35Q75) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)
Related Items (20)
Dynamical compact elastic bodies in general relativity ⋮ Cosmological Newtonian limits on large spacetime scales ⋮ A note on incompressibility of relativistic fluids and the instantaneity of their pressures ⋮ Post-Newtonian expansions for perfect fluids ⋮ On slowly rotating axisymmetric solutions of the Einstein-Euler equations ⋮ Future stability of the FLRW spacetime for a large class of perfect fluids ⋮ Local existence of solutions to the Euler-Poisson system, including densities without compact support ⋮ Local existence of solutions of self gravitating relativistic perfect fluids ⋮ Blowups and Longtime Developments with Near-Boundary Mass Accretions of Irregularly Shaped Euler–Poisson Dominated Molecular Clouds in Astrophysics ⋮ On the well-posedness of the vacuum Einstein's equations ⋮ Mathematical general relativity ⋮ Local existence of solutions to the Euler-Poisson system, including densities without compact support ⋮ Cosmological post-Newtonian expansions to arbitrary order ⋮ Newtonian limits of isolated cosmological systems on long time scales ⋮ A RIGOROUS FORMULATION OF THE COSMOLOGICAL NEWTONIAN LIMIT WITHOUT AVERAGING ⋮ The Newtonian limit on cosmological scales ⋮ A post-Newtonian expansion including radiation damping for a collisionless plasma ⋮ THE NON-RELATIVISTIC LIMIT OF THE EULER–NORDSTRÖM SYSTEM WITH COSMOLOGICAL CONSTANT ⋮ Newtonian limit for the relativistic Euler-Poisson equations with vacuum ⋮ Existence of families of spacetimes with a Newtonian limit
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- An existence proof for the gravitating BPS monopole
- Post-Newtonian expansions for perfect fluids
- Local existence of classical solutions for the Einstein-Euler system using weighted Sobolev spaces of fractional order
- Elliptic systems in H(s,delta) spaces on manifolds which are Euclidean at infinity
- The Newtonian limit of the spherically symmetric Vlasov-Einstein system
- Covariant Newtonian limit of Lorentz space-times
- The Newtonian limit for asymptotically flat solutions of the Vlasov- Einstein system
- On the existence of rotating stars in general relativity
- On the Newtonian limit of general relativity
- Asymptotics for symmetric hyperbolic systems with a large parameter
- Partial differential equations. 3: Nonlinear equations
- Rotationally symmetric Ricci flow on asymptotically flat manifolds
- The gravitational equations and the problem of motion
- The Einstein–Vlasov–Maxwell (EVM) system with spherical symmetry
- Rough solutions of the Einstein constraint equations
- Convergent and divergent perturbation series and the post-Minkowskian approximation scheme
- The mass of an asymptotically flat manifold
- Relativistic and non-relativistic classical field theory on five-dimensional spacetime
- Radiative gravitational fields in general relativity I. General structure of the field outside the source
- Symmetric hyperbolic systems with a large parameter
- The initial value problem for a class of general relativistic fluid bodies
- On the definition of post-newtonian approximations
- A note on the relativistic Euler equations
- Fast and slow solutions in General Relativity: The initialization procedure
- Problems with Different Time Scales for Nonlinear Partial Differential Equations
- On mapping properties of the general relativistic constraints operator in weighted function spaces, with applications
- Post-Newtonian Equations of Hydrodynamics and the Stability of Gaseous Masses in General Relativity
- Newtonian perturbations and the Einstein–Yang–Mills-dilaton equations
This page was built for publication: The Newtonian limit for perfect fluids