55 research outputs found
The Newtonian limit for perfect fluids
We prove that there exists a class of non-stationary solutions to the
Einstein-Euler equations which have a Newtonian limit. The proof of this result
is based on a symmetric hyperbolic formulation of the Einstein-Euler equations
which contains a singular parameter \ep = v_T/c where is a
characteristic velocity scale associated with the fluid and is the speed of
light. The symmetric hyperbolic formulation allows us to derive \ep
independent energy estimates on weighted Sobolev spaces. These estimates are
the main tool used to analyze the behavior of solutions in the limit \ep
\searrow 0.Comment: Differs slightly from the published versio
The Newtonian limit on cosmological scales
We establish the existence of a wide class of inhomogeneous relativistic
solutions to the Einstein-Euler equations that are well approximated on
cosmological scales by solutions of Newtonian gravity. Error estimates
measuring the difference between the Newtonian and relativistic solutions are
provided.Comment: This version agrees with the published on
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