Future global stability for relativistic perfect fluids with linear equations of state $p=K\rho$ where $1/3<K<1/2$

Abstract

We establish the future stability of nonlinear perturbations of a class of homogeneous solutions to the relativistic Euler equations with a linear equation of state $p=K\rho$ on exponentially expanding FLRW spacetimes for the equation of state parameter values $1/3<K<1/2$.

Comments typos corrected; agrees with the published version

References in corpus (1)

• Stabilizing relativistic fluids on spacetimes with non-accelerated expansion

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