Stabilizing relativistic fluids on spacetimes with non-accelerated expansion
arXiv:2002.02119 · doi:10.1007/s00220-020-03924-9
Abstract
We establish global regularity and stability for the irrotational relativistic Euler equations with equation of state , where , for small initial data in the expanding direction of FLRW spacetimes of the form $(\mathbb R\times\mathbb T^3,-d\tb^2+\tb^2δ_{ij} dx^i dx^j)$. This provides the first case of non-dust fluid stabilization by spacetime expansion where the expansion rate is of power law type but non-accelerated. In particular, the time integral of the inverse scale factor diverges as .
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