Friedmann-Robertson-Walker models do not require zero active mass

preprint2016arXivOpen access

Abstract

The Rh=ctR_h = ct cosmological model has received considerable attention in recent years owing to claims that it is favoured over the standard ΛΛ cold dark matter (ΛΛCDM) model by most observational data. A key feature of the Rh=ctR_h = ct model is that the zero active mass condition ρ+3p=0ρ+ 3p = 0 holds at all epochs. Most recently, Melia has claimed that this condition is a requirement of the symmetries of the Friedmann-Robertson-Walker (FRW) spacetime. We demonstrate that this claim is false and results from a flaw in the logic of Melia's argument.

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