The Rh=ctR_{\mathrm{h}}=ct universe and quintessence

preprint2016arXivOpen access

Abstract

Over the last few years the Rh=ctR_{\mathrm{h}}=ct universe has received a lot of attention, particularly when observational evidence seems to favor this over the standard ΛΛ cold dark matter (ΛCDMΛCDM) universe. Like the ΛCDMΛCDM, the Rh=ctR_{\mathrm{h}}=ct universe is based on a Friedmann-Robertson-Walker (FRW) cosmology where the total energy density ρρ and pressure pp of the cosmic fluid contain a dark energy component besides the usual (dark and baryonic) matter and radiation components. However unlike the ΛCDMΛCDM this model has the simple equation of state (EOS) ρ+3p=0ρ+ 3p = 0, i.e., its total active gravitational mass vanishes, which would therefore exclude a cosmological constant as the source of its dark energy component. Faced with this issue, in this paper we examine various possible sources for the dark energy component of the Rh=ctR_{\mathrm{h}}=ct universe and show that quintessence which has been used in other various dynamical dark energy models could also be a possible source in this case.

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