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- W3121752101 abstract "We investigate the prospects for determining the accelerating history of the Universe from upcoming measurements of the expansion rate $H(z)$. In our analyses, we use Monte Carlo simulations based on $w$CDM models to generate samples with different characteristics and calculate the evolution of the deceleration parameter $q(z)$. We show that a cosmographic (and, therefore, model-independent) evidence for cosmic acceleration ($q(z<z_t) < 0$, where $z_t$ is the transition redshift) will only be possible with an accuracy in $H(z)$ data greater than the expected in current planned surveys. A brief discussion about the prospects for reconstructing the dark energy equation of state from the parameters $H(z)$ and $q(z)$ is also included." @default.
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- W3121752101 date "2011-09-26" @default.
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- W3121752101 title "Cosmography and cosmic acceleration" @default.
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- W3121752101 doi "https://doi.org/10.1111/j.1365-2966.2011.19603.x" @default.
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