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• W2323193228 abstract "A phenomenological attempt at alleviating the so-called coincidence problem is to allow the dark matter and dark energy to interact. By assuming a specific class of coupled quintessence models, characterized by a constant interaction parameter $ϵ$, we investigate the precision in the measurements of the expansion rate $H(z)$ required by future experiments in order to detect a possible deviation from the standard $ensuremath{Lambda}mathrm{CDM}$ model ($ϵ=0$). We perform our analysis at two levels, namely, through Monte Carlo simulations based on $ϵmathrm{CDM}$ models, in which $H(z)$ samples with different accuracies are generated and through an analytic method that calculates the error propagation of $ϵ$ as a function of the error in $H(z)$. We show that our analytical approach traces simulations accurately and find that to detect an interaction using $H(z)$ data only, these must reach an accuracy better than 1%." @default.
• W2323193228 created "2016-06-24" @default.
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• W2323193228 date "2013-04-08" @default.
• W2323193228 modified "2023-09-25" @default.
• W2323193228 title "Probing interaction in the dark sector" @default.
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• W2323193228 doi "https://doi.org/10.1103/physrevd.87.087301" @default.
• W2323193228 hasPublicationYear "2013" @default.
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